C
Clara Sousa-Silva
Researcher at Massachusetts Institute of Technology
Publications - 63
Citations - 2146
Clara Sousa-Silva is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Exoplanet & Venus. The author has an hindex of 17, co-authored 58 publications receiving 1347 citations. Previous affiliations of Clara Sousa-Silva include Jožef Stefan Institute & Harvard University.
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Journal ArticleDOI
The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres
Jonathan Tennyson,Sergei N. Yurchenko,Ahmed Al-Refaie,Emma J. Barton,Katy L. Chubb,Phillip A. Coles,S. Diamantopoulou,Maire N. Gorman,Christian Hill,Aden Lam,Lorenzo Lodi,Laura K. McKemmish,Yueqi Na,Alec Owens,Oleg L. Polyansky,Tom Rivlin,Clara Sousa-Silva,Daniel S. Underwood,Andrey Yachmenev,Emil J. Zak +19 more
TL;DR: The ExoMol database as mentioned in this paper provides extensive line lists of molecular transitions which are valid over extended temperature ranges, including lifetimes of individual states, temperature-dependent cooling functions, Lande g-factors, partition functions, cross sections, k-coefficients and transition dipoles with phase relations.
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Phosphine gas in the cloud decks of Venus
Jane Greaves,Jane Greaves,Anita M. S. Richards,William Bains,Paul B. Rimmer,Paul B. Rimmer,Hideo Sagawa,David L. Clements,Sara Seager,Janusz J. Petkowski,Clara Sousa-Silva,Sukrit Ranjan,Emily Drabek-Maunder,Helen J. Fraser,Annabel Cartwright,Ingo Mueller-Wodarg,Zhuchang Zhan,Per Friberg,Iain Coulson,E’lisa Lee,Jim Hoge +20 more
TL;DR: In this paper, the apparent presence of PH3 gas in Venus's atmosphere, where any phosphorus should be in oxidized forms, has been inferred from single line millimetre-waveband spectral detections (quality up to ~15σ) from the JCMT and ALMA telescopes.
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The TESS Objects of Interest Catalog from the TESS Prime Mission
Natalia Guerrero,Sara Seager,Chelsea X. Huang,Andrew Vanderburg,Andrew Vanderburg,Aylin Garcia Soto,Ismael Mireles,Katharine Hesse,William Fong,Ana Glidden,Avi Shporer,David W. Latham,Karen A. Collins,Samuel N. Quinn,Jennifer Burt,Diana Dragomir,Ian J. M. Crossfield,Roland Vanderspek,Michael Fausnaugh,Christopher J. Burke,George R. Ricker,Tansu Daylan,Zahra Essack,Maximilian N. Günther,H. P. Osborn,H. P. Osborn,Joshua Pepper,Pamela Rowden,Lizhou Sha,Steven Villanueva,Daniel A. Yahalomi,Liang Yu,Sarah Ballard,Natalie M. Batalha,David Berardo,Ashley Chontos,Jason A. Dittmann,Gilbert A. Esquerdo,Thomas Mikal-Evans,Rahul Jayaraman,Akshata Krishnamurthy,Dana R. Louie,Nicholas Mehrle,Prajwal Niraula,Benjamin V. Rackham,Joseph E. Rodriguez,Stephen J. L. Rowden,Clara Sousa-Silva,David Watanabe,Ian Wong,Zhuchang Zhan,Goran Zivanovic,Jessie L. Christiansen,David R. Ciardi,M. Swain,Michael B. Lund,Susan E. Mullally,Scott W. Fleming,David R. Rodriguez,Patricia T. Boyd,Elisa V. Quintana,Thomas Barclay,Thomas Barclay,Knicole D. Colón,S. Rinehart,Joshua E. Schlieder,Mark Clampin,Jon M. Jenkins,Joseph D. Twicken,Joseph D. Twicken,Douglas A. Caldwell,Douglas A. Caldwell,Jeffrey L. Coughlin,Jeffrey L. Coughlin,Chris Henze,Jack J. Lissauer,Robert L. Morris,Robert L. Morris,Mark E. Rose,Jeffrey C. Smith,Jeffrey C. Smith,Peter Tenenbaum,Peter Tenenbaum,Eric B. Ting,Bill Wohler,Bill Wohler,Gáspár Á. Bakos,Jacob L. Bean,Zachory K. Berta-Thompson,Allyson Bieryla,Luke G. Bouma,Lars A. Buchhave,Nathaniel R. Butler,David Charbonneau,John P. Doty,Jian Ge,Matthew J. Holman,Andrew W. Howard,Lisa Kaltenegger,Stephen R. Kane,Hans Kjeldsen,Laura Kreidberg,Douglas N. C. Lin,Charlotte Minsky,Norio Narita,Martin Paegert,András Pál,Enric Palle,Dimitar Sasselov,Alton Spencer,Alessandro Sozzetti,Keivan G. Stassun,Keivan G. Stassun,Guillermo Torres,Stéphane Udry,Joshua N. Winn +115 more
TL;DR: In this article, the authors presented 2241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its 2-year Prime Mission.
Journal ArticleDOI
ExoMol line lists – VII. The rotation–vibration spectrum of phosphine up to 1500 K
TL;DR: In this article, a comprehensive hot line list is calculated for the ground electronic state of a star, called SAlTY, which contains almost 16.8 billion transitions between 7.5 million energy levels and is suitable for simulating spectra up to temperatures of 1500~K.
Journal ArticleDOI
Impact of Space Weather on Climate and Habitability of Terrestrial Type Exoplanets
Vladimir Airapetian,Rory Barnes,Ofer Cohen,Glyn Collinson,W. C. Danchi,Chuanfei Dong,A. D. Del Genio,K. Garcia-Sage,Alex Glocer,Nat Gopalswamy,John Lee Grenfell,Guillaume Gronoff,M. G% udel,Konstantin Herbst,W. G. Henning,Charles H. Jackman,Meng Jin,Colin P. Johnstone,Lisa Kaltenegger,Christina Kay,Kensei Kobayashi,W. Kuang,Gang Li,Benjamin J. Lynch,T. L% uftinger,Tj.G. Luhmann,Hiroyuki Maehara,Martin G. Mlynczak,Yuta Notsu,Ramses M. Ramirez,Sarah Rugheimer,M. Scheucher,J. E. Schlieder,Kazunari Shibata,Clara Sousa-Silva,Vlada Stamenkovic,R.J. Strangeway,Arcadi V. Usmanov,Panagiotis Vergados,Olga P. Verkhoglyadova,Aline A. Vidotto,Mary A. Voytek,Michael J. Way,Gary P. Zank,Yosuke Yamashiki +44 more
TL;DR: The current progress in the detection of terrestrial type exoplanets has opened a new avenue in the characterization of exoplanetary atmospheres and in the search for biosignatures of life with the upcoming ground-based and space missions as mentioned in this paper.