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Publications

To acknowledge the support by DFG within the priority program SPP 1992 please add the following acknowledgement to your publications:

XX acknowledges the support of the DFG priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets (XX XXXX/XX)”

Current number of publications: 244

Year
  • 2018
  • 2019
  • 2020
  • 2021
  • 2022
  1. K. Herbst, L. R. Baalmann, A. Bykov, N. Engelbrecht, S. E. S. Ferreira, V. V. Izmodenov, S. D. Korolkov, K. P. Levenfish, J. L. Linsky, D. M. -A. Meyer, K. Scherer, R. Du Toit Strauss

    Astrospheres of Planet-Hosting Cool Stars and Beyond ⋅ When Modeling Meets Observations

    DOI
  2. L. M. Serrano, D. Gandolfi, A. J. Mustill, O. Barragán, J. Korth, F. Dai, S. Redfield, M. Fridlund, K. W. F. Lam, M. R. Díaz, S. Grziwa, K. A. Collins, J. H. Livingston, W. D. Cochran, C. Hellier, S. E. Bellomo, T. Trifonov, F. Rodler, J. Alarcon, J. M. Jenkins, D. W. Latham, G. Ricker, S. Seager, R. Vanderspek, J. N. Winn, S. Albrecht, K. I. Collins, S. Csizmadia, T. Daylan, H. J. Deeg, M. Esposito, M. Fausnaugh, I. Georgieva, E. Goffo, E. W. Guenther, A. P. Hatzes, S. B. Howell, E. L. N. Jensen, R. Luque, A. W. Mann, F. Murgas, H. L. M. Osborne, E. Pallé, C. M. Persson, P. Rowden, A. Rudat, A. M. S. Smith, J. D. Twicken, V. Van Eylen, C. Ziegler

    A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system

  3. E. V. Turtelboom, L. M. Weiss, C. D. Dressing, G. Nowak, E. Pallé, C. Beard, S. Blunt, C. Brinkman, A. Chontos, Z. R. Claytor, F. Dai, P. A. Dalba, S. Giacalone, E. Gonzales, C. K. Harada, M. L. Hill, R. Holcomb, J. Korth, J. Lubin, T. Masseron, M. Macdougall, A. W. Mayo, T. Močnik, J. M. Akana Murphy, A. S. Polanski, M. Rice, R. A. Rubenzahl, N. Scarsdale, K. G. Stassun, D. B. Tyler, J. Van Zandt, I. Crossfield, H. J. Deeg, B. Fulton, D. Gandolfi, A. W. Howard, D. Huber, H. Isaacson, S. R. Kane, K. W. F. Lam, R. Luque, E. L. Martín, G. Morello, J. Orell-Miquel, E. A. Petigura, P. Robertson, A. Roy, V. Van Eylen, D. Baker, A. A. Belinski, A. Bieryla, D. R. Ciardi, K. A. Collins, N. Cutting, D. J. Della-Rose, T. B. Ellingsen, E. Furlan, T. Gan, C. L. Gnilka, P. Guerra, S. B. Howell, M. Jimenez, D. W. Latham, M. Larivière, K. V. Lester, J. Lillo-Box, L. Luker, C. R. Mann, P. Plavchan, B. Safonov, B. Skinner, I. A. Strakhov, J. Wittrock, D. Caldwell, Z. Essack, J. M. Jenkins, E. V. Quintana, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn

    The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246

  4. P. Schöfer, S. V. Jeffers, A. Reiners, M. Zechmeister, B. Fuhrmeister, M. Lafarga, I. Ribas, A. Quirrenbach, P. J. Amado, J. A. Caballero, G. Anglada-Escudé, F. F. Bauer, V. J. S. Béjar, M. Cortés-Contreras, E. Díez Alonso, S. Dreizler, E. W. Guenther, O. Herbort, E. N. Johnson, A. Kaminski, M. Kürster, D. Montes, J. C. Morales, S. Pedraz, L. Tal-Or

    The CARMENES search for exoplanets around M dwarfs. Rotational variation in activity indicators of Ross 318, YZ CMi, TYC 3529-1437-1, and EV Lac

  5. N. Engelbrecht, A. Vogt, K. Herbst, R. Du Toit Strauss, R. A. Burger

    Revisiting the Revisited Palmer Consensus: New Insights from Jovian Electron Transport

    bib

    @article{Engelbrecht_2022,
    doi = {10.3847/1538-4357/ac58f5},
    url = {https://doi.org/10.3847/1538-4357/ac58f5},
    year = 2022,
    month = {apr},
    publisher = {American Astronomical Society},
    volume = {929},
    number = {1},
    pages = {8},
    author = {N. Eugene Engelbrecht and Adrian Vogt and Konstantin Herbst and R. Du Toit Strauss and R. A. Burger},
    title = {Revisiting the Revisited Palmer Consensus: New Insights from Jovian Electron Transport},
    journal = {The Astrophysical Journal},
    abstract = {Novel insights into the behavior of the diffusion coefficients of charged particles in the inner heliosphere are of great importance to any study of the transport of these particles and are especially relevant with regard to the transport of low-energy electrons. The present study undertakes an exhaustive investigation into the diffusion parameters needed to reproduce low-energy electron intensities as observed at Earth, using a state-of-the-art 3D cosmic ray transport code. To this end, the transport of Jovian electrons is considered, as Jupiter represents the predominant source of these particles in the inner heliosphere, and because a careful comparison of model results with observations taken during periods of good and poor magnetic connectivity between Earth and Jupiter allows for conclusions to be drawn as to both parallel and perpendicular diffusion coefficients. This study then compares these results with the predictions made by various scattering theories. Best-fit parameters for parallel and perpendicular mean free paths at 1 au fall reasonably well within the span of observational values reported by previous studies, but best-fit radial and rigidity dependences vary widely. However, a large number of diffusion parameters lead to reasonable to-good fits to observations, and it is argued that considerable caution must be exercised when comparing theoretical results for diffusion coefficients with diffusion parameters calculated from particle transport studies.}
    }

    DOI
  6. H. Q. Tran, P. B. Bowler, M. Endl, W. D. Cochran, P. J. MacQueen, D. Gandolfi, C. M. Persson, M. Fridlund, E. Pallé, G. Nowak, H. J. Deeg, R. Luque, J. H. Livingston, P. Kabáth, J. Laskar, J. Subjak, S. B. Howell, S. H. Albrecht, K. A. Collins, M. Esposito, S. Grziwa, V. Van Eylen, E. Goffo, C. Huang, J. M. Jenkins, M. Karjalainen, R. Karjalainen, E. Knudstrup, J. Korth, K. W. F. Lam, D. W. Latham, A. Levine, H. L. M. Osborne, S. N. Quinn, S. Redfield, G. R. Ricker, S. Seager, L. M. Serrano, A. M. S. Smith, J. D. Twicken, J. N. Winn

    TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

  7. J. Mah, R. Brasser, J. M. Y. Woo, A. Bouvier, S. J. Mojzsis

    Evidence of a primordial isotopic gradient in the inner region of the solar protoplanetary disc

  8. A. Krieger, S. Wolf

    Feasibility of detecting and characterizing embedded low-mass giant planets in gaps in the VIS/NIR wavelength range

  9. A. P. Hatzes, D. Gandolfi, J. Korth, F. Rodler, S. Sabotta, M. Esposito, O. Barragán, J. H. Livingston, V. Van Eylen, L. M. Serrano, R. Luque, A. M. S. Smith, S. Redfield, C. M. Persson, E. Pallé, M. Paetzold, G. Nowak, H. L. M. Osborne, N. Narita, S. Mathur, K. W. F. Lam, P. Kabáth, M. C. Johnson, E. W. Guenther, S. Grziwa, E. Goffo, M. Fridlund, M. Endl, H. J. Deeg, Sz. Csizmadia, W. D. Cochran, L. González-Cuesta, P. Chaturvedi, I. Carleo, J. Cabrera, P. G. Beck, S. Albrecht

    A Radial Velocity Study of the Planetary System of Pi Mensae: Improved Planet Parameters for PI Mensae c and a Third Planet on a 125-d Orbit

  10. K. Stock, D. Veras, M. X. Cai, R. Spurzem, S. Portegies Zwart

    Birth cluster simulations of planetary systems with multiple super-Earths: initial conditions for white dwarf pollution drivers

  11. J. Kemmer, S. Dreizler, D. Kossakowski, S. Stock, A. Quirrenbach, J. A. Caballero, P. J. Amado, K. A. Collins, N. Espinoza, E. Herrero, J. M. Jenkins, D. W. Latham, J. Lillo-Box, N. Narita, E. Pallé, A. Reiners, I. Ribas, G. Ricker, E. Rodríguez, S. Seager, R. Vanderspek, R. Wells, J. Winn, F. J. Aceituno, V. J. S. Béjar, T. Barclay, P. Bluhm, P. Chaturvedi, C. Cifuentes, K. I. Collins, M. Cortés-Contreras, B. O. Demory, M. Fausnaugh, Y. Gómez Maqueo Chew, D. Galadí-Enríquez, T. Gan, M. Gillon, A. Golovin, A. P. Hatzes, Th. Henning, C. Huang, S. V. Jeffers, A. Kaminski, M. Kunimoto, M. Kürster, M. J. López-González, M. Lafarga, R. Luque, J. McCormac, K. Molaverdikhani, D. Montes, J. C. Morales, V. M. Passegger, S. Reffert, L. Sabin, P. Schöfer, N. Schanche, M. Schlecker, U. Schroffenegger, R. P. Schwarz, A. Schweitzer, A. Sota, P. Tenenbaum, T. Trifonov, S. Vanaverbeke, M. Zechmeister

    Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b

  12. V. Wolthoff, S. Reffert, A. Quirrenbach, M. I. Jones, R. A. Wittenmyer, J. S. Jenkins

    Precise radial velocities of giant stars XVI. Planet occurrence rates from the combined analysis of the Lick, EXPRESS, and PPPS giant star surveys

  13. B. Ercolano, C. Rab, K. Molaverdikhani, B. Edwards, T. Preibisch, L. Testi, I. Kamp, W. -F. Thi

    Observations of PAHs in the atmospheres of discs and exoplanets

    bib

    @article{10.1093/mnras/stac505,
    author = {Ercolano, Barbara and Rab, Christian and Molaverdikhani, Karan and Edwards, Billy and Preibisch, Thomas and Testi, Leonardo and Kamp, Inga and Thi, Wing-Fai},
    title = "{Observations of PAHs in the atmospheres of discs and exoplanets}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {512},
    number = {1},
    pages = {430-438},
    year = {2022},
    month = {02},
    abstract = "{Polycyclic aromatic hydrocarbons (PAHs) play a key role in the chemical and hydrodynamical evolution of the atmospheres of exoplanets and planet-forming discs. If they can survive the planet formation process, PAHs are likely to be involved in pre-biotic chemical reactions eventually leading to more complex molecules such as amino acids and nucleotides, which form the basis for life as we know it. However, the abundance and specific role of PAHs in these environments is largely unknown due to limitations in sensitivity and range of wavelength of current and previous space-borne facilities. Upcoming infrared space spectroscopy missions, such as Twinkle and Ariel, present a unique opportunity to detect PAHs in the atmospheres of exoplanets and planet-forming discs. In this work, we present synthetic observations based on conservative numerical modelling of typical planet-forming discs and a transiting hot Saturnian planet around solar-type star. Our models show that Twinkle and Ariel might both be able to detect the 3.3 \\$\\mu\\$m PAH feature within reasonable observing time in discs and transiting planets, assuming that PAHs are present with an abundance of at least one-tenth of the interstellar medium value.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac505},
    url = {https://doi.org/10.1093/mnras/stac505},
    eprint = {https://academic.oup.com/mnras/article-pdf/512/1/430/42897794/stac505.pdf},
    }

    DOI arXiv
  14. T.W. Moldenhauer, R. Kuiper, W. Kley, C. W. Ormel

    Recycling of the first atmospheres of embedded planets: Dependence on core mass and optical depth

  15. J. Subjak, M. Endl, P. Chaturvedi, R. Karjalainen, W. D. Cochran, M. Esposito, D. Gandolfi, K. W. F. Lam, K. G. Stassun, J. Žák, N. Lodieu, H. M. J. Boffin, P. J. MacQueen, A. P. Hatzes, E. W. Guenther, I. Georgieva, S. Grziwa, H. Schmerling, M. Skarka, M. Blažek, M. Karjalainen, M. Špoková, H. Isaacson, A. W. Howard, C. Burke, V. Van Eylen, M. C. V. Fridlund, E. Goffo, B. Falk, J. M. Jenkins, J. Korth, J. J. Lissauer, J. H. Livingston, R. Luque, A. Muresan, H. P. Osborn, E. Pallé, C. M. Persson, S. Redfield, G. R. Ricker, S. Seager, L. M. Serrano, A. M. S. Smith, P. Kabáth

    TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet

  16. N. Davari, R. Capuzzo-Dolcetta, R. Spurzem

    Stability of planetary systems within the S-star cluster: the Solar system analogues

    bib

    @article{10.1093/mnras/stac462,
    author = {Davari, N and Capuzzo–Dolcetta, R and Spurzem, R},
    title = "{Stability of planetary systems within the S-star cluster: the Solar system analogues}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    year = {2022},
    month = {02},
    abstract = "{A dynamically relaxed dense cluster comprised of about 40 stars (the so-called S-stars) inhabits the central region of the Galaxy. Their stars revolve around the Sgr A* massive object. To understand the dynamical evolution of planetary systems in a particular environment like that around Sgr A*, we carry out direct N–body simulations of planetary systems embedded in the S–star cluster. In this work, we investigate the short-term stability of the planets orbiting around S-stars after their close interactions with the central massive black hole of our galaxy. We find that planetary systems go through encounters with the SMBH and the nearby stars. We determine the frequency and the strength of planetary systems’ encounters with the nearby stars as these encounters remarkably increase for systems assigned to S-stars closer to the SMBH. The SMBH severely destabilizes the planetary systems, though we noted that the small oscillations in the mutual eccentricity and inclination of the planetary system could be caused by the planet–planet coupling and the near-resonance effect between the two planets. We obtain estimates of the fraction of survivor planets (\\$\\sim 51\\\\%\\$), and find that planets stripped from their hosting star are generally captured on close orbits around Sgr A*. We notify while gas giants are tidally disrupted, terrestrial planets do not. We estimate that Sgr A* flares can be due to the tidal disruption events of starless giant planets.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac462},
    url = {https://doi.org/10.1093/mnras/stac462},
    note = {stac462},
    eprint = {https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac462/42549403/stac462.pdf},
    }

    DOI arXiv
  17. A. Papaioannou, A. Kouloumvakos, A. Mishev, R. Vainio, K. Herbst, I. Usoskin, A. P. Rouillard, A. Anastasiadis, R. Wimmer-Schweingruber, J. Gieseler, P. Kühl

    The First Ground Level Enhancement of Solar Cycle 25 on 28 October 2021

  18. J. Eberhardt, T. Trifonov, M. Kürster, S. Stock, Th. Henning, A. Wollbold, S. Reffert, M. H. Lee, M. Zechmeister, F. Rodler, O. Zakhozhay, P. Heeren, D. Gandolfi, O. Barragán, M. Tala-Pinto, V. Wolthoff, P. Sarkis, S. S. Brems

    Dynamical architecture of the HD 107148 system

  19. E. González-Álvarez, M. R. Zapatero Osorio, J. Sanz-Forcada, J. A. Caballero, S. Reffert, V. J. S. Béjar, A. P. Hatzes, E. Herrero, S. V. Jeffers, J. Kemmer, M. J. López-González, R. Luque, K. Molaverdikhani, G. Morello, E. Nagel, A. Quirrenbach, E. Rodríguez, C. Rodríguez López, M. Schlecker, A. Schweitzer, S. Stock, V. M. Passegger, T. Trifonov, P. J. Amado, D. Baker, P. T. Boyd, C. Cadieux, D. Charbonneau, K. A. Collins, R. Doyon, S. Dreizler, N. Espinoza, G. Fűrész, E. Furlan, K. Hesse, S. B. Howell, J. M. Jenkins, R. C. Kidwell, D. W. Latham, K. K. McLeod, D. Montes, J. C. Morales, T. O'Dwyer, S. Pedraz, A. Reiners, I. Ribas, S. N. Quinn, C. Schnaible, S. Seager, B. Skinner, J. C. Smith, R. P. Schwarz, A. Shporer, R. Vanderspek, J. N. Winn

    A multi-planetary system orbiting the early-M dwarf TOI-1238

  20. J. L. Grenfell, F. Wunderlich, M. Sinnhuber, K. Herbst, R. Lehmann, M. Scheucher, S. Gebauer, G. Arnold, H. Rauer

    Atmospheric processes affecting methane on Mars

  21. T. N. Delage, S. Okuzumi, M. Flock, P. Pinilla, N. Dzyurkevich

    Steady-state accretion in magnetized protoplanetary disks

  22. M. Rengel, D. Shulyak, P. Hartogh, H. Sagawa, R. Moreno, C. Jarchow, D. Breitschwerdt

    Ground-based HCN submillimetre measurements in Titan’s atmosphere: an intercomparison with Herschel observations

  23. O. Voelkel, H. Klahr, C. Mordasini, A. Emsenhuber

    On the multiple generations of planetary embryos

  24. R. Bischoff, St. Raetz, M. Fernández, R. Neuhäuser, M. Mugrauer, C. Huang, W. P. Chen, A. Sota, J. Jiménez Ortega, V. V. Hambaryan, P. Zieliński, M. Dróżdż, W. Ogloza, W. Stenglein, E. Hohmann, K. -U. Michel

