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The Transiting Exoplanet Survey Satellite (TESS) will be conducting a nearly all-sky photometric survey over two years, with a core mission goal to discover small transiting exoplanets orbiting nearby bright stars. It will obtain 30-minute…

Transiting exoplanets in multi-planet systems exhibit non-Keplerian orbits as a result of the gravitational influence from companions which can cause the times and durations of transits to vary. The amplitude and periodicity of the transit…

Earth and Planetary Astrophysics · Physics 2019-12-24 Kyle A. Pearson

In the last decade, over a million stars were monitored to detect transiting planets. Manual interpretation of potential exoplanet candidates is labor intensive and subject to human error, the results of which are difficult to quantify.…

Instrumentation and Methods for Astrophysics · Physics 2017-12-20 Kyle A. Pearson , Leon Palafox , Caitlin A. Griffith

The Transiting Exoplanet Survey Satellite (TESS) will perform a two-year survey of nearly the entire sky, with the main goal of detecting exoplanets smaller than Neptune around bright and nearby stars. There do not appear to be any…

Earth and Planetary Astrophysics · Physics 2017-05-26 L. G. Bouma , Joshua N. Winn , Jacobi Kosiarek , P. R. McCullough

Continuous data releases throughout the TESS primary mission will provide unique opportunities for the exoplanet community at large to contribute to maximizing TESS's scientific return via the discovery and validation of transiting planets.…

Earth and Planetary Astrophysics · Physics 2019-07-31 Ryan Cloutier

The kepler and TESS missions have generated over 100,000 potential transit signals that must be processed in order to create a catalog of planet candidates. During the last few years, there has been a growing interest in using machine…

Space-based transit missions such as Kepler and TESS have demonstrated that planets are ubiquitous. However, the success of these missions heavily depends on ground-based radial velocity (RV) surveys, which combined with transit photometry…

The Transiting Exoplanet Survey Satellite (TESS) will embark in 2018 on a 2-year wide-field survey mission, discovering over a thousand terrestrial, super-Earth and sub-Neptune-sized exoplanets potentially suitable for follow-up…

Earth and Planetary Astrophysics · Physics 2018-02-28 Dana R. Louie , Drake Deming , Loic Albert , L. G. Bouma , Jacob Bean , Mercedes Lopez-Morales

Space-based missions such as TESS are identifying a wealth of short-period ($\lesssim30$ d) transiting planets. Despite the growing number of confirmed and candidate planets, the sample is still incomplete and highly biased, challenging…

Earth and Planetary Astrophysics · Physics 2026-04-27 M. Lafarga , D. J. Armstrong , K. Cui , A. Hadjigeorghiou , V. Kunovac , L. Doyle , E. M. Bryant , R. F. Díaz , L. A. Nieto , A. Osborn

We present a prediction of the transiting exoplanet yield of the TESS primary mission, in order to guide follow-up observations and science projects utilizing TESS discoveries. Our new simulations differ from previous work by using (1) an…

The Transiting Exoplanet Survey Satellite (TESS) is currently concluding its 2-year primary science mission searching 85% of the sky for transiting exoplanets. TESS has already discovered well over one thousand TESS objects of interest…

Earth and Planetary Astrophysics · Physics 2020-10-07 Dana R. Louie , Norio Narita , Akihiko Fukui , Enric Palle , Motohide Tamura , Nobuhiko Kusakabe , Hannu Parviainen , Drake Deming

The upcoming TESS mission is expected to find thousands of transiting planets around bright stars, yet for three-quarters of the fields observed the temporal coverage will limit discoveries to planets with orbital periods below 13.7 days.…

Instrumentation and Methods for Astrophysics · Physics 2017-01-25 David M. Kipping , Christopher Lam

The Transiting Exoplanet Survey Satellite (TESS) is focusing on relatively bright stars and has found thousands of planet candidates. However, mainly because of the low spatial resolution of its cameras ($\approx$ 21 arcsec/pixel), TESS is…

JWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5,000 confirmed planets, more than 4,000 TESS planet candidates are still unconfirmed and many of the best planets for…

