C
Chelsea X. Huang
Researcher at Massachusetts Institute of Technology
Publications - 148
Citations - 3903
Chelsea X. Huang is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 32, co-authored 126 publications receiving 2973 citations. Previous affiliations of Chelsea X. Huang include University of Southern Queensland & Princeton University.
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Journal ArticleDOI
THE AGE AND AGE SPREAD OF THE PRAESEPE AND HYADES CLUSTERS: A CONSISTENT, ∼800 Myr PICTURE FROM ROTATING STELLAR MODELS
TL;DR: The authors fit the upper main sequence of the Praesepe and Hyades open clusters using stellar models with and without rotation, and showed that rotation can remove the need for large age spreads in intermediate-age clusters, and that these clusters may be significantly older than commonly accepted.
Journal ArticleDOI
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
Warm Jupiters are less lonely than hot Jupiters: close neighbours
TL;DR: In this paper, the authors uncover a dramatic distinction in the prevalence of sub-Jovian companions, between systems that contain hot Jupiters (periods inward of 10 days) and those that host warm Jupsiters(periods between 10 and 200 days).
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Bayesian Ages for Early-type Stars from Isochrones Including Rotation, and a Possible Old Age for the Hyades
TL;DR: In this article, the authors combine a new treatment of rotation with a Bayesian statistical framework to constrain the ages and other properties of early-type stars and derive a substantially older age for the Hyades open cluster.
Journal ArticleDOI
TESS Discovery of an ultra-short-period planet around the nearby M dwarf LHS 3844
Roland Vanderspek,Chelsea X. Huang,Andrew Vanderburg,George R. Ricker,David W. Latham,Sara Seager,Joshua N. Winn,Jon M. Jenkins,Jennifer Burt,Jason A. Dittmann,Elisabeth R. Newton,Samuel N. Quinn,Avi Shporer,David Charbonneau,Jonathan Irwin,Kristo Ment,Jennifer G. Winters,Karen A. Collins,Phil Evans,Tianjun Gan,Rhodes Hart,Eric L. N. Jensen,John F. Kielkopf,Shude Mao,William Waalkes,François Bouchy,Maxime Marmier,Louise D. Nielsen,G. Ottoni,Francesco Pepe,Damien Ségransan,Stéphane Udry,Todd J. Henry,Leonardo A. Paredes,Hodari-Sadiki James,R. Hinojosa,Michele L. Silverstein,Enric Palle,Zachory K. Berta-Thompson,Misty Davies,Michael Fausnaugh,Ana Glidden,Joshua Pepper,Edward H. Morgan,Mark E. Rose,Joseph D. Twicken,J. Villasenor,Tess Team +47 more
TL;DR: In this article, a hot Earth was detected around LHS 3844, an M dwarf located 15 pc away from the Earth, which has a radius of $1.32\pm 0.02$ $R_\oplus$ and orbits the star every 11 hours.