    Young Exoplanet Transit Initiative follow-up observations of the T Tauri star CVSO 30 with transit-like dips

    bib

    @article{10.1093/mnras/stac293,
    author = {Bischoff, R and Raetz, St and Fernández, M and Mugrauer, M and Neuhäuser, R and Huang, P C and Chen, W P and Sota, A and Jiménez Ortega, J and Hambaryan, V V and Zieliński, P and Dróżdż, M and Ogłoza, W and Stenglein, W and Hohmann, E and Michel, K-U},
    title = "{Young Exoplanet Transit Initiative follow-up observations of the T Tauri star CVSO 30 with transit-like dips}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {3},
    pages = {3487-3500},
    year = {2022},
    month = {02},
    abstract = "{The T Tauri star CVSO 30, also known as PTFO 8-8695, was studied intensively with ground-based telescopes as well as with satellites over the last decade. It showed a variable light curve with additional repeating planetary transit-like dips every ∼10.8 h. However, these dimming events changed in depth and duration since their discovery and from autumn 2018 on, they were not even present or near the predicted observing times. As reason for the detected dips and their changes within the complex light curve, e.g. a disintegrating planet, a circumstellar dust clump, stellar spots, possible multiplicity, and orbiting clouds at a Keplerian co-rotating radius were discussed and are still under debate. In this paper, we present additional optical monitoring of CVSO 30 with the meter class telescopes of the Young Exoplanet Transit Initiative in Asia and Europe over the last 7 yr and characterize CVSO 30 with the new Early Data Release 3 of the European Space Agency-Gaia mission. As a result, we describe the evolution of the dimming events in the optical wavelength range since 2014 and present explanatory approaches for the observed variabilities. We conclude that orbiting clouds of gas at a Keplerian co-rotating radius are the most promising scenario to explain most changes in CVSO 30’s light curve.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac293},
    url = {https://doi.org/10.1093/mnras/stac293},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/3/3487/42571812/stac293.pdf},
    }

    DOI arXiv
  25. D. Mesa, C. Ginski, R. Gratton, S. Ertel, K. Wagner, M. Bonavita, D. Fedele, M. Meyer, T. Henning, M. Langlois, A. Garufi, S. Antoniucci, R. Claudi, D. Defrère, S. Desidera, M. Janson, N. Pawellek, E. Rigliaco, V. Squicciarini, A. Zurlo, A. Boccaletti, M. Bonnefoy, F. Cantalloube, G. Chauvin, M. Feldt, J. Hagelberg, E. Hugot, A. M. Lagrange, C. Lazzoni, D. Maurel, C. Perrot, C. Petit, D. Rouan, A. Vigan

    Signs of late infall and possible planet formation around DR Tau using VLT/SPHERE and LBTI/LMIRCam

  26. E. W. Guenther

    The impact of faculae on the radius determination of exoplanets: the case of the M-star GJ 1214

    bib

    @article{10.1093/mnras/stac108,
    author = {Guenther, Eike W},
    title = "{The impact of faculae on the radius determination of exoplanets: the case of the M-star GJ 1214}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {1},
    pages = {1115-1120},
    year = {2022},
    month = {01},
    abstract = "{Precise measurements of exoplanets radii are of key importance for our understanding of the origin and nature of these objects. Measurement of the planet radii using the transit method has reached a precision that the effects of stellar surface features have to be taken into account. While the effects from spots have already been studied in detail, our knowledge of the effects caused by faculae is still limited. This is particularly the case for M-stars. Faculae can pose a problem if they are inhomogeneously distributed on the stellar surface. Using the eclipse mapping method, we study the distribution of the faculae on the surface of GJ 1214 using the Ca ii H\\&K lines as tracers. In order to assess the homogeneity of the distribution in a quantitative way, we introduce the inhomogeneity factor (IHF). IHF is 0 per cent if the distribution is homogeneous, positive, if the plage regions are preferentially located along the path of the planet, and negative, if they are preferentially located outside the path of the planet. For GJ 1214, we derive a rather small value of \\$\\rm IHF=7.7\_\\{-7.7\\}^\\{+12.0\\}\\{\\{\\ \\rm per\\ cent\\}\\}\\$. We discuss the relevance of this result in the context of the PLATO and ARIEL missions.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac108},
    url = {https://doi.org/10.1093/mnras/stac108},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/1/1115/42385991/stac108.pdf},
    }

    DOI arXiv
  27. S. Boro Saikia, T. Lueftinger, C. P. Folsom, A. Antonova, E. Alecian, S.-F. Donati, M. Guedel, J. C. Hall, S. V. Jeffers, O. Kochukhov, S. C. Marsden, Y. T. Metodieva, M. Mittag, J. Morin, V. Perdelwitz, P. Petit, M. Schmid, A. A. Vidotto

    Time evolution of magnetic activity cycles in young suns: The curious case of κ Ceti

  28. D. Ó Fionnagáin, R. D. Kavanagh, A. A. Vidotto, S. V. Jeffers, P. Petit, S. Marsden, J. Morin, A. Golden

    Coronal Mass Ejections and Type II Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani

    bib

    @article{_Fionnag_in_2022,
    doi = {10.3847/1538-4357/ac35de},
    url = {https://doi.org/10.3847/1538-4357/ac35de},
    year = 2022,
    month = {jan},
    publisher = {American Astronomical Society},
    volume = {924},
    number = {2},
    pages = {115},
    author = {D{\'{u}}alta {\'{O}} Fionnag{\'{a}}in and Robert D. Kavanagh and Aline A. Vidotto and Sandra V. Jeffers and Pascal Petit and Stephen Marsden and Julien Morin and Aaron Golden},
    title = {Coronal Mass Ejections and Type {II} Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani},
    journal = {The Astrophysical Journal},
    abstract = {We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of ϵ Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and 2013, and estimate the radio emission frequencies associated with these events. These stellar eruptions have proven to be elusive, although a promising approach to detect and characterize these phenomena are low-frequency radio observations of potential type II bursts as CME-induced shocks propagate through the stellar corona. Stellar type II radio bursts are expected to emit below 450 MHz, similarly to their solar counterparts. We show that the length of time these events remain above the ionospheric cutoff is not necessarily dependent on the stellar magnetic cycle, but more on the eruption location relative to the stellar magnetic field. We find that these type II bursts would remain within the frequency range of LOFAR for a maximum of 20–30 minutes post-eruption for the polar CMEs (50 minutes for second harmonics). We find evidence of slower equatorial CMEs, which result in slightly longer observable windows for the 2008 and 2013 simulations. Stellar magnetic geometry and strength have a significant effect on the detectability of these events. We place the CMEs in the context of the stellar mass-loss rate (27–48× solar mass-loss rate), showing that they can amount to 3%–50% of the stellar wind mass-loss rate for ϵ Eridani. Continuous monitoring of likely stellar CME candidates with low-frequency radio telescopes will be required to detect these transient events.}
    }

    DOI arXiv
  29. D. Cont, F. Yan, A. Reiners, L. Nortmann, K. Molaverdikhani, M. Stangret, Th. Henning, I. Ribas, A. Quirrenbach, J. A. Caballero, M. R. Zapatero Osorio, P. J. Amado, J. Aceituno, N. Casasayas-Barris, S. Czesla, A. Kaminski, M. López-Puertas, D. Montes, J. C. Morales, G. Morello, E. Nagel, A. Sánchez-López, E. Sedaghati, M. Zechmeister

    Silicon in the dayside atmospheres of two ultra-hot Jupiters

  30. A. Vogt, N. Engelbrecht, N. Eugene, B. Heber, A. Kopp, K. Herbst

    Numerical and experimental evidence for a new interpretation of residence times in space

  31. J. Mah, R. Brasser, A. Bouvier, S. J. Mojzsis

    Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar system

    bib

    @article{10.1093/mnras/stab3766,
    author = {Mah, J and Brasser, R and Bouvier, A and Mojzsis, S J},
    title = "{Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar system}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {1},
    pages = {158-175},
    year = {2021},
    month = {12},
    abstract = "{Recent work has shown that aside from the classical view of collisions by increasingly massive planetesimals, the accretion of mm to m-sized ‘pebbles’ can also reproduce the mass–orbit distribution of the terrestrial planets. Here, we perform N-body simulations to study the effects of pebble accretion on to growing planetesimals of different diameters located in the inner Solar system. The simulations are run to occur during the lifetime of the gas disc while also simultaneously taking Jupiter’s growth into account. We find that pebble accretion can increase the mass in the solid disc by at least a few times its initial mass with reasonable assumptions that pebbles fragment to smaller sized grains at the snow line and that gas-disc-induced orbital migration effects are in force. Such a large contribution in mass by pebbles would seem to imply that the isotopic composition of the inner Solar system should be similar to the pebble source (i.e. outer Solar system). This implication appears to violate the observed nucleosynthetic isotopic dichotomy of the sampled Solar system. Thus, pebble accretion played little or no role in terrestrial planet formation.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab3766},
    url = {https://doi.org/10.1093/mnras/stab3766},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/1/158/42362609/stab3766.pdf},
    }
    author={Mah, J and Brasser, R and Bouvier, A and Mojzsis, S J},
    year={2021},
    month={Dec},
    pages={158–175} }

    DOI arXiv
  32. G.-D. Marleau, Y. Aoyama, R. Kuiper, K. Follette, N. J. Turner, G. Cugno, C. F. Manara, S. Y. Haffert, D. Kitzmann, S. C. Ringqvist, K. R. Wagner, R. van Boekel, S. Sallum, M. Janson, T. O. B. Schmidt, L. Venuti, C. Lovis, C. Mordasini

    Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H α

  33. K. A. Rybicki, L. Wyrzykowski, E. Bachelet, A. Cassan, P. Zieliński, A. Gould, S. Calchi Novati, J. C. Yee, Y. H. Ryu, M. Gromadzki, P. Mikolajczyk, N. Ihanec, K. Kruszyńska, F. J. Hambsch, S. Zola, S. J. Fossey, S. Awiphan, N. Nakharutai, F. Lewis, E. F. Olivares, S. Hodgkin, A. Delgado, E. Breedt, D. L. Harrison, M. van Leeuwen, G. Rixon, T. Wevers, A. Yoldas, A. Udalski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, J. Skowron, R. Poleski, K. Ulaczyk, P. Mróz, P. Iwanek, M. Wrona, R. A. Street, Y. Tsapras, M. Hundertmark, M. Dominik, C. Beichman, G. Bryden, S. Carey, B. S. Gaudi, C. Henderson, Y. Shvartzvald, W. Zang, W. Zhu, G. Christie, J. Green, S. Hennerley, J. McCormick, L. A. G. Monard, T. Natusch, R. W. Pogge, I. Gezer, A. Gurgul, Z. Kaczmarek, M. Konacki, M. C. Lam, M. Maskoliunas, E. Pakštienė, M. Ratajczak, A. Stankevičiutė, J. Zdanavičius, O. Ziólkowska

    Single-lens mass measurement in the high-magnification microlensing event Gaia19bld located in the Galactic disc

  34. E. Bachelet, P. Zieliński, M. Gromadzki, I. Gezer, K. A. Rybicki, K. Kruszyńska, N. Ihanec, L. Wyrzykowski, R. A. Street, Y. Tsapras, M. Hundertmark, A. Cassan, D. Harbeck, M. Rabus

    A spectroscopic follow-up for Gaia19bld

  35. E. Marfil, H. M. Tabernero, D. Montes, J. A. Caballero, F. J. Lázaro, J. I. González Hernández, E. Nagel, V. M. Passegger, A. Schweitzer, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, C. Cifuentes, M. Cortés-Contreras, S. Dreizler, C. Duque-Arribas, D. Galadí-Enríquez, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, Á. López-Gallifa, J. C. Morales, Y. Shan, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Stellar atmospheric parameters of target stars with SteParSyn

  36. M. Küffmeier, C. P. Dullemond, S. Reissl, F. G. Goicovic

    Misaligned disks induced by infall

  37. S. Khalafinejad, K. Molaverdikhani, J. Blecic, M. Mallonn, L. Nortmann, J. A. Caballero, H. Rahmati, A. Kaminski, S. Sadegi, E. Nagel, L. Carone, P. J. Amado, M. Azzaro, F. F. Bauer, N. Casasayas-Barris, S. Czesla, C. von Essen, L. Fossati, M. Guedel, Th. Henning, M. López-Puertas, M. Lendl, T. Lueftinger, D. Montes, M. Oshagh, A. Quirrenbach, E. Pallé, S. Reffert, A. Reiners, I. Ribas, S. Stock, F. Yan, M. R. Zapatero Osorio, M. Zechmeister

    Probing the atmosphere of WASP-69 b with low- and high-resolution transmission spectroscopy

  38. D. Kossakowski, J. Kemmer, P. Bluhm, S. Stock, J. A. Caballero, V. J. S. Béjar, C. Cardona Guillén, N. Lodieu, K. A. Collins, M. Oshagh, M. Schlecker, N. Espinoza, E. Pallé, Th. Henning, L. Kreidberg, M. Kürster, P. J. Amado, D. R. Anderson, J. C. Morales, S. Cartwright, D. Charbonneau, P. Chaturvedi, C. Cifuentes, D. M. Conti, M. Cortés-Contreras, S. Dreizler, D. Galadí-Enríquez, P. Guerra, R. Hart, C. Hellier, C. Henze, E. Herrero, S. V. Jeffers, J. M. Jenkins, E. L. N. Jensen, A. Kaminski, J. Kielkopf, M. Kunimoto, M. Lafarga, D. W. Latham, J. Lillo-Box, R. Luque, K. Molaverdikhani, D. Montes, G. Morello, E. H. Morgan, G. Nowak, A. Pavlov, M. Perger, E. V. Quintana, A. Quirrenbach, S. Reffert, A. Reiners, G. Ricker, I. Ribas, C. Rodríguez López, M. R. Zapatero Osorio, S. Seager, P. Schöfer, A. Schweitzer, T. Trifonov, S. Vanaverbeke, R. Vanderspek, R. West, J. Winn, M. Zechmeister

    TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf

  39. M. Janson, R. Gratton, L. Rodet, A. Vigan, M. Bonnefoy, P. Delorme, E. E. Mamajek, S. Reffert, L. Stock, G.-D. Marleau, M. Langlois, G. Chauvin, S. Desidera, S. C. Ringqvist, L. Mayer, G. Viswanath, V. Squicciarini, M. R. Meyer, M. Samland, S. Petrus, R. Helled, M. Kenworthy, S. P. Quanz, B. Biller, T. Henning, D. Mesa, N. Engler, J. C. Carson

    A wide-orbit giant planet in the high-mass b Centauri binary system

  40. A. Cassan, C. Ranc, O. Absil, L. Wyrzykowski, K. A. Rybicki, E. Bachelet, J. -B. Le Bouquin, M. Hundertmark, R. Street, J. Surdej, Y. Tsapras, J. Wambsganss, O. Wertz

    Microlensing mass measurement from images of rotating gravitational arcs

    DOI
  41. T. Stolker, S. Y. Haffert, A. Y. Kesseli, R. G. van Holstein, Y. Aoyama, J. Brinchmann, G. Cugno, J. H. Girard, G.-D. Marleau, M. R. Meyer, J. Milli, S. P. Quanz, I. A. G. Snellen, K. O. Todorov

    Characterizing the Protolunar Disk of the Accreting Companion GQ Lupi B

    bib

    @article{Stolker_2021,
    doi = {10.3847/1538-3881/ac2c7f},
    url = {https://doi.org/10.3847/1538-3881/ac2c7f},
    year = 2021,
    month = {dec},
    publisher = {American Astronomical Society},
    volume = {162},
    number = {6},
    pages = {286},
    author = {Tomas Stolker and Sebastiaan Y. Haffert and Aurora Y. Kesseli and Rob G. van Holstein and Yuhiko Aoyama and Jarle Brinchmann and Gabriele Cugno and Julien H. Girard and Gabriel-Dominique Marleau and Michael R. Meyer and Julien Milli and Sascha P. Quanz and Ignas A. G. Snellen and Kamen O. Todorov},
    title = {Characterizing the Protolunar Disk of the Accreting Companion {GQ} Lupi B{\ast}},
    journal = {The Astronomical Journal},
    abstract = {GQ Lup B is a young and accreting, substellar companion that appears to drive a spiral arm in the circumstellar disk of its host star. We report high-contrast imaging observations of GQ Lup B with VLT/NACO at 4–5 μm and medium-resolution integral field spectroscopy with VLT/MUSE. The optical spectrum is consistent with an M9 spectral type, shows characteristics of a low-gravity atmosphere, and exhibits strong Hα emission. The H − M′ color is ≳1 mag redder than field dwarfs with similar spectral types, and a detailed analysis of the spectral energy distribution (SED) from optical to mid-infrared wavelengths reveals excess emission in the L′, NB4.05, and M′ bands. The excess flux is well described by a blackbody component with T disk ≈ 460 K and R disk ≈ 65 R J and is expected to trace continuum emission from small grains in a protolunar disk. We derive an extinction of A V ≈ 2.3 mag from the broadband SED with a suspected origin in the vicinity of the companion. We also combine 15 yr of astrometric measurements and constrain the mutual inclination with the circumstellar disk to 84 ± 9 deg, indicating a tumultuous dynamical evolution or a stellar-like formation pathway. From the measured Hα flux and the estimated companion mass, M p ≈ 30 M J, we derive an accretion rate of . We speculate that the disk is in a transitional stage in which the assembly of satellites from a pebble reservoir has opened a central cavity while GQ Lup B is in the final stages of its formation.}
    }

    DOI arXiv
  42. K. W. F. Lam, Sz. Csizmadia, N. Astudillo-Defru, X. Bonfils, D. Gandolfi, Sebastiano Padovan, M. Esposito, C. Hellier, T. Hirano, J. Livingston, F. Murgas, A. M. S. Smith, K. A. Collins, S. Mathur, R. A. García, S. Howell, N. C. Santos, F. Dai, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, S. Albrecht, J. M. Almenara, E. Artigau, O. Barragán, F. Bouchy, J. Cabrera, D. Charbonneau, P. Chaturvedi, A. Chaushev, J. L. Christiansen, W. D. Cochran, X. Delfosse, R. F. Díaz, R. Doyon, P. Eigmüller, P. Figueira, T. Forveille, M. Fridlund, E. Goffo, I. Georgieva, S. Grziwa, E. W. Guenther, A. P. Hatzes, M. C. Johnson, P. Kabáth, E. Knudstrup, J. Korth, J. J. Lissauer, C. Lovis, R. Luque, R. Morris, N. Narita, H. Osborne, F. Pepe, C. M. Persson, S. N. Quinn, H. Rauer, S. Redfield, J. E. Schlieder, D. Ségransan, L. M. Serrano, J. C. Smith, J. Subjak, J. D. Twicken, S. Udry, V. Van Eylen, M. Vezie, J. R. de Meideiros, G. Gaisné, P. Lewin, C. Melo, E. H. Morgan, M. Mayor

    GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star

    bib

    @article{doi:10.1126/science.aay3253,
    author = {Kristine W. F. Lam and Szilárd Csizmadia and Nicola Astudillo-Defru and Xavier Bonfils and Davide Gandolfi and Sebastiano Padovan and Massimiliano Esposito and Coel Hellier and Teruyuki Hirano and John Livingston and Felipe Murgas and Alexis M. S. Smith and Karen A. Collins and Savita Mathur and Rafael A. Garcia and Steve B. Howell and Nuno C. Santos and Fei Dai and George R. Ricker and Roland Vanderspek and David W. Latham and Sara Seager and Joshua N. Winn and Jon M. Jenkins and Simon Albrecht and Jose M. Almenara and Etienne Artigau and Oscar Barragán and François Bouchy and Juan Cabrera and David Charbonneau and Priyanka Chaturvedi and Alexander Chaushev and Jessie L. Christiansen and William D. Cochran and José R. De Meideiros and Xavier Delfosse and Rodrigo F. Díaz and René Doyon and Philipp Eigmüller and Pedro Figueira and Thierry Forveille and Malcolm Fridlund and Guillaume Gaisné and Elisa Goffo and Iskra Georgieva and Sascha Grziwa and Eike Guenther and Artie P. Hatzes and Marshall C. Johnson and Petr Kabáth and Emil Knudstrup and Judith Korth and Pablo Lewin and Jack J. Lissauer and Christophe Lovis and Rafael Luque and Claudio Melo and Edward H. Morgan and Robert Morris and Michel Mayor and Norio Narita and Hannah L. M. Osborne and Enric Palle and Francesco Pepe and Carina M. Persson and Samuel N. Quinn and Heike Rauer and Seth Redfield and Joshua E. Schlieder and Damien Ségransan and Luisa M. Serrano and Jeffrey C. Smith and Ján Šubjak and Joseph D. Twicken and Stéphane Udry and Vincent Van Eylen and Michael Vezie },
    title = {GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star},
    journal = {Science},
    volume = {374},
    number = {6572},
    pages = {1271-1275},
    year = {2021},
    doi = {10.1126/science.aay3253},

    URL = {https://www.science.org/doi/abs/10.1126/science.aay3253},
    eprint = {https://www.science.org/doi/pdf/10.1126/science.aay3253}
    ,
    abstract = { The mass and radius of an exoplanet determine its mean density, which provides information about the possible interior structure. Lam et al. have identified a planet on a 7.7-hour orbit around a nearby red dwarf star. The authors determined the planet’s radius from the transit, then used radial velocity observations to measure the mass. They found a sub-Earth–sized planet with a density almost equivalent to pure iron. Its high surface temperature is close to the vaporization point of iron, suggesting that it is the iron core of a planet that has lost its outer mantle. —KTS The nearby exoplanet GJ 367b has a density consistent with pure iron. Ultrashort-period (USP) exoplanets have orbital periods shorter than 1 day. Precise masses and radii of USP exoplanets could provide constraints on their unknown formation and evolution processes. We report the detection and characterization of the USP planet GJ 367b using high-precision photometry and radial velocity observations. GJ 367b orbits a bright (V-band magnitude of 10.2), nearby, and red (M-type) dwarf star every 7.7 hours. GJ 367b has a radius of 0.718 ± 0.054 Earth-radii and a mass of 0.546 ± 0.078 Earth-masses, making it a sub-Earth planet. The corresponding bulk density is 8.106 ± 2.165 grams per cubic centimeter—close to that of iron. An interior structure model predicts that the planet has an iron core radius fraction of 86 ± 5\%, similar to that of Mercury’s interior. }
    }

    DOI arXiv
  43. A. M. S. Smith, S. N. Breton, Sz. Csizmadia, F. Dai, D. Gandolfi, R. A. García, A. W. Howard, H. Isaacson, J. Korth, K. W. F. Lam, S. Mathur, G. Nowak, F. Pérez Hernández, C. M. Persson, S. H. Albrecht, O. Barragán, J. Cabrera, W. D. Cochran, H. J. Deeg, M. Fridlund, I. Georgieva, E. Goffo, E. W. Guenther, A. P. Hatzes, P. Kabáth, J. H. Livingston, R. Luque, S. Redfield, F. Rodler, L. M. Serrano, V. Van Eylen

    K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant

    bib

    @article{10.1093/mnras/stab3497,
    author = {Smith, A M S and Breton, S N and Csizmadia, Sz and Dai, F and Gandolfi, D and García, R A and Howard, A W and Isaacson, H and Korth, J and Lam, K W F and Mathur, S and Nowak, G and Pérez Hernández, F and Persson, C M and Albrecht, S H and Barragán, O and Cabrera, J and Cochran, W D and Deeg, H J and Fridlund, M and Georgieva, I Y and Goffo, E and Guenther, E W and Hatzes, A P and Kabath, P and Livingston, J H and Luque, R and Palle, E and Redfield, S and Rodler, F and Serrano, L M and Van Eylen, V},
    title = "{K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {510},
    number = {4},
    pages = {5035-5049},
    year = {2021},
    month = {12},
    abstract = "{We report new photometric and spectroscopic observations of the K2-99 planetary system. Asteroseismic analysis of the short-cadence light curve from K2’s Campaign 17 allows us to refine the stellar properties. We find K2-99 to be significantly smaller than previously thought, with R⋆ = 2.55 ± 0.02 R⊙. The new light curve also contains four transits of K2-99 b, which we use to improve our knowledge of the planetary properties. We find the planet to be a non-inflated warm Jupiter, with Rb = 1.06 ± 0.01 \\$\\mathrm\\{R\_\\{\\rm Jup\\}\\}\\$. 60 new radial velocity measurements from HARPS, HARPS-N, and HIRES enable the determination of the orbital parameters of K2-99 c, which were previously poorly constrained. We find that this outer planet has a minimum mass Mcsin ic = 8.4 ± 0.2 \\$\\mathrm\\{M\_\\{\\rm Jup\\}\\}\\$, and an eccentric orbit (ec = 0.210 ± 0.009) with a period of 522.2 ± 1.4 d. Upcoming TESS observations in 2022 have a good chance of detecting the transit of this planet, if the mutual inclination between the two planetary orbits is small.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab3497},
    url = {https://doi.org/10.1093/mnras/stab3497},
    eprint = {https://academic.oup.com/mnras/article-pdf/510/4/5035/42245480/stab3497.pdf},
    }

    DOI arXiv
  44. Ó. Carrión-González, A. García Muñoz, N. C. Santos, J. Cabrera, Sz. Csizmadia, H. Rauer

    Constraining the radius and atmospheric properties of directly imaged exoplanets through multi-phase observations

  45. K. Herbst, J. L. Grenfell, M. Sinnhuber, F. Wunderlich

    INCREASE: An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs

    bib

    @article{https://doi.org/10.1002/asna.20210072,
    author = {Herbst, Konstantin and Grenfell, John Lee and Sinnhuber, Miriam and Wunderlich, Fabian},
    title = {INCREASE: An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs},
    journal = {Astronomische Nachrichten},
    volume = {n/a},
    number = {n/a},
    pages = {},
    keywords = {atmospheres, biosignatures, cosmic rays, habitability},
    doi = {https://doi.org/10.1002/asna.20210072},
    url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.20210072},
    eprint = {https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210072},
    abstract = {Abstract Exoplanets are as diverse as they are fascinating. They vary from ultrahot Jupiter-like low-density planets to presumed gas-ice-rock mixture worlds such as GJ 1214b or worlds as LHS 1140b, which features twice the Earth's bulk density. Regarding the great diversity of exoplanetary atmospheres, much remains to be explored. For a few selected objects such as GJ1214b, Proxima Centauri b, and the TRAPPIST-1 planets, the first observations of their atmospheres have already been achieved or are expected in the near future with the launch of the James Webb Space Telescope envisaged in October 2021. However, in order to interpret these observations, model studies of planetary atmospheres that account for various processes—such as atmospheric escape, outgassing, climate, photochemistry, as well as the physics of air showers and the transport of stellar energetic particles and galactic cosmic rays through the stellar astrospheres and planetary magnetic fields—are necessary. Here, we present our model suite INCREASE, a planned extension of the model suite discussed in Herbst, Grenfell, et al. (2019).}
    }

    DOI
  46. F. Liebing, S. V. Jeffers, A. Reiners, M. Zechmeister

    Convective blueshift strengths of 810 F to M solar-type stars

  47. Y. Shan, A. Reiners, D. Fabbian, E. Marfil, D. Montes, H. M. Tabernero, I. Ribas, J. A. Caballero, A. Quirrenbach, P. J. Amado, J. Aceituno, V. J. S. Béjar, M. Cortés-Contreras, S. Dreizler, A. P. Hatzes, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, J. C. Morales, E. Nagel, E. Pallé, V. M. Passegger, C. Rodríguez López, A. Schweitzer, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Not-so-fine hyperfine-split vanadium lines in cool star spectra

  48. M. Stangret, E. Pallé, N. Casasayas-Barris, M. Oshagh, A. Bello-Arufe, R. Luque, V. Nascimbeni, F. Yan, J. Orell-Miquel, D. Sicilia, L. Malavolta, B. C. Addison, L. A. Buchhave, A. S. Bonomo, F. Borsa, S. H. C. Cabot, M. Cecconi, D. A. Fischer, A. Harutyunyan, J. M. Mendonça, G. Nowak, H. Parviainen, A. Sozzetti, R. Tronsgaard

    The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions

  49. J. C. Yee, W. Zang, A. Udalski, Y. H. Ryu, J. Green, S. Hennerley, A. Marmont, T. Sumi, S. Mao, M. Gromadzki, P. Mróz, J. Skowron, R. Poleski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, S. Kozlowski, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. D. Albrow, S. J. Chung, A. Gould, C. Han, K. H. Hwang, Y. K. Jung, H. W. Kim, I. G. Shin, Y. Shvartzvald, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, Y. Lee, B. G. Park, R. W. Pogge, E. Bachelet, G. Christie, M. P. G. Hundertmark, D. Maoz, J. McCormick, T. Natusch, M. T. Penny, R. A. Street, Y. Tsapras, C. A. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, S. Johnson, W. Zhu, I. A. Bond, F. Abe, R. Barry, D. P. Bennett, A. Bhattacharya, M. Donachie, H. Fujii, A. Fukui, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, M. C. Alex Li, Y. Matsubara, Y. Muraki, S. Miyazaki, G. Olmschenk, C. Ranc, N. J. Rattenbury, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. J. Tristram, T. Yamawaki, A. Yonehara, MOA Collaboration

    OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet

  50. S. Brown Sevilla, M. Keppler, M. Barraza-Alfaro, J. D. Melon Fuksman, N. T. Kurtovic, P. Pinilla, M. Feldt, W. Brandner, C. Ginski, Th. Henning, H. Klahr, R. Asensio-Torres, F. Cantalloube, A. Garufi, R. G. van Holstein, M. Langlois, F. Menard, E. Rickman, M. Benisty, G. Chauvin, A. Zurlo, L. Weber, A. Pavlov, J. Ramos, S. Rochat, R. Roelfsema

    A multiwavelength analysis of the spiral arms in the protoplanetary disk around WaOph 6

  51. B. Ercolano, G. Picogna, K. Monsch, J. J. Drake, T. Preibisch

    The dispersal of protoplanetary discs – II: photoevaporation models with observationally derived irradiating spectra

    bib

    @article{10.1093/mnras/stab2590,
    author = {Ercolano, Barbara and Picogna, Giovanni and Monsch, Kristina and Drake, Jeremy J and Preibisch, Thomas},
    title = "{The dispersal of protoplanetary discs – II: photoevaporation models with observationally derived irradiating spectra}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {2},
    pages = {1675-1685},
    year = {2021},
    month = {09},
    abstract = "{Young solar-type stars are known to be strong X-ray emitters and their X-ray spectra have been widely studied. X-rays from the central star may play a crucial role in the thermodynamics and chemistry of the circumstellar material as well as in the atmospheric evolution of young planets. In this paper, we present model spectra based on spectral parameters derived from the observations of young stars in the Orion nebula cluster from the Chandra Orion Ultradeep Project (COUP). The spectra are then used to calculate new photoevaporation prescriptions that can be used in disc and planet population synthesis models. Our models clearly show that disc wind mass loss rates are controlled by the stellar luminosity in the soft (\\$100\\, \\mathrm\\{eV\\}\\$ to \\$1\\, \\mathrm\\{keV\\}\\$) X-ray band. New analytical relations are provided for the mass loss rates and profiles of photoevaporative winds as a function of the luminosity in the soft X-ray band. The agreement between observed and predicted transition disc statistics moderately improved using the new spectra, but the observed population of strongly accreting large cavity discs can still not be reproduced by these models. Furthermore, our models predict a population of non-accreting transition discs that are not observed. This highlights the importance of considering the depletion of millimetre-sized dust grains from the outer disc, which is a likely reason why such discs have not been detected yet.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2590},
    url = {https://doi.org/10.1093/mnras/stab2590},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/2/1675/40513968/stab2590.pdf},
    }

    DOI arXiv
  52. D. Höning, P. Baumeister, J. L. Grenfell, N. Tosi, M. J. Way

    Early Habitability and Crustal Decarbonation of a Stagnant-Lid Venus

    bib

    @article{https://doi.org/10.1029/2021JE006895,
    author = {Höning, Dennis and Baumeister, Philipp and Grenfell, John Lee and Tosi, Nicola and Way, Michael J.},
    title = {Early Habitability and Crustal Decarbonation of a Stagnant-Lid Venus},
    journal = {Journal of Geophysical Research: Planets},
    volume = {126},
    number = {10},
    pages = {e2021JE006895},
    keywords = {carbon cycle, exoplanets, habitability, planetary evolution, stagnant-lid, Venus},
    doi = {https://doi.org/10.1029/2021JE006895},
    url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2021JE006895},
    eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2021JE006895},
    note = {e2021JE006895 2021JE006895},
    abstract = {Abstract Little is known about the early evolution of Venus and a potential habitable period during the first 1 billion years. In particular, it remains unclear whether or not plate tectonics and an active carbonate-silicate cycle were present. In the presence of liquid water but without plate tectonics, weathering would have been limited to freshly produced basaltic crust, with an early carbon cycle restricted to the crust and atmosphere. With the evaporation of surface water, weathering would cease. With ongoing volcanism, carbonate sediments would be buried and sink downwards. Thereby, carbonates would heat up until they become unstable and the crust would become depleted in carbonates. With supply to the atmosphere the surface temperature rises further, the depth below which decarbonation occurs decreases, causing the release of even more . We assess the habitable period of an early stagnant-lid Venus by employing a coupled interior-atmosphere evolution model accounting for degassing, weathering, carbonate burial, and crustal decarbonation. We find that if initial surface conditions allow for liquid water, weathering can keep the planet habitable for up to 900 Myr, followed by evaporation of water and rapid crustal carbonate depletion. For the atmospheric of stagnant-lid exoplanets, we predict a bimodal distribution, depending on whether or not these planets experienced a runaway greenhouse in their history. Planets with high atmospheric could be associated with crustal carbonate depletion as a consequence of a runaway greenhouse, whereas planets with low atmospheric would indicate active silicate weathering and thereby a habitable climate.},
    year = {2021}
    }

    DOI arXiv
  53. S. Sabotta, M. Schlecker, P. Chaturvedi, E. W. Guenther, I. Muñoz Rodríguez, J. C. Muñoz Sánchez, J. A. Caballero, Y. Shan, S. Reffert, I. Ribas, A. Reiners, A. P. Hatzes, P. J. Amado, H. Klahr, J. C. Morales, A. Quirrenbach, Th. Henning, S. Dreizler, E. Pallé, M. Perger, M. Azzaro, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, D. Montes, V. M. Passegger, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Planet occurrence rates from a subsample of 71 stars

  54. N. Manger, T. Pfeil, H. Klahr

    High-resolution parameter study of the vertical shear instability – II: dependence on temperature gradient and cooling time

    bib

    @article{10.1093/mnras/stab2599,
    author = {Manger, Natascha and Pfeil, Thomas and Klahr, Hubert},
    title = "{High-resolution parameter study of the vertical shear instability – II: dependence on temperature gradient and cooling time}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {4},
    pages = {5402-5409},
    year = {2021},
    month = {09},
    abstract = "{A certain appeal to the alpha model for turbulence and related viscosity in accretion discs was that one scales the Reynolds stresses simply on the thermal pressure, assuming that turbulence driven by a certain mechanism will attain a characteristic Mach number in its velocity fluctuations. Besides the notion that there are different mechanism driving turbulence and angular momentum transport in a disc, we also find that within a single instability mechanism, here the vertical shear instability, stresses do not linearly scale with thermal pressure. Here, we demonstrate in numerical simulations the effect of the gas temperature gradient and the thermal relaxation time on the average stresses generated in the non-linear stage of the instability. We find that the stresses scale with the square of the exponent of the radial temperature profile at least for a range of dlog T/dlog R = [−0.5, −1], beyond which the pressure scale height varies too much over the simulation domain, to provide clear results. Stresses are also dependent on thermal relaxation times, provided they are longer than 10−3 orbital periods. The strong dependence of viscous transport of angular momentum on the local conditions in the disc (especially temperature, temperature gradient, and surface density/optical depth) challenges the ideas of viscosity leading to smooth density distributions, opening a route for structure (ring) formation and time variable mass accretion.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2599},
    url = {https://doi.org/10.1093/mnras/stab2599},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/4/5402/40979724/stab2599.pdf},
    }

    DOI arXiv
  55. L. Fossati, M. E. Young, D. Shulyak, T. Koskinen, C. Huang, P. E. Cubillos, K. France, A. G. Sreejith

    Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

  56. M. P. Döllinger, M. Hartmann

    A sanity check for planets around evolved Stars

    DOI
  57. G. Cugno, P. Patapis, T. Stolker, S. P. Quanz, A. Boehle, H. J. Hoeijmakers, G.-D. Marleau, P. Mollière, E. Nasedkin, I. A. G. Snellen

    Molecular mapping of the PDS70 system. No molecular absorption signatures from the forming planet PDS70 b