Earth and Planetary Astrophysics · Physics 2023-08-21 Benjamin J. Hord , Eliza M. -R. Kempton , Thomas Mikal-Evans , David W. Latham , David R. Ciardi , Diana Dragomir , Knicole D. Colón , Gabrielle Ross , Andrew Vanderburg , Zoe L. de Beurs , Karen A. Collins , Cristilyn N. Watkins , Jacob Bean , Nicolas B. Cowan , Tansu Daylan , Caroline V. Morley , Jegug Ih , David Baker , Khalid Barkaoui , Natalie M. Batalha , Aida Behmard , Alexander Belinski , Zouhair Benkhaldoun , Paul Benni , Krzysztof Bernacki , Allyson Bieryla , Avraham Binnenfeld , Pau Bosch-Cabot , François Bouchy , Valerio Bozza , Rafael Brahm , Lars A. Buchhave , Michael Calkins , Ashley Chontos , Catherine A. Clark , Ryan Cloutier , Marion Cointepas , Kevin I. Collins , Dennis M. Conti , Ian J. M. Crossfield , Fei Dai , Jerome P. de Leon , Georgina Dransfield , Courtney Dressing , Adam Dustor , Gilbert Esquerdo , Phil Evans , Sergio B. Fajardo-Acosta , Jerzy Fiołka , Raquel Forés-Toribio , Antonio Frasca , Akihiko Fukui , Benjamin Fulton , Elise Furlan , Tianjun Gan , Davide Gandolfi , Mourad Ghachoui , Steven Giacalone , Emily A. Gilbert , Michaël Gillon , Eric Girardin , Erica Gonzales , Ferran Grau Horta , Joao Gregorio , Michael Greklek-McKeon , Pere Guerra , J. D. Hartman , Coel Hellier , Krzysztof G. Hełminiak , Thomas Henning , Michelle L. Hill , Keith Horne , Andrew W. Howard , Steve B. Howell , Daniel Huber , Howard Isaacson , Giovanni Isopi , Emmanuel Jehin , Jon M. Jenkins , Eric L. N. Jensen , Marshall C. Johnson , Andrés Jordán , Stephen R. Kane , John F. Kielkopf , Vadim Krushinsky , Sławomir Lasota , Elena Lee , Pablo Lewin , John H. Livingston , Jack Lubin , Michael B. Lund , Franco Mallia , Christopher R. Mann , Giuseppe Marino , Nataliia Maslennikova , Bob Massey , Rachel Matson , Elisabeth Matthews , Andrew W. Mayo , Tsevi Mazeh , Kim K. McLeod , Edward J. Michaels , Teo Močnik , Mayuko Mori , Georgia Mraz , Jose A. Muñoz , Norio Narita , Louise Dyregaard Nielsen , Hugh Osborn , Enric Palle , Aviad Panahi , Riccardo Papini , Alex S. Polanski , Adam Popowicz , Francisco J. Pozuelos , Samuel N. Quinn , Don J. Radford , Phillip A. Reed , Howard M. Relles , Malena Rice , Paul Robertson , Joseph E. Rodriguez , Lee J. Rosenthal , Ryan A. Rubenzahl , Nicole Schanche , Joshua Schlieder , Richard P. Schwarz , Ramotholo Sefako , Avi Shporer , Alessandro Sozzetti , Gregor Srdoc , Chris Stockdale , Alexander Tarasenkov , Thiam-Guan Tan , Mathilde Timmermans , Eric B. Ting , Judah Van Zandt , JP Vignes , Ian Waite , Noriharu Watanabe , Lauren M. Weiss , Justin Wittrock , George Zhou , Carl Ziegler , Shay Zucker

In the search for life in the cosmos, NASA's Transiting Exoplanet Survey Satellite (TESS) mission has already monitored about 74% of the sky for transiting extrasolar planets, including potentially habitable worlds. However, TESS only…

Earth and Planetary Astrophysics · Physics 2021-05-05 L. Kaltenegger , J. Pepper , P. M. Christodoulou , K. Stassun , S. Quinn , C. Burke

The Transiting Exoplanet Survey Satellite (TESS) has identified several thousand planet candidates orbiting a wide variety of stars, and has provided an exciting opportunity for demographic studies. However, current TESS planet searches…

The upcoming TESS mission will detect thousands of candidate transiting exoplanets. Those candidates require extensive follow-up observations to distinguish genuine planets from false positives, and to resolve the physical properties of the…

Earth and Planetary Astrophysics · Physics 2018-10-23 David R. Ciardi , Joshua Pepper , Knicole Colon , Stephen R. Kane , With Input from the Astrophysical Community