  58. V. Van Eylen, N. Astudillo-Defru, X. Bonfils, J. Livingston, T. Hirano, R. Luque, K. W. F. Lam, A. B. Justesen, J. N. Winn, D. Gandolfi, G. Nowak, E. Pallé, S. Albrecht, F. Dai, B. Campos Estrada, J. E. Owen, D. Foreman-Mackey, M. Fridlund, J. Korth, S. Mathur, T. Forveille, T. Mikal-Evans, H. L. M. Osborne, J. M. Almenara, C. S. K. Ho, E. Artigau, O. Barragán, S. C. C. Barros, F. Bouchy, J. Cabrera, D. Caldwell, D. Charbonneau, P. Chaturvedi, W. D. Cochran, S. Csizmadia, M. Damasso, X. Delfosse, J. De Medeiros, R. F. Díaz, R. Doyon, M. Esposito, G. Fűrész, P. Figueira, I. Georgieva, E. Goffo, S. Grziwa, E. W. Guenther, A. P. Hatzes, J. M. Jenkins, P. Kabáth, E. Knudstrup, D. W. Latham, B. Lavie, C. Lovis, R. Mennickent, S. E. Mullally, F. Murgas, N. Narita, F. A. Pepe, C. M. Persson, S. Redfield, G. R. Ricker, N. C. Santos, S. Seager, L. M. Serrano, A. M. S. Smith, A. Suárez Mascareño, J. Subjak, J. D. Twicken, S. Udry, R. Vanderspek, M. R. Zapatero Osorio

    Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley

    bib

    @article{10.1093/mnras/stab2143,
    author = {Van Eylen, V and Astudillo-Defru, N and Bonfils, X and Livingston, J and Hirano, T and Luque, R and Lam, K W F and Justesen, A B and Winn, J N and Gandolfi, D and Nowak, G and Palle, E and Albrecht, S and Dai, F and Campos Estrada, B and Owen, J E and Foreman-Mackey, D and Fridlund, M and Korth, J and Mathur, S and Forveille, T and Mikal-Evans, T and Osborne, H L M and Ho, C S K and Almenara, J M and Artigau, E and Barragán, O and Barros, S C C and Bouchy, F and Cabrera, J and Caldwell, D A and Charbonneau, D and Chaturvedi, P and Cochran, W D and Csizmadia, S and Damasso, M and Delfosse, X and De Medeiros, J R and Díaz, R F and Doyon, R and Esposito, M and Fűrész, G and Figueira, P and Georgieva, I and Goffo, E and Grziwa, S and Guenther, E and Hatzes, A P and Jenkins, J M and Kabath, P and Knudstrup, E and Latham, D W and Lavie, B and Lovis, C and Mennickent, R E and Mullally, S E and Murgas, F and Narita, N and Pepe, F A and Persson, C M and Redfield, S and Ricker, G R and Santos, N C and Seager, S and Serrano, L M and Smith, A M S and Mascareño, A Suárez and Subjak, J and Twicken, J D and Udry, S and Vanderspek, R and Zapatero Osorio, M R},
    title = "{Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {507},
    number = {2},
    pages = {2154-2173},
    year = {2021},
    month = {08},
    abstract = "{We report on precise Doppler measurements of L231-32 (TOI-270), a nearby M dwarf (d = 22 pc, M⋆ = 0.39 M⊙, R⋆ = 0.38 R⊙), which hosts three transiting planets that were recently discovered using data from the Transiting Exoplanet Survey Satellite (TESS). The three planets are 1.2, 2.4, and 2.1 times the size of Earth and have orbital periods of 3.4, 5.7, and 11.4 d. We obtained 29 high-resolution optical spectra with the newly commissioned Echelle Spectrograph for Rocky Exoplanet and Stable Spectroscopic Observations (ESPRESSO) and 58 spectra using the High Accuracy Radial velocity Planet Searcher (HARPS). From these observations, we find the masses of the planets to be 1.58 ± 0.26, 6.15 ± 0.37, and 4.78 ± 0.43 M⊕, respectively. The combination of radius and mass measurements suggests that the innermost planet has a rocky composition similar to that of Earth, while the outer two planets have lower densities. Thus, the inner planet and the outer planets are on opposite sides of the ‘radius valley’ – a region in the radius-period diagram with relatively few members – which has been interpreted as a consequence of atmospheric photoevaporation. We place these findings into the context of other small close-in planets orbiting M dwarf stars, and use support vector machines to determine the location and slope of the M dwarf (Teff \\< 4000 K) radius valley as a function of orbital period. We compare the location of the M dwarf radius valley to the radius valley observed for FGK stars, and find that its location is a good match to photoevaporation and core-powered mass-loss models. Finally, we show that planets below the M dwarf radius valley have compositions consistent with stripped rocky cores, whereas most planets above have a lower density consistent with the presence of a H-He atmosphere.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2143},
    url = {https://doi.org/10.1093/mnras/stab2143},
    eprint = {https://academic.oup.com/mnras/article-pdf/507/2/2154/40141388/stab2143.pdf},
    }

    DOI arXiv
  59. Y. Aoyama, G.-D. Marleau, M. Ikoma, C. Mordasini

    Comparison of Planetary Hα-emission Models: A New Correlation with Accretion Luminosity

  60. J. P. de Leon, J. H. Livingston, M. Endl, W. D. Cochran, T. Hirano, R. A. García, S. Mathur, K. W. F. Lam, J. Korth, A. A. Trani, F. Dai, E. Díez Alonso, A. Castro-Gonzáles, M. Fridlund, A. Fukui, D. Gandolfi, P. Kabáth, M. Kuzuhara, R. Luque, A. B. Savel, H. Gill, C. Dressing, S. Giacalone, N. Narita, E. Pallé, V. Van Eylen, M. Tamura

    37 new validated planets in overlapping K2 campaigns

    bib

    @article{10.1093/mnras/stab2305,
    author = {de Leon, J P and Livingston, J and Endl, M and Cochran, W D and Hirano, T and García, R A and Mathur, S and Lam, K W F and Korth, J and Trani, A A and Dai, F and Díez Alonso, E and Castro-González, A and Fridlund, M and Fukui, A and Gandolfi, D and Kabath, P and Kuzuhara, M and Luque, R and Savel, A B and Gill, H and Dressing, C and Giacalone, S and Narita, N and Palle, E and Van Eylen, V and Tamura, M},
    title = "{37 new validated planets in overlapping K2 campaigns}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {1},
    pages = {195-218},
    year = {2021},
    month = {08},
    abstract = "{We analysed 68 candidate planetary systems first identified during Campaigns 5 and 6 (C5 and C6) of the NASA K2 mission. We set out to validate these systems by using a suite of follow-up observations, including adaptive optics, speckle imaging, and reconnaissance spectroscopy. The overlap between C5 with C16 and C18, and C6 with C17, yields light curves with long baselines that allow us to measure the transit ephemeris very precisely, revisit single transit candidates identified in earlier campaigns, and search for additional transiting planets with longer periods not detectable in previous works. Using vespa, we compute false positive probabilities of less than 1 per cent for 37 candidates orbiting 29 unique host stars and hence statistically validate them as planets. These planets have a typical size of 2.2 R⊕ and orbital periods between 1.99 and 52.71 d. We highlight interesting systems including a sub-Neptune with the longest period detected by K2, sub-Saturns around F stars, several multiplanetary systems in a variety of architectures. These results show that a wealth of planetary systems still remains in the K2 data, some of which can be validated using minimal follow-up observations and taking advantage of analyses presented in previous catalogues.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2305},
    url = {https://doi.org/10.1093/mnras/stab2305},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/1/195/40435487/stab2305.pdf},
    }

    DOI arXiv
  61. M. Lafarga, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, J. A. Caballero, M. Azzaro, V. J. S. Béjar, M. Cortés-Contreras, S. Dreizler, A. P. Hatzes, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, D. Montes, J. C. Morales, M. Oshagh, C. Rodríguez López, P. Schöfer, A. Schweitzer, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Mapping stellar activity indicators across the M dwarf domain

  62. M. Bergemann, R. Hoppe, E. Semenova, M. Carlsson, S. A. Yakovleva, Y. V. Voronov, M. Bautista, A. Nemer, A. K. Belyaev, J. Leenaarts, L. Mashonkina, A. Reiners, M. Ellwarth

    Solar oxygen abundance

    bib

    @article{10.1093/mnras/stab2160,
    author = {Bergemann, Maria and Hoppe, Richard and Semenova, Ekaterina and Carlsson, Mats and Yakovleva, Svetlana A and Voronov, Yaroslav V and Bautista, Manuel and Nemer, Ahmad and Belyaev, Andrey K and Leenaarts, Jorrit and Mashonkina, Lyudmila and Reiners, Ansgar and Ellwarth, Monika},
    title = "{Solar oxygen abundance}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {2},
    pages = {2236-2253},
    year = {2021},
    month = {07},
    abstract = "{Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of the solar photospheric oxygen (O) abundance. New atomic models of O and Ni are used to perform non-local thermodynamic equilibrium (NLTE) calculations with 1D hydrostatic (MARCS) and 3D hydrodynamical (Stagger and Bifrost) models. The Bifrost 3D MHD simulations are used to quantify the influence of the chromosphere. We compare the 3D NLTE line profiles with new high-resolution, R\\$\\approx 700\\, 000\\$, spatially resolved spectra of the Sun obtained using the IAG FTS instrument. We find that the O i lines at 777 nm yield the abundance of log A(O) = 8.74 ± 0.03 dex, which depends on the choice of the H-impact collisional data and oscillator strengths. The forbidden [O i] line at 630 nm is less model dependent, as it forms nearly in LTE and is only weakly sensitive to convection. However, the oscillator strength for this transition is more uncertain than for the 777 nm lines. Modelled in 3D NLTE with the Ni i blend, the 630 nm line yields an abundance of log A(O) = 8.77 ± 0.05 dex. We compare our results with previous estimates in the literature and draw a conclusion on the most likely value of the solar photospheric O abundance, which we estimate at log A(O) = 8.75 ± 0.03 dex.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2160},
    url = {https://doi.org/10.1093/mnras/stab2160},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/2/2236/40587625/stab2160.pdf},
    }

    DOI arXiv
  63. F. Mekhaldi, F. Adolphi, K. Herbst, R. Muscheler

    The Signal of Solar Storms Embedded in Cosmogenic Radionuclides: Detectability and Uncertainties

    bib

    @article{https://doi.org/10.1029/2021JA029351,
    author = {Mekhaldi, F. and Adolphi, F. and Herbst, K. and Muscheler, R.},
    title = {The Signal of Solar Storms Embedded in Cosmogenic Radionuclides: Detectability and Uncertainties},
    journal = {Journal of Geophysical Research: Space Physics},
    volume = {126},
    number = {8},
    pages = {e2021JA029351},
    keywords = {solar storms, cosmogenic radionuclides, ice cores, solar particle events},
    doi = {https://doi.org/10.1029/2021JA029351},
    url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2021JA029351},
    eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029351},
    note = {e2021JA029351 2021JA029351},
    abstract = {Abstract The threat that solar storms pose to our ever-modernizing society has gathered significant interest in the recent past. This is partly due to the discoveries of large peaks in the content of cosmogenic radionuclides such as radiocarbon (14C) in tree rings and beryllium-10 (10Be) and chlorine-36 (36Cl) in ice cores that were linked to extreme solar storms dated to the past millennia. To better assess the threat that they represent, we need to better quantify the relationship between their energy spectrum and their magnitude with respect to the content of the radionuclides that we measure in environmental archives such as ice cores. Here, we model the global production rate that the 59 largest particle storms coming from the Sun have induced for 10Be, 14C, and 36Cl during the past 70 years. We also consider the deposition flux in 10Be and 36Cl over the high latitudes where all Greenland ice cores are located. Our analysis shows that it is unlikely that any recent solar particle event can be detected in 10Be from ice cores. By relating these values to empirical data from ice cores, we are able to quantify different detection limits and uncertainties for 10Be and 36Cl. Due to different sensitivities to solar energetic particles, we assess that 10Be may only be suitable to detect a limited number of extreme solar storms, while 36Cl is suitable to detect any extreme particle event. This implies that the occurrence-rate estimates of extreme solar storms, based mainly on 14C and 10Be, relate to a small population of potential events.},
    year = {2021}
    }

    DOI
  64. E. W. Guenther, D. Woeckel, P. Chaturvedi, S. Kumar, M. K. Srivastava

    The flare-activity of 2MASS J16111534-1757214 in the upper Scorpius association

    bib

    @article{10.1093/mnras/stab1973,
    author = {Guenther, E W and Wöckel, D and Chaturvedi, P and Kumar, V and Srivastava, M K and Muheki, P},
    title = "{The flare-activity of 2MASS J16111534–1757214 in the upper Scorpius association}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {507},
    number = {2},
    pages = {2103-2114},
    year = {2021},
    month = {07},
    abstract = "{Flares are known to play an important role for the evolution of the atmospheres of young planets. In order to understand the evolution of planets, it is thus important to study the flare-activity of young stars. This is particularly the case for young M‐stars, because they are very active. We study photometrically and spectroscopically the highly active M‐star 2MASS J16111534–1757214. We show that it is a member of the Upper Sco OB association, which has an age of 5–10 Myrs. We also re-evaluate the status of other bona-fide M‐stars in this region and identify 42 members. Analyzing the K2-light curves, we find that 2MASS J16111534–1757214 has, on average, one super-flare with \\$\\rm E\\ge 10^\\{35\\}\\$ erg every 620 h, and one with \\$\\rm E\\ge 10^\\{34\\}\\$ erg every 52 h. Although this is the most active M‐star in the Upper Sco association, the power-law index of its flare-distribution is similar to that of other M‐stars in this region. 2MASS J16111534–1757214 as well as other M‐stars in this region show a broken power-law distribution in the flare-frequency diagram. Flares larger than \\$\\rm E \\ge 3\\, 10^\\{34\\}\\$ erg have a power-law index \\$\\rm \\beta =-1.3\\pm 0.1\\$ and flares smaller than that \\$\\rm \\beta =-0.8\\pm 0.1\\$. We furthermore conclude that the flare-energy distribution for young M‐stars is not that different from solar-like stars.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab1973},
    url = {https://doi.org/10.1093/mnras/stab1973},
    eprint = {https://academic.oup.com/mnras/article-pdf/507/2/2103/40205335/stab1973.pdf},
    }

    DOI arXiv
  65. G. M. Brandt, T. D. Brandt, T. J. Dupuy, D. Michalik, G.-D. Marleau

    The First Dynamical Mass Measurement in the HR 8799 System

  66. S. Kumar, A. J. Poser, M. Schöttler, U. Kleinschmidt, W. Dietrich, J. Wicht, M. French, R. Redmer

    Ionization and transport in partially ionized multicomponent plasmas: Application to atmospheres of hot Jupiters

    bib

    @article{2021PhRvE.103f3203K,
    author = {{Kumar}, Sandeep and {Poser}, Anna Julia and {Sch{\"o}ttler}, Manuel and {Kleinschmidt}, Uwe and {Dietrich}, Wieland and {Wicht}, Johannes and {French}, Martin and {Redmer}, Ronald},
    title = {{Ionization and transport in partially ionized multicomponent plasmas: Application to atmospheres of hot Jupiters}},
    journal = {\pre},
    keywords = {Physics - Plasma Physics, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jun,
    volume = {103},
    number = {6},
    eid = {063203},
    pages = {063203},
    doi = {10.1103/PhysRevE.103.063203},
    archiveprefix = {arXiv},
    eprint = {2106.03092},
    primaryclass = {physics.plasm-ph},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021PhRvE.103f3203K},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  67. I. Georgieva, C. M. Persson, O. Barragán, G. Nowak, M. Fridlund, E. Pallé, D. Locci, R. Luque, I. Carleo, D. Gandolfi, S. R. Kane, J. Korth, K. G. Stassun, J. Livingston, E. Matthews, K. A. Collins, S. B. Howell, L. M. Serrano, S. Albrecht, A. Bieryla, C. E. Brasseur, D. R. Ciardi, W. D. Cochran, K. Colòn, I. Crossfield, Sz. Csizmadia, H. J. Deeg, M. Esposito, E. Furlan, T. Gan, E. Goffo, E. Gonzales, S. Grziwa, E. W. Guenther, P. Guerra, T. Hirano, J. M. Jenkins, E. L. N. Jensen, P. Kabáth, E. Knudstrup, K. W. F. Lam, D. W. Latham, A. Levine, R. A. Matson, S. McDermott, H. L. M. Osborne, M. Paegert, S. N. Quinn, S. Redfield, G. R. Ricker, J. E. Schlieder, N. Scott, S. Seager, A. M. S. Smith, P. Tenenbaum, J. D. Twicken, R. Vanderspek, V. Van Eylen, J. N. Winn

    Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260

    bib

    @article{10.1093/mnras/stab1464,
    author = {Georgieva, I Y and Persson, C M and Barragán, O and Nowak, G and Fridlund, M and Locci, D and Palle, E and Luque, R and Carleo, I and Gandolfi, D and Kane, S R and Korth, J and Stassun, K G and Livingston, J and Matthews, E C and Collins, K A and Howell, S B and Serrano, L M and Albrecht, S and Bieryla, A and Brasseur, C E and Ciardi, D and Cochran, W D and Colon, K D and Crossfield, I J M and Csizmadia, Sz and Deeg, H J and Esposito, M and Furlan, E and Gan, T and Goffo, E and Gonzales, E and Grziwa, S and Guenther, E W and Guerra, P and Hirano, T and Jenkins, J M and Jensen, E L N and Kabáth, P and Knudstrup, E and Lam, K W F and Latham, D W and Levine, A M and Matson, R A and McDermott, S and Osborne, H L M and Paegert, M and Quinn, S N and Redfield, S and Ricker, G R and Schlieder, J E and Scott, N J and Seager, S and Smith, A M S and Tenenbaum, P and Twicken, J D and Vanderspek, R and Van Eylen, V and Winn, J N},
    title = "{Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {505},
    number = {4},
    pages = {4684-4701},
    year = {2021},
    month = {05},
    abstract = "{We present the discovery and characterization of two sub-Neptunes in close orbits, as well as a tentative outer planet of a similar size, orbiting TOI-1260 – a low metallicity K6 V dwarf star. Photometry from Transiting Exoplanet Survey Satellite(TESS) yields radii of Rb = 2.33 ± 0.10 and Rc = 2.82 ± 0.15 R⊕, and periods of 3.13 and 7.49 d for TOI-1260 b and TOI-1260 c, respectively. We combined the TESS data with a series of ground-based follow-up observations to characterize the planetary system. From HARPS-N high-precision radial velocities we obtain Mb = \\$8.6 \_\\{ - 1.5 \\} ^ \\{ + 1.4 \\}\\$ and Mc = \\$11.8 \_\\{ - 3.2 \\} ^ \\{ + 3.4 \\}\\$ M⊕. The star is moderately active with a complex activity pattern, which necessitated the use of Gaussian process regression for both the light-curve detrending and the radial velocity modelling, in the latter case guided by suitable activity indicators. We successfully disentangle the stellar-induced signal from the planetary signals, underlining the importance and usefulness of the Gaussian process approach. We test the system’s stability against atmospheric photoevaporation and find that the TOI-1260 planets are classic examples of the structure and composition ambiguity typical for the 2–3 R⊕ range.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab1464},
    url = {https://doi.org/10.1093/mnras/stab1464},
    eprint = {https://academic.oup.com/mnras/article-pdf/505/4/4684/38824317/stab1464.pdf},
    }

    DOI arXiv
  68. R. Dawson, C. Huang, R. Brahm, K. A. Collins, M. J. Hobson, A. Jordán, J. Dong, J. Korth, T. Trifonov, L. Abe, A. Agabi, I. Bruni, R. P. Butler, M. Barbieri, K. I. Collins, D. Conti, J. D. Crane, N. Crouzet, G. Dransfield, P. Evans, N. Espinoza, T. Gan, T. Guillot, T. Henning, J. J. Lissauer, E. Jensen, W. Sainte, D. Mékarnia, G. Myers, S. Nandakumar, H. Relles, P. Sarkis, P. Torres, S. Shectman, F. X. Schmider, A. Shporer, C. Stockdale, J. Teske, A. Triaud, S. Wang, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, L. Bouma, J. A. Burt, D. Charbonneau, A. Levine, S. McDermott, B. McLean, M. Rose, B. Wohler

    Precise Transit and Radial-velocity Characterization of a Resonant Pair: The Warm Jupiter TOI-216c and Eccentric Warm Neptune TOI-216b.

    bib

    @ARTICLE{2021AJ....161..161D,
    author = {{Dawson}, Rebekah I. and {Huang}, Chelsea X. and {Brahm}, Rafael and {Collins}, Karen A. and {Hobson}, Melissa J. and {Jord{\'a}n}, Andr{\'e}s and {Dong}, Jiayin and {Korth}, Judith and {Trifonov}, Trifon and {Abe}, Lyu and {Agabi}, Abdelkrim and {Bruni}, Ivan and {Butler}, R. Paul and {Barbieri}, Mauro and {Collins}, Kevin I. and {Conti}, Dennis M. and {Crane}, Jeffrey D. and {Crouzet}, Nicolas and {Dransfield}, Georgina and {Evans}, Phil and {Espinoza}, N{\'e}stor and {Gan}, Tianjun and {Guillot}, Tristan and {Henning}, Thomas and {Lissauer}, Jack J. and {Jensen}, Eric L.~N. and {Sainte}, Wenceslas Marie and {M{\'e}karnia}, Djamel and {Myers}, Gordon and {Nandakumar}, Sangeetha and {Relles}, Howard M. and {Sarkis}, Paula and {Torres}, Pascal and {Shectman}, Stephen and {Schmider}, Fran{\c{c}}ois-Xavier and {Shporer}, Avi and {Stockdale}, Chris and {Teske}, Johanna and {Triaud}, Amaury H.~M.~J. and {Wang}, Sharon Xuesong and {Ziegler}, Carl and {Ricker}, G. and {Vanderspek}, R. and {Latham}, David W. and {Seager}, S. and {Winn}, J. and {Jenkins}, Jon M. and {Bouma}, L.~G. and {Burt}, Jennifer A. and {Charbonneau}, David and {Levine}, Alan M. and {McDermott}, Scott and {McLean}, Brian and {Rose}, Mark E. and {Vanderburg}, Andrew and {Wohler}, Bill},
    title = "{Precise Transit and Radial-velocity Characterization of a Resonant Pair: The Warm Jupiter TOI-216c and Eccentric Warm Neptune TOI-216b}",
    journal = {\aj},
    keywords = {Exoplanet astronomy, Exoplanet dynamics, Transit timing variation method, Radial velocity, 486, 490, 1710, 1332, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    volume = {161},
    number = {4},
    eid = {161},
    pages = {161},
    doi = {10.3847/1538-3881/abd8d0},
    archivePrefix = {arXiv},
    eprint = {2102.06754},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021AJ....161..161D},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  69. V. Christiaens, M. G. Ubeira-Gabellini, H. Cánovas, P. Delorme, B. Pairet, O. Absil, S. Casassus, J. Girard, A. Zurlo, Y. Aoyama, G.-D. Marleau, L. Spina, N. Marel, L. Cieza, G. Lodato, S. Pérez, C. Pinte, D. Price, M. Reggiani

    A faint companion around CrA-9: protoplanet or obscured binary?

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    @ARTICLE{2021MNRAS.502.6117C,
    author = {{Christiaens}, V. and {Ubeira-Gabellini}, M. -G. and {C{\'a}novas}, H. and {Delorme}, P. and {Pairet}, B. and {Absil}, O. and {Casassus}, S. and {Girard}, J.~H. and {Zurlo}, A. and {Aoyama}, Y. and {Marleau}, G. -D. and {Spina}, L. and {van der Marel}, N. and {Cieza}, L. and {Lodato}, G. and {P{\'e}rez}, S. and {Pinte}, C. and {Price}, D.~J. and {Reggiani}, M.},
    title = "{A faint companion around CrA-9: protoplanet or obscured binary?}",
    journal = {\mnras},
    keywords = {techniques: image processing, planets and satellites: formation, planet-disc interactions, protoplanetary discs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = apr,
    volume = {502},
    number = {4},
    pages = {6117-6139},
    doi = {10.1093/mnras/stab480},
    archivePrefix = {arXiv},
    eprint = {2102.10288},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.6117C},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  70. I. Kondo, J. C. Yee, D. P. Bennett, T. Sumi, N. Koshimoto, I. A. Bond, A. Gould, A. Udalski, Y. Shvartzvald, Y. K. Jung, W. Zang, V. Bozza, E. Bachelet, M. Hundertmark, N. J. Rattenbury, F. Abe, R. K. Barry, A. Bhattacharya, M. Donachie, A. Fukui, H. Fujii, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, J. Li, Y. Matsubara, S. Miyazaki, Y. Muraki, G. Olmschenk, C. Ranc, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. J. Tristram, T. Yamawaki, A. Yonehara, P. Mróz, R. Poleski, J. Skowron, M. K. Szymański, I. Szymański, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. Albrow, S. J. Chung, C. Han, K. H. Hwang, H. W. Kim, I. G. Shin, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, S.L. Lee, B. G. Park, R. W. Pogge, Y. H. Ryu, C. A. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, W. Zhu, D. Maoz, M. T. Penny, M. Dominik, U. G. Jørgensen, P. Longa-Peña, N. Peixinho, S. Sajadian, J. Skottfelt, C. Snodgrass, J. Tregloan-Reed, M. J. Burgdorf, J. Campbell-White, Y. I. Fujii, T. C. Hinse, E. Khalouei, S. Rahvar, M. Rabus, J. Southworth, Y. Tsapras, R. A. Street, D. M. Bramich, A. Cassan, K. Horne, S. Mao, A. Saha

    OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf.

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    @ARTICLE{2021arXiv210402157K,
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    title = "{OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    eid = {arXiv:2104.02157},
    pages = {arXiv:2104.02157},
    archivePrefix = {arXiv},
    eprint = {2104.02157},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210402157K},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  71. S. Ataiee, W. Kley

    Pushing planets into an inner cavity by a resonant chain

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    @article{2021A&A...648A..69A,
    author = {{Ataiee}, S. and {Kley}, W.},
    title = {{Pushing planets into an inner cavity by a resonant chain}},
    journal = {\aap},
    keywords = {methods: numerical, hydrodynamics, planets and satellites: dynamical evolution and stability, protoplanetary disks, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    volume = {648},
    eid = {A69},
    pages = {A69},
    doi = {10.1051/0004-6361/202038772},
    archiveprefix = {arXiv},
    eprint = {2102.08612},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...648A..69A},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  72. N. Casasayas-Barris, M. Stangret, V. Bourrier, H. M. Tabernero, F. Yan, F. Borsa, R. Allart, M. R. Zapatero Osorio, C. Lovis, S. G. Sousa, G. Chen, M. Oshagh, N. C. Santos, F. Pepe, R. Rebolo, P. Molaro, S. Cristiani, V. Adibekyan, Y. Alibert, C. Allende Prieto, F. Bouchy, O. Demangeon, P. Di Marcantonio, V. D'Odorico, D. Ehrenreich, P. Figueira, R. Génova Santos, J. I. González Hernández, B. Lavie, J. Lillo-Box, G. Lo Curto, C. Martins, A. Mehner, G. Micela, N. Nunes, E. Poretti, A. Sozzetti, A. Suárez Mascareño, S. Udry

    The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution

    bib

    @ARTICLE{2021A&A...647A..26C,
    author = {{Casasayas-Barris}, N. and {Palle}, E. and {Stangret}, M. and {Bourrier}, V. and {Tabernero}, H.~M. and {Yan}, F. and {Borsa}, F. and {Allart}, R. and {Zapatero Osorio}, M.~R. and {Lovis}, C. and {Sousa}, S.~G. and {Chen}, G. and {Oshagh}, M. and {Santos}, N.~C. and {Pepe}, F. and {Rebolo}, R. and {Molaro}, P. and {Cristiani}, S. and {Adibekyan}, V. and {Alibert}, Y. and {Allende Prieto}, C. and {Bouchy}, F. and {Demangeon}, O.~D.~S. and {Di Marcantonio}, P. and {D'Odorico}, V. and {Ehrenreich}, D. and {Figueira}, P. and {G{\'e}nova Santos}, R. and {Gonz{\'a}lez Hern{\'a}ndez}, J.~I. and {Lavie}, B. and {Lillo-Box}, J. and {Lo Curto}, G. and {Martins}, C.~J.~A.~P. and {Mehner}, A. and {Micela}, G. and {Nunes}, N.~J. and {Poretti}, E. and {Sozzetti}, A. and {Su{\'a}rez Mascare{\~n}o}, A. and {Udry}, S.},
    title = "{The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution}",
    journal = {\aap},
    keywords = {planets and satellites: individual: HD 209458b, planets and satellites: atmospheres, methods: observational, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = mar,
    volume = {647},
    eid = {A26},
    pages = {A26},
    doi = {10.1051/0004-6361/202039539},
    archivePrefix = {arXiv},
    eprint = {2101.04094},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..26C},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  73. E. Brown, S. C. Marsden, M. Mengel, S. V. Jeffers, I. Millburn, M. Mittag, P. Petit, A. Vidotto, J. Morin, V. See, M. M. Jardine, J. González-Pérez, BCool Collaboration

    Magnetic field and chromospheric activity evolution of HD 75332: a rapid magnetic cycle in an F star without a hot Jupiter

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    @ARTICLE{2021MNRAS.501.3981B,
    author = {{Brown}, E.~L. and {Marsden}, S.~C. and {Mengel}, M.~W. and {Jeffers}, S.~V. and {Millburn}, I. and {Mittag}, M. and {Petit}, P. and {Vidotto}, A.~A. and {Morin}, J. and {See}, V. and {Jardine}, M. and {Gonz{\'a}lez-P{\'e}rez}, J.~N. and {BCool Collaboration}},
    title = "{Magnetic field and chromospheric activity evolution of HD 75332: a rapid magnetic cycle in an F star without a hot Jupiter}",
    journal = {\mnras},
    keywords = {stars: activity, stars: magnetic field, stars: individual (HD 75332), Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = mar,
    volume = {501},
    number = {3},
    pages = {3981-4003},
    doi = {10.1093/mnras/staa3878},
    archivePrefix = {arXiv},
    eprint = {2012.05407},
    primaryClass = {astro-ph.SR},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.3981B},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  74. R. Asensio-Torres, T. Henning, F. Cantalloube, P. Pinilla, D. Mesa, A. Garufi, S. Jorquera, R. Gratton, G. Chauvin, J. Szulagyi, R. van Boekel, R. Dong, G.-D. Marleau, M. Benisty, M. Villenave, C. Bergez-Casalou, C. Desgrange, M. Janson, M. Keppler, M. Langlois, F. Menard, E. Rickman, T. Stolker, M. Feldt, T. Fusco, L. Gluck, A. Pavlov, J. Ramos

    Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks

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    @ARTICLE{2021arXiv210305377A,
    author = {{Asensio-Torres}, R. and {Henning}, Th. and {Cantalloube}, F. and {Pinilla}, P. and {Mesa}, D. and {Garufi}, A. and {Jorquera}, S. and {Gratton}, R. and {Chauvin}, G. and {Szulagyi}, J. and {van Boekel}, R. and {Dong}, R. and {Marleau}, G. -D. and {Benisty}, M. and {Villenave}, M. and {Bergez-Casalou}, C. and {Desgrange}, C. and {Janson}, M. and {Keppler}, M. and {Langlois}, M. and {Menard}, F. and {Rickman}, E. and {Stolker}, T. and {Feldt}, M. and {Fusco}, T. and {Gluck}, L. and {Pavlov}, A. and {Ramos}, J.},
    title = "{Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = mar,
    eid = {arXiv:2103.05377},
    pages = {arXiv:2103.05377},
    archivePrefix = {arXiv},
    eprint = {2103.05377},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210305377A},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  75. F. Wunderlich, M. Scheucher, J. L. Grenfell, F. Schreier, C. Sousa-Silva, M. Godolt, H. Rauer

    Detectability of biosignatures on LHS 1140 b

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    author = {{Wunderlich}, Fabian and {Scheucher}, Markus and {Grenfell}, John Lee and {Schreier}, Franz and {Sousa-Silva}, Clara and {Godolt}, Mareike and {Rauer}, Heike},
    title = "{Detectability of biosignatures on LHS 1140 b}",
    journal = {\aap},
    keywords = {planets and satellites: terrestrial planets, planets and satellites: detection, planets and satellites: composition, planets and satellites: atmospheres, techniques: spectroscopic, astrochemistry, Astrophysics - Earth and Planetary Astrophysics, Physics - Chemical Physics},
    year = 2021,
    month = mar,
    volume = {647},
    eid = {A48},
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    doi = {10.1051/0004-6361/202039663},
    archivePrefix = {arXiv},
    eprint = {2012.11426},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..48W},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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    DOI arXiv
  76. R. H. Tilbrook, M. R. Burleigh, J. C. Costes, S. Gill, L. D. Nielsen, J. I. Vines, D. Queloz, S. T. Hodgkin, H. L. Worters, M. R. Goad, J. S. Acton, B. A. Henderson, D. J. Armstrong, D. R. Anderson, D. Bayliss, F. Bouchy, J. T. Briegal, E. M. Bryant, S. L. Casewell, A. Chaushev, B. F. Cooke, P. Eigmüller, E. Gillen, M. N. Günther, A. Hogan, J. S. Jenkins, M. Lendl, J. McCormac, M. Moyano, L. Raynard, A. M. S. Smith, S. Udry, C. A. Watson, R. G. West, P. J. Wheatley, H. Breytenbach, R. R. Sefako, J. K. Thomas, D. R. Alves

    NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey

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    @article{2021MNRAS.tmp..893T,
    author = {{Tilbrook}, Rosanna H. and {Burleigh}, Matthew R. and {Costes}, Jean C. and {Gill}, Samuel and {Nielsen}, Louise Dyregaard and {Vines}, Jos{\'e} I. and {Queloz}, Didier and {Hodgkin}, Simon T. and {Worters}, Hannah L. and {Goad}, Michael R. and {Acton}, Jack S. and {Henderson}, Beth A. and {Armstrong}, David J. and {Anderson}, David R. and {Bayliss}, Daniel and {Bouchy}, Fran{\c{c}}ois and {Briegal}, Joshua T. and {Bryant}, Edward M. and {Casewell}, Sarah L. and {Chaushev}, Alexander and {Cooke}, Benjamin F. and {Eigm{\"u}ller}, Philipp and {Gillen}, Edward and {G{\"u}nther}, Maximilian N. and {Hogan}, Aleisha and {Jenkins}, James S. and {Lendl}, Monika and {McCormac}, James and {Moyano}, Maximiliano and {Raynard}, Liam and {Smith}, Alexis M.~S. and {Udry}, St{\'e}phane and {Watson}, Christopher A. and {West}, Richard G. and {Wheatley}, Peter J. and {Breytenbach}, Hannes and {Sefako}, Ramotholo R. and {Thomas}, Jessymol K. and {Alves}, Douglas R.},
    title = {{NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey}},
    journal = {\mnras},
    keywords = {planetary systems, planets and satellites: detection, planets and satellites: gaseous planets, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = mar,
    doi = {10.1093/mnras/stab815},
    archiveprefix = {arXiv},
    eprint = {2103.10302},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.tmp..893T},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  77. T.W. Moldenhauer, R. Kuiper, W. Kley

    Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres

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    title = "{Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = feb,
    eid = {arXiv:2102.00939},
    pages = {arXiv:2102.00939},
    archivePrefix = {arXiv},
    eprint = {2102.00939},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210200939M},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  78. G. Scandariato, F. Borsa, D. Sicilia, L. Malavolta, K. Biazzo, A. S. Bonomo, G. Bruno, R. Claudi, E. Covino, P. Di Marcantonio, M. Esposito, G. Frustagli, A. F. Lanza, J. Maldonado, A. Maggio, L. Mancini, G. Micela, D. Nardiello, M. Rainer, V. Singh, A. Sozzetti, L. Affer, S. Benatti, A. Bignamini, V. Biliotti, R. Capuzzo-Dolcetta, I. Carleo, R. Cosentino, M. Damasso, S. Desidera, A. Gurtubai, A. Ghedina, P. Giacobbe, E. Giani, A. Harutyunyan, N. Hernandez, M. Hernandez Diaz, C. Knapic, G. Leto, A. F. Martinez Fiorenzano, E. Molinari, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, E. Poretti, H. Stoev

    The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy

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    title = "{The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy}",
    journal = {\aap},
    keywords = {techniques: spectroscopic, planets and satellites: atmospheres, planets and satellites: detection, planets and satellites: gaseous planets, planets and satellites: individual: 51 Peg b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = feb,
    volume = {646},
    eid = {A159},
    pages = {A159},
    doi = {10.1051/0004-6361/202039271},
    archivePrefix = {arXiv},
    eprint = {2012.10435},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.159S},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  79. M. Janson, V. Squicciarini, P. Delorme, R. Gratton, M. Bonnefoy, S. Reffert, S. C. Eriksson, A. Vigan, M. Langlois, N. Engler, G. Chauvin, S. Desidera, L. Mayer, G.-D. Marleau, A. J. Bohn, M. Samland, M. Meyer, V. D'Orazi, T. Henning, S. P. Quanz, M. Kenworthy, J. C. Carson

    BEAST begins: sample characteristics and survey performance of the B-star Exoplanet Abundance Study

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    @ARTICLE{2021A&A...646A.164J,
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    title = "{BEAST begins: sample characteristics and survey performance of the B-star Exoplanet Abundance Study}",
    journal = {\aap},
    keywords = {planets and satellites: detection, stars: early-type, brown dwarfs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = feb,
    volume = {646},
    eid = {A164},
    pages = {A164},
    doi = {10.1051/0004-6361/202039683},
    archivePrefix = {arXiv},
    eprint = {2101.02043},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.164J},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  80. L. Carone, P. Mollière, G. Zhou, J. Bouwman, F. Yan, R. Baeyens, D. Apai, N. Espinoza, B. V. Rackham, A. Jordán, D. Angerhausen, L. Decin, M. Lendl, O. Venot, T. Henning

    Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b

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    title = "{Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b}",
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    keywords = {methods: observational, planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    archivePrefix = {arXiv},
    eprint = {2006.05382},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.168C},
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    }

    DOI arXiv
  81. K. Monsch, G. Picogna, B. Ercolano, W. Kley

    Giant planet migration during the disc dispersal phase

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    author = {{Monsch}, Kristina and {Picogna}, Giovanni and {Ercolano}, Barbara and {Kley}, Wilhelm},
    title = "{Giant planet migration during the disc dispersal phase}",
    journal = {\aap},
    keywords = {protoplanetary disks, planet-disk interactions, planets and satellites: gaseous planets, X-rays: stars, methods: numerical, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = feb,
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    doi = {10.1051/0004-6361/202039658},
    archivePrefix = {arXiv},
    eprint = {2101.01179},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.169M},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  82. A. Smith, J. S. Acton, D. R. Anderson, D. J. Armstrong, D. Bayliss, C. Belardi, F. Bouchy, R. Brahm, J. T. Briegal, E. Bryant, M. R. Burleigh, J. Cabrera, A. Chaushev, B. Cooke, J. C. Costes, S. Csizmadia, P. Eigmüller, A. Erikson, S. Gill, E. Gillen, M. R. Goad, M. N. Günther, C. B. Henderson, A. Hogan, A. Jordán, M. Lendl, J. McCormac, M. Moyano, L. D. Nielsen, H. Rauer, L. Raynard, R. H. Tilbrook, O. Turner, S. Udry, J. I. Vines, C. A. Watson, R. G. West, P. J. Wheatley

    NGTS-14Ab: a Neptune-sized transiting planet in the desert

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    keywords = {planetary systems, planets and satellites: detection, planets and satellites: individual: NGTS-14Ab, binaries: general, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = feb,
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    archivePrefix = {arXiv},
    eprint = {2101.01470},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.183S},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  83. P. Gao, H. R. Wakeford, S. Moran, V. Parmentier

    Aerosols in Exoplanet Atmospheres

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    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics},
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    pages = {arXiv:2102.03480},
    archivePrefix = {arXiv},
    eprint = {2102.03480},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210203480G},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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    DOI arXiv
  84. W. Dietrich, P. Wulff, J. Wicht, U. R. Christensen

    Linking Zonal Winds and Gravity II: explaining the equatorially antisymmetric gravity moments of Jupiter

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    keywords = {Astrophysics - Earth and Planetary Astrophysics},
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    eid = {arXiv:2102.12854},
    pages = {arXiv:2102.12854},
    archivePrefix = {arXiv},
    eprint = {2102.12854},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210212854D},
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    DOI arXiv
  85. J. D. Melon Fuksman, H. Klahr, M. Flock, A. Mignone

    A Two-moment Radiation Hydrodynamics Scheme Applicable to Simulations of Planet Formation in Circumstellar Disks

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    DOI arXiv
  86. S. Petrus, M. Bonnefoy, G. Chauvin, B. Charnay, G.-D. Marleau, R. Gratton, A. M. Lagrange, J. Rameau, C. Mordasini, M. Nowak, P. Delorme, A. Boccaletti, A. Carlotti, M. Houllé, A. Vigan, F. Allard, S. Desidera, V. D'Orazi, H. J. Hoeijmakers, A. Wyttenbach, B. Lavie

    A medium-resolution spectrum of the exoplanet HIP 65426 b

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    DOI arXiv
  87. H. Parviainen, M. R. Zapatero Osorio, G. Nowak, A. Fukui, F. Murgas, N. Narita, K. G. Stassun, J. H. Livingston, K. A. Collins, D. Hidalgo Soto, V. J. S. Béjar, J. Korth, M. Monelli, P. Montañés-Rodríguez, N. Casasayas-Barris, G. Chen, N. Crouzet, J. de Leon, A. Hernandez, K. Kawauchi, P. Klagyivik, N. Kusakabe, R. Luque, M. Mori, T. Nishiumi, J. Prieto-Arranz, M. Tamura, N. Watanabe, T. Gan, E. Jensen, T. Barclay, J. Doty, J. M. Jenkins, D. W. Latham, M. Paegert, G. Ricker, D. Rodriguez, S. Seager, A. Shporer, R. Vanderspek, J. Noel Villaseñor, J. N. Winn, B. Wohler, I. Wong

    TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis

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    title = "{TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis}",
    journal = {\aap},
    keywords = {stars: individual: TIC 218 795 833, planets and satellites: general, methods: statistical, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = jan,
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    archivePrefix = {arXiv},
    eprint = {2011.11458},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..16P},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  88. F. Yan, A. Wyttenbach, N. Casasayas-Barris, A. Reiners, T. Henning, P. Mollière, S. Czesla, L. Nortmann, K. Molaverdikhani, G. Chen, I. A. G. Snellen, M. Zechmeister, C. Huang, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, D. Cont, S. Khalafinejad, J. Khaimova, M. López-Puertas, D. Montes, E. Nagel, M. Oshagh, S. Pedraz, M. Stangret

    Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b

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    title = "{Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b}",
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-33b, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jan,
    volume = {645},
    eid = {A22},
    pages = {A22},
    doi = {10.1051/0004-6361/202039302},
    archivePrefix = {arXiv},
    eprint = {2011.07888},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..22Y},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  89. R. Luque, L. M. Serrano, K. Molaverdikhani, M. Nixon, J. Livingston, E. Guenther, N. Madhusudhan, G. Nowak, J. Korth, W. D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. Colòn, I. Crossfield, S. Csizmadia, F. Dai, H. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R. Goeke, S. Grziwa, A. P. Hatzes, C. E. Henze, S. Howell, J. Irwin, J. M. Jenkins, E. Jensen, P. Kabáth, R. Kidwell, J. Kielkopf, E. Knudstrup, K. W. F. Lam, D. W. Latham, J. J. Lissauer, A. W. Mann, E. Matthews, I. Mireles, N. Narita, M. Paegert, C. M. Persson, S. Redfield, G. Ricker, F. Rodler, J. E. Schlieder, N. Scott, S. Seager, J. Subjak, T. Tan, E. B. Ting, R. Vanderspek, V. Van Eylen, J. N. Winn, C. Ziegler

    A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776

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    @ARTICLE{2021A&A...645A..41L,
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    title = "{A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776}",
    journal = {\aap},
    keywords = {planetary systems, techniques: photometric, techniques: radial velocities, stars: individual: LP 961-53, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jan,
    volume = {645},
    eid = {A41},
    pages = {A41},
    doi = {10.1051/0004-6361/202039455},
    archivePrefix = {arXiv},
    eprint = {2009.08338},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..41L},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  90. O. Schib, C. Mordasini, N. Wenger, G.-D. Marleau, R. Helled

    The influence of infall on the properties of protoplanetary discs. Statistics of masses, sizes, lifetimes, and fragmentation

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    title = "{The influence of infall on the properties of protoplanetary discs. Statistics of masses, sizes, lifetimes, and fragmentation}",
    journal = {\aap},
    keywords = {instabilities, protoplanetary disks, accretion, accretion disks, planets and satellites: formation, stars: formation},
    year = 2021,
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    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..43S},
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    }

    DOI arXiv
  91. P. Sarkis, C. Mordasini, T. Henning, G.-D. Marleau, P. Mollière

    Evidence of three mechanisms explaining the radius anomaly of hot Jupiters.

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    title = "{Evidence of three mechanisms explaining the radius anomaly of hot Jupiters}",
    journal = {\aap},
    keywords = {planets and satellites: gaseous planets, planets and satellites: interiors, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jan,
    volume = {645},
    eid = {A79},
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..79S},
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    DOI arXiv
  92. O. Voelkel, R. Deienno, K. Kretke, H. Klahr

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    primaryClass = {astro-ph.EP},
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  93. O. Voelkel, R. Deienno, K. Kretke, H. Klahr

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    keywords = {planets and satellites: formation, planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jan,
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    archivePrefix = {arXiv},
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.132V},
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    primaryClass = {astro-ph.IM},
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    Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley

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    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = jan,
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    pages = {arXiv:2101.01593},
    archivePrefix = {arXiv},
    eprint = {2101.01593},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210101593V},
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  96. J. C. Yee, W. Zang, A. Udalski, Y. H. Ryu, J. Green, S. Hennerley, A. Marmont, T. Sumi, S. Mao, M. Gromadzki, P. Mróz, J. Skowron, R. Poleski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. Albrow, S. J. Chung, A. Gould, C. Han, K. H. Hwang, Y. K. Jung, H. W. Kim, I. G. Shin, Y. Shvartzvald, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, E. Bachelet, G. Christie, M. Hundertmark, D. Maoz, J. McCormick, T. Natusch, M. T. Penny, R. Street, Y. Tsapras, C. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, S. Johnson, W. Zhu, I. A. Bond, F. Abe, R. Barry, D. P. Bennett, A. Bhattacharya, M. Donachie, H. Fujii, A. Fukui, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, M. Li, Y. Matsubara, Y. Muraki, S. Miyazaki, G. Olmschenk, C. Ranc, N. J. Rattenbury, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. Tristram, T. Yamawaki, A. Yonehara

    OGLE-2019-BLG-0960Lb: The Smallest Microlensing Planet

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    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = jan,
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    pages = {arXiv:2101.04696},
    archivePrefix = {arXiv},
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    primaryClass = {astro-ph.EP},
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  97. T. Stolker, G.-D. Marleau, G. Cugno, P. Mollière, S. P. Quanz, K. O. Todorov, J. Kühn

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  98. M. Tala-Pinto, S. Reffert, A. Quirrenbach, S. Stock, T. Trifonov, D. S. Mitchell

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    title = {{The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS}},
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    month = nov,
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    primaryclass = {astro-ph.EP},
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    The widest broadband transmission spectrum (0.38-1.71 μm) of HD 189733b from ground-based chromatic Rossiter-McLaughlin observations

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  105. O. Voelkel, H. Klahr, C. Mordasini, C. Lenz

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  106. R. Helled, G. Mazzola, R. Redmer

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    DOI arXiv
  113. C. Mai, S. J. Desch, R. Kuiper, G.-D. Marleau, C. P. Dullemond

    The Dynamic Proto-atmospheres around Low-mass Planets with Eccentric Orbits

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    title = {{The Dynamic Proto-atmospheres around Low-mass Planets with Eccentric Orbits}},
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    keywords = {Hydrodynamics, Planetary atmospheres, Planet formation, Elliptical orbits, 1963, 1244, 1241, 457, Astrophysics - Earth and Planetary Astrophysics},
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    DOI arXiv
  114. F. Yan, A. Reiners, K. Molaverdikhani, N. Casasayas-Barris, L. Nortmann, G. Chen, P. Mollière, M. Stangret

    A temperature inversion with atomic iron in the ultra-hot dayside atmosphere of WASP-189b

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    title = {{A temperature inversion with atomic iron in the ultra-hot dayside atmosphere of WASP-189b}},
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    keywords = {planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-189b, Astrophysics - Earth and Planetary Astrophysics},
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    month = aug,
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    pages = {L5},
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  115. Ó. Carrión-González, A. García Muñoz, J. Cabrera, S. Csizmadia, N. C. Santos, H. Rauer

    Directly imaged exoplanets in reflected starlight: the importance of knowing the planet radius.

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    title = {{Directly imaged exoplanets in reflected starlight: the importance of knowing the planet radius}},
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    keywords = {planets and satellites: atmospheres, planets and satellites: gaseous planets, radiative transfer, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
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    DOI arXiv
  116. P. Mollière, T. Stolker, S. Lacour, G. P. P. L. Otten, J. Shangguan, B. Charnay, T. Molyarova, M. Nowak, T. Henning, G.-D. Marleau, D. A. Semenov, E. van Dishoeck, F. Eisenhauer, P. Garcia, R. Garcia Lopez, J. H. Girard, A. Z. Greenbaum, S. Hinkley, P. Kervella, L. Kreidberg, A. L. Maire, E. Nasedkin, L. Pueyo, I. A. G. Snellen, A. Vigan, J. Wang, P. T. de Zeeuw, A. Zurlo

    Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e

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    title = {{Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e}},
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    DOI arXiv
  117. C. T. Lenz, H. Klahr, T. Birnstiel, K. Kretke, S. Stammler

    Constraining the parameter space for the solar nebula. The effect of disk properties on planetesimal formation

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    title = {{Constraining the parameter space for the solar nebula. The effect of disk properties on planetesimal formation}},
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    keywords = {accretion, accretion disks, protoplanetary disks, circumstellar matter, turbulence, methods: numerical, minor planets, asteroids: general},
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    eid = {A61},
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    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...640A..61L},
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    DOI arXiv
  118. Y. Hirao, D. P. Bennett, Y. H. Ryu, N. Koshimoto, A. Udalski, J. C. Yee, T. Sumi, I. A. Bond, Y. Shvartzvald, F. Abe, R. K. Barry, A. Bhattacharya, M. Donachie, A. Fukui, Y. Itow, I. Kondo, A. Li Man Cheung, Y. Matsubara, T. Matsuo, S. Miyazaki, Y. Muraki, M. Nagakane, C. Ranc, N. J. Rattenbury, H. Suematsu, H. Shibai, D. Suzuki, P. J. Tristram, A. Yonehara, MOA Collaboration, J. Skowron, R. Poleski, P. Mróz, M. K. Szymański, I. Soszyński, P. Pietrukowicz, K. Ulaczyk, K. A. Rybicki, P. Iwanek, OGLE Collaboration, M. D. Albrow, S. J. Chung, A. Gould, C. Han, K. H. Hwang, Y. K. Jung, I. G. Shin, W. Zang, S. M. Cha, D. J. Kim, H. W. Kim, S. L. Kim, C. H. Lee, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, KMTNet Collaboration, C. A. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, W. Zhu, Spitzer Team, E. Bachelet, G. Bolt, G. Christie, M. Hundertmark, T. Natusch, D. Maoz, J. McCormick, R. A. Street, T. G. Tan, Y. Tsapras, LCO, μFUN Follow-up Teams, U. G. Jørgensen, M. Dominik, V. Bozza, J. Skottfelt, C. Snodgrass, S. Ciceri, R. Figuera Jaimes, D. F. Evans, N. Peixinho, T. C. Hinse, M. J. Burgdorf, J. Southworth, S. Rahvar, S. Sajadian, M. Rabus, C. von Essen, Y. I. Fujii, J. Campbell-White, S. Lowry, C. Helling, L. Mancini, L. K. Haikala, MiNDSTEp Collaboration, R. Kandori, IRSF Team

    OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk

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    eprint = {2004.09067},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  119. G. Ortenzi, L. Noack, F. Sohl, C. M. Guimond, J. L. Grenfell, C. Dorn, J. M. Schmidt, S. Vulpius, N. Katyal, D. Kitzmann, H. Rauer

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    K2-280 b – a low density warm sub-Saturn around a mildly evolved star

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    title = {{K2-280 b - a low density warm sub-Saturn around a mildly evolved star}},
    journal = {\mnras},
    keywords = {techniques: photometric, techniques: radial velocities, techniques: spectroscopic, planets and satellites: detection, stars: individual: (EPIC 216494238, K2-280), Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  121. M. Lisogorskyi, S. Boro Saikia, S. V. Jeffers, H. R. A. Jones, J. Morin, M. Mengel, A. Reiners, A. A. Vidotto, P. Petit

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    year = 2020,
    month = jul,
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  122. F. Flammini Dotti, M. B. N. Kouwenhoven, Q. Shu, W. Hao, R. Spurzem

    Planetary systems in a star cluster II: intermediate-mass black holes and planetary systems

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    journal = {\mnras},
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    month = jul,
    volume = {497},
    number = {3},
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    archiveprefix = {arXiv},
    eprint = {2007.11999},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  123. B. Akinsanmi, S. C. C. Barros, N. C. Santos, M. Oshagh, L. M. Serrano

    Constraining the oblateness of transiting planets with photometry and spectroscopy

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    year = 2020,
    month = jul,
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    number = {3},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  124. K. Stock, M. X. Cai, R. Spurzem, M. B. N. Kouwenhoven, S. Portegies Zwart

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    title = {{On the survival of resonant and non-resonant planetary systems in star clusters}},
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    year = 2020,
    month = jul,
    volume = {497},
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    archiveprefix = {arXiv},
    eprint = {2007.11601},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  125. S. Gill, P. J. Wheatley, B. F. Cooke, A. Jordán, L. D. Nielsen, D. Bayliss, D. R. Anderson, J. I. Vines, M. Lendl, J. S. Acton, D. J. Armstrong, F. Bouchy, R. Brahm, E. M. Bryant, M. R. Burleigh, S. L. Casewell, P. Eigmüller, N. Espinoza, E. Gillen, M. R. Goad, N. Grieves, M. N. Günther, T. Henning, M. J. Hobson, A. Hogan, J. S. Jenkins, J. McCormac, M. Moyano, H. P. Osborn, D. Pollacco, D. Queloz, H. Rauer, L. Raynard, F. Rojas, P. Sarkis, A. M. S. Smith, M. Tala-Pinto, R. H. Tilbrook, S. Udry, C. A. Watson, R. G. West

    NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event

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    title = {{NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event}},
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    keywords = {Exoplanet astronomy, Exoplanet detection methods, Exoplanets, Extrasolar gas giants, Photometry, High resolution spectroscopy, 486, 489, 498, 509, 1234, 2096, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    eprint = {2005.00006},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...898L..11G},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  126. M. Scheucher, F. Wunderlich, J. L. Grenfell, M. Godolt, F. Schreier, D. Kappel, R. Haus, K. Herbst, H. Rauer

    Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module

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    title = {{Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module}},
    journal = {\apj},
    keywords = {Radiative transfer simulations, Radiative transfer, Computational methods, Exoplanets, Extrasolar rocky planets, Exoplanet atmospheres, Planetary atmospheres, Mini Neptunes, Super Earths, 1967, 1335, 1965, 498, 511, 487, 1244, 1063, 1655, Astrophysics - Earth and Planetary Astrophysics},
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    eid = {44},
    pages = {44},
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    archiveprefix = {arXiv},
    eprint = {2005.02114},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...898...44S},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  127. P. Bluhm, R. Luque, N. Espinoza, J. A. Caballero, S. Dreizler, J. H. Livingston, S. Mathur, A. Quirrenbach, S. Stock, V. Van Eylen, G. Nowak, E. D. Lopez, S. Csizmadia, M. R. Zapatero Osorio, P. Schöfer, J. Lillo-Box, M. Oshagh, E. González-Álvarez, P. J. Amado, D. Barrado, V. J. S. Béjar, B. Cale, P. Chaturvedi, C. Cifuentes, W. D. Cochran, K. A. Collins, K. I. Collins, M. Cortés-Contreras, E. Díez Alonso, M. El Mufti, A. Ercolino, M. Fridlund, E. Gaidos, R. A. García, I. Georgieva, L. González-Cuesta, P. Guerra, A. P. Hatzes, T. Henning, E. Herrero, D. Hidalgo, G. Isopi, S. V. Jeffers, J. M. Jenkins, E. L. N. Jensen, P. Kabáth, A. Kaminski, J. Kemmer, J. Korth, D. E. Kossakowski, M. Kürster, M. Lafarga, F. Mallia, D. Montes, J. C. Morales, M. Morales-Calderón, F. Murgas, N. Narita, V. M. Passegger, S. Pedraz, C. M. Persson, P. Plavchan, H. Rauer, S. Redfield, S. Reffert, A. Reiners, I. Ribas, G. R. Ricker, C. Rodríguez López, A. R. G. Santos, S. Seager, M. Schlecker, A. Schweitzer, Y. Shan, M. G. Soto, J. Subjak, L. Tal-Or, T. Trifonov, S. Vanaverbeke, R. Vanderspek, J. Wittrock, M. Zechmeister, F. Zohrabi

    Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?

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    title = {{Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?}},
    journal = {\aap},
    keywords = {techniques: photometric, techniques: radial velocities, stars: individual: TOI-1235, stars: late-type, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
    volume = {639},
    eid = {A132},
    pages = {A132},
    doi = {10.1051/0004-6361/202038160},
    archiveprefix = {arXiv},
    eprint = {2004.06218},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A.132B},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  128. M. Lombart, G. Chauvin, P. Rojo, E. Lagadec, P. Delorme, H. Beust, M. Bonnefoy, R. Galicher, R. Gratton, D. Mesa, M. Bonavita, F. Allard, A. Bayo, A. Boccaletti, S. Desidera, J. Girard, J. S. Jenkins, H. Klahr, G. Laibe, A. M. Lagrange, C. Lazzoni, G.-D. Marleau, D. Minniti, C. Mordasini

    VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures

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    title = {{VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures}},
    journal = {\aap},
    keywords = {techniques: imaging spectroscopy, planets and satellites: detection, planets and satellites: fundamental parameters, planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    eid = {A54},
    pages = {A54},
    doi = {10.1051/0004-6361/202037961},
    archiveprefix = {arXiv},
    eprint = {2005.08850},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..54L},
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    }

    DOI arXiv
  129. G. Guilluy, V. Andretta, F. Borsa, P. Giacobbe, A. Sozzetti, E. Covino, V. Bourrier, L. Fossati, A. S. Bonomo, M. Esposito, M. S. Giampapa, A. Harutyunyan, M. Rainer, M. Brogi, G. Bruno, R. Claudi, G. Frustagli, A. F. Lanza, L. Mancini, L. Pino, E. Poretti, G. Scandariato, L. Affer, C. Baffa, A. Baruffolo, S. Benatti, K. Biazzo, A. Bignamini, W. Boschin, I. Carleo, M. Cecconi, R. Cosentino, M. Damasso, S. Desidera, G. Falcini, A. F. Martinez Fiorenzano, A. Ghedina, E. González-Álvarez, J. Guerra, N. Hernandez, G. Leto, A. Maggio, L. Malavolta, J. Maldonado, G. Micela, E. Molinari, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, A. Reiners

    The GAPS programme at TNG. XXII. The GIARPS view of the extended helium atmosphere of HD 189733 b accounting for stellar activity

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    title = {{The GAPS programme at TNG. XXII. The GIARPS view of the extended helium atmosphere of HD 189733 b accounting for stellar activity}},
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, planets and satellites: fundamental parameters, techniques: spectroscopic, planets and satellites: individual: HD 189733 b, stars: activity, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    eid = {A49},
    pages = {A49},
    doi = {10.1051/0004-6361/202037644},
    archiveprefix = {arXiv},
    eprint = {2005.05676},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..49G},
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    }

    DOI arXiv
  130. D. Shulyak, L. M. Lara, M. Rengel, N. E. Nèmec

    Stellar impact on disequilibrium chemistry and observed spectra of hot Jupiter atmospheres

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    title = {{Stellar impact on disequilibrium chemistry and observed spectra of hot Jupiter atmospheres}},
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, planets and satellites: composition, stars: activity, methods: numerical, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
    volume = {639},
    eid = {A48},
    pages = {A48},
    doi = {10.1051/0004-6361/201937210},
    archiveprefix = {arXiv},
    eprint = {2005.01470},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..48S},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  131. S. Hojjatpanah, M. Oshagh, P. Figueira, N. C. Santos, E. M. Amazo-Gómez, S. G. Sousa, V. Adibekyan, B. Akinsanmi, O. Demangeon, J. Faria, J. Gomes da Silva, N. Meunier

    The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations

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    title = {{The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations}},
    journal = {\aap},
    keywords = {techniques: spectroscopic, planets and satellites: detection, techniques: radial velocities, techniques: photometric, stars: activity, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    doi = {10.1051/0004-6361/202038035},
    archiveprefix = {arXiv},
    eprint = {2005.10105},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..35H},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  132. S. V. Jeffers, S. Dreizler, J. R. Barnes, C. A. Haswell, R. P. Nelson, E. Rodríguez, M. J. López-González, N. Morales, R. Luque, M. Zechmeister, S. S. Vogt, J. S. Jenkins, Z. M. Berdiñas, G. A. L. Coleman, M. R. Díaz, I. Ribas, H. R. A. Jones, R. P. Butler, C. G. Tinney, J. Bailey, B. D. Carter, S. O'Toole, R. A. Wittenmyer, J. D. Crane, F. Feng, S. A. Shectman, J. Teske, A. Reiners, P. J. Amado, G. Anglada-Escudé

    A multiplanet system of super-Earths orbiting the brightest red dwarf star GJ 887

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    title = {{A multiplanet system of super-Earths orbiting the brightest red dwarf star GJ 887}},
    journal = {Science},
    keywords = {ASTRONOMY; PLANET SCI, Astrophysics - Earth and Planetary Astrophysics},
    year = 2020,
    month = jun,
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    pages = {1477-1481},
    doi = {10.1126/science.aaz0795},
    archiveprefix = {arXiv},
    eprint = {2006.16372},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020Sci...368.1477J},
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    DOI arXiv
  133. N. R. Deacon, A. L. Kraus

    Wide binaries are rare in open clusters

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    author = {{Deacon}, N.~R. and {Kraus}, A.~L.},
    title = {{Wide binaries are rare in open clusters}},
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    keywords = {binaries: visual, stars: formation, open clusters and associations: individual, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
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    month = jun,
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    number = {4},
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    doi = {10.1093/mnras/staa1877},
    archiveprefix = {arXiv},
    eprint = {2006.06679},
    primaryclass = {astro-ph.SR},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.5176D},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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    DOI arXiv
  134. S. C. Eriksson, R. Asensio-Torres, M. Janson, Y. Aoyama, G.-D. Marleau, M. Bonnefoy, S. Petrus

    Strong Hα emission and signs of accretion in a circumbinary planetary mass companion from MUSE

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    title = {{Strong H{\ensuremath{\alpha}} emission and signs of accretion in a circumbinary planetary mass companion from MUSE}},
    journal = {\aap},
    keywords = {planets and satellites: individual: 2MASS J01033563-5515561 (AB)b (Delorme 1 (AB)b), planetary systems, accretion, accretion disks, stars: low-mass, techniques: imaging spectroscopy, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    month = jun,
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    eid = {L6},
    pages = {L6},
    doi = {10.1051/0004-6361/202038131},
    archiveprefix = {arXiv},
    eprint = {2005.11725},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638L...6E},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  135. A. Bhandare, R. Kuiper, T. Henning, C. Fendt, M. Flock, G.-D. Marleau

    Birth of convective low-mass to high-mass second Larson cores

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    author = {{Bhandare}, Asmita and {Kuiper}, Rolf and {Henning}, Thomas and {Fendt}, Christian and {Flock}, Mario and {Marleau}, Gabriel-Dominique},
    title = {{Birth of convective low-mass to high-mass second Larson cores}},
    journal = {\aap},
    keywords = {stars: formation, methods: numerical, hydrodynamics, radiative transfer, equation of state, convection, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Computational Physics},
    year = 2020,
    month = jun,
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    eid = {A86},
    pages = {A86},
    doi = {10.1051/0004-6361/201937029},
    archiveprefix = {arXiv},
    eprint = {2004.12419},
    primaryclass = {astro-ph.SR},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638A..86B},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
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    DOI arXiv
  136. L. Nortmann, N. Casasayas-Barris, M. Lampón, M. López-Puertas, J. A. Caballero, J. Sanz-Forcada, L. M. Lara, E. Nagel, F. Yan, F. J. Alonso-Floriano, P. J. Amado, G. Chen, C. Cifuentes, M. Cortés-Contreras, S. Czesla, K. Molaverdikhani, D. Montes, V. M. Passegger, A. Quirrenbach, A. Reiners, I. Ribas, A. Sánchez-López, A. Schweitzer, M. Stangret, M. R. Zapatero Osorio, M. Zechmeister

    A He I upper atmosphere around the warm Neptune GJ 3470 b

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    title = {{A He I upper atmosphere around the warm Neptune GJ 3470 b}},
    journal = {\aap},
    keywords = {planetary systems, planets and satellites: atmospheres, planet-star interactions, planets and satellites: general, planets and satellites: individual: GJ 3470b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jun,
    volume = {638},
    eid = {A61},
    pages = {A61},
    doi = {10.1051/0004-6361/202037719},
    archiveprefix = {arXiv},
    eprint = {2004.12812},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638A..61P},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  137. M. Stangret, N. Casasayas-Barris, F. Yan, A. Sánchez-López, M. López-Puertas

    Detection of Fe I and Fe II in the atmosphere of MASCARA-2b using a cross-correlation method

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    title = {{Detection of Fe I and Fe II in the atmosphere of MASCARA-2b using a cross-correlation method}},
    journal = {\aap},
    keywords = {planetary systems, planets and satellites: individual: MASCARA2-b, planets and satellites: atmospheres, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jun,
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    doi = {10.1051/0004-6361/202037541},
    archiveprefix = {arXiv},
    eprint = {2003.04650},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638A..26S},
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    DOI arXiv
  138. S. Gill, B. F. Cooke, D. Bayliss, L. D. Nielsen, M. Lendl, P. J. Wheatley, D. R. Anderson, M. Moyano, E. M. Bryant, J. S. Acton, C. Belardi, F. Bouchy, M. R. Burleigh, S. L. Casewell, A. Chaushev, M. R. Goad, J. A. G. Jackman, J. S. Jenkins, J. McCormac, M. N. Günther, H. P. Osborn, D. Pollacco, L. Raynard, A. M. S. Smith, R. H. Tilbrook, J. D. Turner, S. Udry, J. I. Vines, C. A. Watson, R. G. West

    A long-period (P = 61.8 d) M5V dwarf eclipsing a Sun-like star from TESS and NGTS

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    Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M super-Earth and two warm 14.7 and 10.2-M sub-Neptunes

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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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  142. E. M. Amazo-Gómez, A. I. Shapiro, S. K. Solanki, N. A. Krivova, G. Kopp, T. Reinhold, M. Oshagh, A. Reiners

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    Prox Centauri b: A strong case for including Cosmic-Ray-induced Chemistry in Atmospheric Biosignatures Studies

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  146. S. Boldt, M. Oshagh, S. Dreizler, M. Mallonn, N. C. Santos, A. Claret, A. Reiners, E. Sedaghati

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    Is there Na I in the atmosphere of HD 209458b?. Effect of the centre-to-limb variation and Rossiter-McLaughlin effect in transmission spectroscopy studies

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    primaryclass = {astro-ph.EP},
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    TOI-132 b: A short-period planet in the Neptune desert transiting a V = 11.3 G-type star★

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    primaryclass = {astro-ph.EP},
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    RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061

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    {Zechmeister}, M. and {Barnes}, J.~R. and {Haswell}, C.~A. and
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    {Anglada-Escud{\'e}}, G.},
    title = {{RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061}},
    journal = {\mnras},
    keywords = {methods: data analysis, techniques: radial velocities, stars: individual: GJ 1061, stars: late-type, planetary systems, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = mar,
    volume = {493},
    number = {1},
    pages = {536-550},
    doi = {10.1093/mnras/staa248},
    archiveprefix = {arXiv},
    eprint = {1908.04717},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.493..536D},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

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  152. J. P. Faria, V. Adibekyan, E. M. Amazo-Gómez, S. C. C. Barros, J. D. Camacho, O. Demangeon, P. Figueira, A. Mortier, M. Oshagh, F. Pepe, N. C. Santos, J. Gomes da Silva, A. R. Costa Silva, S. G. Sousa, S. Ulmer-Moll, P. T. P. Viana

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    eprint = {1911.11714},
    primaryclass = {astro-ph.EP},
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  153. J. McCormac, E. Gillen, J. A. G. Jackman, D. J. A. Brown, D. Bayliss, P. J. Wheatley, D. R. Anderson, D. J. Armstrong, F. Bouchy, J. T. Briegal, M. R. Burleigh, J. Cabrera, S. L. Casewell, A. Chaushev, B. Chazelas, P. Chote, B. F. Cooke, J. C. Costes, S. Csizmadia, P. Eigmüller, A. Erikson, E. Foxell, B. T. Gänsicke, M. R. Goad, M. N. Günther, S. T. Hodgkin, M. J. Hooton, J. S. Jenkins, G. Lambert, M. Lendl, E. Longstaff, T. Louden, M. Moyano, L. D. Nielsen, D. Pollacco, D. Queloz, H. Rauer, L. Raynard, A. M. S. Smith, B. Smalley, M. G. Soto, O. Turner, S. Udry, J. I. Vines, S. R. Walker, C. A. Watson, R. G. West

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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    title = {{RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061}},
    journal = {\mnras},
    keywords = {methods: data analysis, techniques: radial velocities, stars: individual: GJ 1061, stars: late-type, planetary systems, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = mar,
    volume = {493},
    number = {1},
    pages = {536-550},
    doi = {10.1093/mnras/staa248},
    archiveprefix = {arXiv},
    eprint = {1908.04717},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.493..536D},
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  155. J. Wicht, W. Dietrich, P. Wulff, U. R. Christensen

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    primaryclass = {astro-ph.EP},
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  156. K. W. F. Lam, J. Korth, K. Masuda, S. Csizmadia, P. Eigmüller, G. Kári Stefánsson, M. Endl, S. Albrecht, P. Robertson, R. Luque, J. H. Livingston, T. Hirano, R. Alonso Sobrino, O. Barragán, J. Cabrera, I. Carleo, A. Chaushev, W. D. Cochran, F. Dai, J. de Leon, H. J. Deeg, A. Erikson, M. Esposito, M. Fridlund, A. Fukui, D. Gandolfi, I. Georgieva, L. González-Cuesta, S. Grziwa, E. W. Guenther, A. P. Hatzes, D. Hidalgo, M. Hjorth, P. Kabáth, E. Knudstrup, M. N. Lund, S. Mahadevan, S. Mathur, P. Montañés-Rodríguez, F. Murgas, N. Narita, D. Nespral,, P. Niraula, M. Pätzold, C. M. Persson, J. Prieto-Arranz, H. Rauer, S. Redfield, I. Ribas, M. Skarka, A. M. S. Smith, J. Subjak, V. Van Eylen

    It Takes Two Planets in Resonance to Tango around K2-146

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    title = {{It Takes Two Planets in Resonance to Tango around K2-146}},
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    eid = {120},
    pages = {120},
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    archiveprefix = {arXiv},
    eprint = {1907.11141},
    primaryclass = {astro-ph.EP},
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    Is there Na I in the atmosphere of HD 209458b?. Effect of the centre-to-limb variation and Rossiter-McLaughlin effect in transmission spectroscopy studies

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    primaryclass = {astro-ph.EP},
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    ISPY-NACO Imaging Survey for Planets around Young stars. Survey description and results from the first 2.5 years of observations

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    eprint = {2002.01807},
    primaryclass = {astro-ph.EP},
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    primaryclass = {astro-ph.IM},
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    title = {{Spitzer Microlensing Parallax Reveals Two Isolated Stars in the Galactic Bulge}},
    journal = {\apj},
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    DOI arXiv
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    DOI arXiv
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    DOI arXiv
  174. C. N. Kimmig, C. P. Dullemond, W. Kley

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    DOI arXiv
  175. M. Küffmeier, F. G. Goicovic, C. P. Dullemond

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    DOI arXiv
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    DOI arXiv
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    DOI arXiv
  178. F. Yan, N. Casasayas-Barris, K. Molaverdikhani, F. J. Alonso-Floriano, A. Reiners, T. Henning, P. Mollière, G. Chen, L. Nortmann, I. A. G. Snellen, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, M. Azzaro, F. F. Bauer, M. Cortés-Contreras, S. Czesla, S. Khalafinejad, L. M. Lara, M. López-Puertas, D. Montes, E. Nagel, M. Oshagh, A. Sánchez-López, M. Stangret, M. Zechmeister

    Ionized calcium in the atmospheres of two ultra-hot exoplanets WASP-33b and KELT-9b

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    VLT/SPHERE exploration of the young multiplanetary system PDS70

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    DOI arXiv
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    Radial velocity confirmation of K2-100b: a young, highly irradiated, and low-density transiting hot Neptune

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    DOI arXiv
  181. Grégoire Montavon, Jasmine MacKenzie, Nadine Nettelmann, Nicola Tosi, Philipp Baumeister, Sebastiano Padovan, Mareike Godolt

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    DOI arXiv
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    {Spurzem}, Rainer},
    title = {{On the survivability of planets in young massive clusters and its implication of planet orbital architectures in globular clusters}},
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    month = nov,
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    pages = {4311-4321},
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    DOI arXiv
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    month = nov,
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    Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star

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    DOI arXiv
  185. J. I. Vines, J. S. Jenkins, J. S. Acton, J. T. Briegal, D. Bayliss, F. Bouchy, C. Belardi, E. M. Bryant, M. R. Burleigh, J. Cabrera, S. L. Casewell, A. Chaushev, B. F. Cooke, S. Csizmadia, P. Eigmüller, A. Erikson, E. Foxell, S. Gill, E. Gillen, M. R. Goad, J. A. G. Jackman, G. W. King, T. Louden, J. McCormac, M. Moyano, L. D. Nielsen, D. Pollacco, D. Queloz, H. Rauer, L. Raynard, A. M. S. Smith, M. G. Soto, R. H. Tilbrook, R. Titz-Weider, J. D. Turner, S. Udry, S. R. Walker, C. A. Watson, R. G. West, P. J. Wheatley

    NGTS-6b: an ultrashort period hot-Jupiter orbiting an old K dwarf

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    OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf

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    month = nov,
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    pages = {4311-4321},
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  187. R. Luque, T. Trifonov, S. Reffert, A. Quirrenbach, M. H. Lee, S. Albrecht, M. Fredslund Andersen, V. Antoci, F. Grundahl, C. Schwab, V. Wolthoff

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  189. A. Leleu, G. A. L. Coleman, S. Ataiee

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    DOI arXiv
  190. A. Bignamini, C. Lovis, D. Mesa, D. Nardiello, E. Covino, L. Malavolta, M. Damasso, M. Esposito, S. Messina, S. Sabotta, V. D'Orazi, V. Nascimbeni, L. Borsato, R. Claudi, S. Benatti, S. Desidera

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  192. F. Flammini Dotti, M. B. N. Kouwenhoven, M. X. Cai, R. Spurzem

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  193. A. García Muñoz, P. C. Schneider

    Rapid Escape of Ultra-hot Exoplanet Atmospheres Driven by Hydrogen Balmer Absorption

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  194. S. Sabotta, P. Kabáth, J. Korth, E. W. Guenther, D. Dupkala, S. Grziwa, T. Klocova, M. Skarka

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  199. J. Wicht, T. Gastine, L. D. V. Duarte, W. Dietrich

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    DOI arXiv
  203. Y. Tsapras, A. Cassan, C. Ranc, E. Bachelet, R. Street, A. Udalski, M. Hundertmark, V. Bozza, J. P. Beaulieu, J. B. Marquette, E. Euteneuer, D. M. Bramich, M. Dominik, R. Figuera Jaimes, K. Horne, S. Mao, J. Menzies, R. Schmidt, C. Snodgrass, I. A. Steele, J. Wambsganss, P. Mróz, M. K. Szymański, I. Soszyński, J. Skowron, P. Pietrukowicz, R. Poleski, K. Ulaczyk, M. Pawlak, U. G. Jørgensen, J. Skottfelt, A. Popovas, S. Ciceri, H. Korhonen, M. Küffmeier, D. F. Evans, N. Peixinho, T. C. Hinse, M. J. Burgdorf, J. Southworth, R. Tronsgaard, E. Kerins, M. I. Andersen, S. Rahvar, Y. Wang, O. Wertz, M. Rabus, S. Calchi Novati, G. D'Ago, G. Scarpetta, L. Mancini, F. Abe, Y. Asakura, D. P. Bennett, A. Bhattacharya, M. Donachie, P. Evans, A. Fukui, Y. Hirao, Y. Itow, K. Kawasaki, N. Koshimoto, M. C. A. Li, C. H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, S. Miyazaki, M. Nagakane, K. Ohnishi, N. Rattenbury, T. Saito, A. Sharan, H. Shibai, D. J. Sullivan, T. Sumi, D. Suzuki, P. J. Tristram, T. Yamada, A. Yonehara, Robonet Team, OGLE Collaboration

    An analysis of binary microlensing event OGLE-2015-BLG-0060

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    title = {{An analysis of binary microlensing event OGLE-2015-BLG-0060}},
    journal = {\mnras},
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    year = 2019,
    month = aug,
    volume = {487},
    number = {4},
    pages = {4603-4614},
    doi = {10.1093/mnras/stz1404},
    archiveprefix = {arXiv},
    eprint = {1906.02630},
    primaryclass = {astro-ph.EP},
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    }

    DOI arXiv
  204. G.-D. Marleau, C. Mordasini, R. Kuiper

    The Planetary Accretion Shock. II. Grid of Postshock Entropies and Radiative Shock Efficiencies for Nonequilibrium Radiation Transport

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    journal = {\apj},
    keywords = {accretion, accretion disks, methods: analytical, methods: numerical, planets and satellites: formation, planets and satellites: gaseous planets, radiative transfer, Astrophysics - Earth and Planetary Astrophysics},
    year = 2019,
    month = aug,
    volume = {881},
    number = {2},
    eid = {144},
    pages = {144},
    doi = {10.3847/1538-4357/ab245b},
    archiveprefix = {arXiv},
    eprint = {1906.05869},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  205. D. K. Sing, P. Lavvas, G. E. Ballester, A. Lecavelier des Etangs, M. S. Marley, N. Nikolov, L. Ben-Jaffel, V. Bourrier, L. A. Buchhave, D. L. Deming, D. Ehrenreich, T. Mikal-Evans, T. Kataria, N. K. Lewis, M. López-Morales, A. García Muñoz, G. W. Henry, J. Sanz-Forcada, J. J. Spake, R. Wakeford, PanCET Collaboration

    The Hubble Space Telescope PanCET Program: Exospheric Mg II and Fe II in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation

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    title = {{The Hubble Space Telescope PanCET Program: Exospheric Mg II and Fe II in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation}},
    journal = {\aj},
    keywords = {planets and satellites: atmospheres, stars: individual: WASP-121, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics},
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    month = aug,
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    eprint = {1908.00619},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  206. C. M. Persson, S. Csizmadia, A. J. Mustill, M. Fridlund, A. P. Hatzes, G. Nowak, I. Georgieva, D. Gandolfi, M. B. Davies, J. H. Livingston, P. Montañés-Rodríguez, M. Endl, T. Hirano, J. Prieto-Arranz, J. Korth, S. Grziwa, M. Esposito, S. Albrecht, M. C. Johnson, O. Barragán, H. Parviainen, V. Van Eylen, R. Alonso Sobrino, P. G. Beck, J. Cabrera, I. Carleo, W. D. Cochran, F. Dai, H. J. Deeg, J. P. de Leon, P. Eigmüller, A. Erikson, A. Fukui, L. González-Cuesta, E. W. Guenther, D. Hidalgo, M. Hjorth, P. Kabáth, E. Knudstrup, N. Kusakabe, K. W. F. Lam, M. N. Lund, R. Luque, S. Mathur, F. Murgas, N. Narita, D. Nespral,, P. Niraula, A. O. Henrik Olofsson, M. Pätzold, H. Rauer, S. Redfield, I. Ribas, M. Skarka, A. M. S. Smith, J. Subjak, M. Tamura

    Greening of the brown-dwarf desert. EPIC 212036875b: a 51 MJ object in a 5-day orbit around an F7 V star

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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  207. D. Höning, N. Tosi, T. Spohn

    Carbon cycling and interior evolution of water-covered plate tectonics and stagnant-lid planets

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    journal = {\aap},
    keywords = {planets and satellites: interiors, planets and satellites: surfaces, planets and satellites: oceans, planets and satellites: atmospheres, planets and satellites: tectonics, planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
    year = 2019,
    month = jul,
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    pages = {A48},
    doi = {10.1051/0004-6361/201935091},
    archiveprefix = {arXiv},
    eprint = {1905.12392},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...627A..48H},
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    }

    DOI arXiv
  208. R. G. West, E. Gillen, D. Bayliss, M. R. Burleigh, L. Delrez, M. N. Günther, S. T. Hodgkin, J. A. G. Jackman, J. S. Jenkins, G. W. King, J. McCormac, L. D. Nielsen, L. Raynard, A. M. S. Smith, M. Soto, O. Turner, P. J. Wheatley, Y. Almleaky, D. J. Armstrong, C. Belardi, F. Bouchy, J. T. Briegal, A. Burdanov, J. Cabrera, S. L. Casewell, A. Chaushev, B. Chazelas, P. Chote, B. F. Cooke, S. Csizmadia, E. Ducrot, P. Eigmüller, A. Erikson, E. Foxell, B. T. Gänsicke, M. Gillon, M. R. Goad, E. Jehin, G. Lambert, E. S. Longstaff, T. Louden, M. Moyano, C. Murray, D. Pollacco, D. Queloz, H. Rauer, S. Sohy, S. J. Thompson, S. Udry, S. R. Walker, C. A. Watson

    NGTS-4b: A sub-Neptune transiting in the desert

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    title = {{NGTS-4b: A sub-Neptune transiting in the desert}},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  209. D. Veras, M. Efroimsky, V. V. Makarov, G. Boué, V. Wolthoff, S. Reffert, A. Quirrenbach, E. P. Tremblay, B. T. Gänsicke

    Orbital relaxation and excitation of planets tidally interacting with white dwarfs

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    DOI arXiv
  210. A. Musso Barcucci, R. Launhardt, G. M. Kennedy, H. Avenhaus, S. S. Brems, R. van Boekel, F. Cantalloube, A. Cheetham, G. Cugno, J. Girard, N. Godoy, T. K. Henning, S. Metchev, A. Müller, J. Olofsson, F. Pepe, S. P. Quanz, A. Quirrenbach, S. Reffert, E. L. Rickman, M. Samland, D. Ségransan

    ISPY – NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring

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    journal = {\aap},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  211. N. R. Deacon, T. Henning, D. E. Kossakowski

    Data-driven stellar parameters for southern TESS FGK targets

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    month = jun,
    volume = {486},
    number = {1},
    pages = {251-265},
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    primaryclass = {astro-ph.SR},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486..251D},
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    DOI arXiv
  212. M. Janson, R. Asensio-Torres, D. André, M. Bonnefoy, P. Delorme, S. Reffert, S. Desidera, M. Langlois, G. Chauvin, R. Gratton, A. J. Bohn, S. C. Eriksson, G.-D. Marleau, A. Vigan, J. C. Carson

    The B-Star Exoplanet Abundance Study: a co-moving 16-25 MJup companion to the young binary system HIP 79098

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    keywords = {brown dwarfs, stars: early-type, planets and satellites: detection, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    volume = {626},
    eid = {A99},
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    eprint = {1906.02787},
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    DOI arXiv
  213. P. Lavvas, T. Koskinen, M. E. Steinrueck, A. García Muñoz, A. P. Showman

    Photochemical Hazes in Sub-Neptunian Atmospheres with a Focus on GJ 1214bLavvas

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    title = {{Photochemical Hazes in Sub-Neptunian Atmospheres with a Focus on GJ 1214b}},
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    keywords = {planets and satellites: atmospheres, planets and satellites: gaseous planets, planets and satellites: individual: GJ 1214b, Astrophysics - Earth and Planetary Astrophysics},
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    month = jun,
    volume = {878},
    number = {2},
    eid = {118},
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    DOI arXiv
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  216. M. Godolt, N. Tosi, B. Stracke, J. Lee Grenfell, T. Ruedas, T. Spohn, H. Rauer

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  218. M. Keppler, R. Teague, J. Bae, M. Benisty, T. Henning, R. van Boekel, E. Chapillon, P. Pinilla, J. P. Williams, G. H. M. Bertrang, S. Facchini, M. Flock, C. Ginski, A. Juhasz, H. Klahr, Y. Liu, A. Müller, L. M. Pérez, A. Pohl, G. Rosotti, M. Samland, D. Semenov

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    DOI arXiv
  227. K. Monsch, B. Ercolano, G. Picogna, T. Preibisch, M. M. Rau

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    number = {3},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  228. T. Trifonov, S. Stock, T. Henning, S. Reffert, M. Kürster, M. H. Lee, B. Bitsch, R. P. Butler, S. S. Vogt

    Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?

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  229. R. Luque, G. Nowak, F. Dai, A. Kaminski, E. Nagel, D. Hidalgo, F. Bauer, M. Lafarga, J. Livingston, O. Barragán, T. Hirano, M. Fridlund, D. Gandolfi, A. B. Justesen, M. Hjorth, V. Van Eylen, J. N. Winn, M. Esposito, J. C. Morales, S. Albrecht, R. Alonso, P. J. Amado, P. Beck, J. A. Caballero, J. Cabrera, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, A. Fukui, S. Grziwa, E. W. Guenther, A. P. Hatzes, E. Knudstrup, J. Korth, K. W. F. Lam, M. N. Lund, S. Mathur, P. Montañés-Rodríguez, N. Narita, D. Nespral,, P. Niraula, M. Pätzold, C. M. Persson, J. Prieto-Arranz, A. Quirrenbach, H. Rauer, S. Redfield, A. Reiners, I. Ribas, A. M. S. Smith

    Detection and characterization of an ultra-dense sub-Neptunian planet orbiting the Sun-like star K2-292

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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  230. E. F. Linder, C. Mordasini, P. Mollière, G.-D. Marleau, M. Malik, S. P. Quanz, M. R. Meyer

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    DOI arXiv
  231. D. Ó Fionnagáin, A. A. Vidotto, P. Petit, C. P. Folsom, S. V. Jeffers, S. C. Marsden, J. Morin, J. D. do Nascimento, BCool Collaboration

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    DOI arXiv
  232. J. Korth, S. Csizmadia, D. Gandolfi, M. Fridlund, M. Pätzold, T. Hirano, J. Livingston, C. M. Persson, H. J. Deeg, A. B. Justesen, O. Barragán, S. Grziwa, M. Endl, R. Tronsgaard, F. Dai, W. D. Cochran, S. Albrecht, R. Alonso, J. Cabrera, P. W. Cauley, F. Cusano, P. Eigmüller, A. Erikson, M. Esposito, E. W. Guenther, A. P. Hatzes, D. Hidalgo, M. Kuzuhara, P. Montañes, N. R. Napolitano, N. Narita, P. Niraula, D. Nespral,, G. Nowak, C. E. Petrillo, S. Redfield, J. Prieto-Arranz, H. Rauer, A. M. S. Smith, C. Tortora, V. Van Eylen, J. N. Winn

    K2-140b and K2-180b – Characterization of a hot Jupiter and a mini-Neptune from the K2 mission

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    DOI arXiv
  233. S. Boro Saikia, T. Lueftinger, S. V. Jeffers, C. P. Folsom, V. See, P. Petit, S. C. Marsden, A. A. Vidotto, J. Morin, A. Reiners, M. Guedel, BCool Collaboration

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  234. N. R. Deacon

    Detecting free-floating planets using water-dependent colour terms in the next generation of infrared space-based surveys

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    DOI arXiv
  235. W. Dietrich, J. Wicht

    Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells

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    DOI arXiv
  236. D. Gandolfi, O. Barragán, J. H. Livingston, M. Fridlund, A. B. Justesen, S. Redfield, L. Fossati, S. Mathur, S. Grziwa, J. Cabrera, R. A. García, C. M. Persson, V. Van Eylen, A. P. Hatzes, D. Hidalgo, S. Albrecht, L. Bugnet, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, M. Esposito, E. Guenther, J. Korth, R. Luque, P. Montañés-Rodríguez, D. Nespral,, G. Nowak, M. Pätzold, J. Prieto-Arranz

    TESS’s first planet. A super-Earth transiting the naked-eye star π Mensae

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    DOI arXiv
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    K2-260 b: a hot Jupiter transiting an F star, and K2-261 b: a warm Saturn around a bright G star

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    Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)Prieto-Arranz

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    title = {{Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)}},
    journal = {\aap},
    keywords = {planetary systems, techniques: high angular resolution, techniques: photometric, techniques: radial velocities, stars: abundances, stars: individual: GJ 9827, Astrophysics - Earth and Planetary Astrophysics},
    year = 2018,
    month = oct,
    volume = {618},
    eid = {A116},
    pages = {A116},
    doi = {10.1051/0004-6361/201832872},
    archiveprefix = {arXiv},
    eprint = {1802.09557},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...618A.116P},
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  240. C. M. Persson, M. Fridlund, O. Barragán, F. Dai, D. Gandolfi, A. P. Hatzes, T. Hirano, S. Grziwa, J. Korth, J. Prieto-Arranz, L. Fossati, V. Van Eylen, A. B. Justesen, J. Livingston, D. Kubyshkina, H. J. Deeg, E. W. Guenther, G. Nowak, J. Cabrera, P. Eigmüller, S. Csizmadia, A. M. S. Smith, A. Erikson, S. Albrecht, R. Alonso Sobrino, W. D. Cochran, M. Endl, M. Esposito, A. Fukui, P. Heeren, D. Hidalgo, M. Hjorth, M. Kuzuhara, N. Narita, D. Nespral,, M. Pätzold, H. Rauer, F. Rodler, J. N. Winn

    Super-Earth of 8 M in a 2.2-day orbit around the K5V star K2-216

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    archiveprefix = {arXiv},
    eprint = {1805.04774},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...618A..33P},
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    Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)

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    title = {{Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)}},
    journal = {\aap},
    keywords = {planetary systems, techniques: high angular resolution, techniques: photometric, techniques: radial velocities, stars: abundances, stars: individual: GJ 9827, Astrophysics - Earth and Planetary Astrophysics},
    year = 2018,
    month = oct,
    volume = {618},
    eid = {A116},
    pages = {A116},
    doi = {10.1051/0004-6361/201832872},
    archiveprefix = {arXiv},
    eprint = {1802.09557},
    primaryclass = {astro-ph.EP},
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    eprint = {1810.02691},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2018Geosc...8..365T},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

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    Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk

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    title = {{Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk}},
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    primaryclass = {astro-ph.EP},
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    Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b

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    primaryclass = {astro-ph.EP},
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    DOI arXiv
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