activity
20182023
most citedThe TESS Objects of Interest Catalog from the TESS Prime Mission

392 citations · 1.9k across the 21 of their papers we have counts for

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17 papers · 1 filter

astro-ph.EP2023★ 11 cited

Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases

Sara Seager, Janusz J. Petkowski, Jingcheng Huang +3

Waste gas products from technological civilizations may accumulate in an exoplanet atmosphere to detectable levels. We propose nitrogen trifluoride (NF3) and sulfur hexafluoride (S…

astro-ph.EP2022★ 22 cited

Photochemical Runaway in Exoplanet Atmospheres: Implications for Biosignatures

Sukrit Ranjan, Sara Seager, Zhuchang Zhan +5

About 2.5 billion years ago, microbes learned to harness plentiful solar energy to reduce CO with HO, extracting energy and producing O as waste. O production from…

astro-ph.EP2021★ 13 cited

Venusian phosphine: a 'Wow!' signal in chemistry?

William Bains, Janusz J. Petkowski, Sara Seager +6

The potential detection of ppb levels phosphine (PH3) in the clouds of Venus through millimeter-wavelength astronomical observations is extremely surprising as PH3 is an unexpected…

astro-ph.EP2021★ 32 cited

Assessment of Ammonia as a Biosignature Gas in Exoplanet Atmospheres

Jingcheng Huang, Sara Seager, Janusz J. Petkowski +2

Ammonia (NH3) in a terrestrial planet atmosphere is generally a good biosignature gas, primarily because terrestrial planets have no significant known abiotic NH3 source. The condi…

astro-ph.EP2021★ 35 cited

Assessment of Isoprene as a Possible Biosignature Gas in Exoplanets with Anoxic Atmospheres

Zhuchang Zhan, Sara Seager, Janusz Jurand Petkowski +4

Research for possible biosignature gases on habitable exoplanet atmosphere is accelerating. We add isoprene, C5H8, to the roster of biosignature gases. We found that formation of i…

astro-ph.EP2021★ 392 cited

The TESS Objects of Interest Catalog from the TESS Prime Mission

Natalia M. Guerrero, S. Seager, Chelsea X. Huang +102

We present 2,241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its two-year prime mission. We list these candidates in the…

astro-ph.EP2021★ 120 cited

Persistence of Flare-Driven Atmospheric Chemistry on Rocky Habitable Zone Worlds

Howard Chen, Zhuchang Zhan, Allison Youngblood +3

Low-mass stars show evidence of vigorous magnetic activity in the form of large flares and coronal mass ejections. Such space weather events may have important ramifications for th…

astro-ph.EP2020★ 268 cited

Phosphine Gas in the Cloud Decks of Venus

Jane S. Greaves, Anita M. S. Richards, William Bains +16

Measurements of trace-gases in planetary atmospheres help us explore chemical conditions different to those on Earth. Our nearest neighbor, Venus, has cloud decks that are temperat…

astro-ph.EP2020★ 68 cited

Phosphine on Venus Cannot be Explained by Conventional Processes

William Bains, Janusz J. Petkowski, Sara Seager +6

The recent candidate detection of ~1 ppb of phosphine in the middle atmosphere of Venus is so unexpected that it requires an exhaustive search for explanations of its origin. Phosp…

astro-ph.EP2020★ 123 cited

A remnant planetary core in the hot-Neptune desert

David J. Armstrong, Théo A. Lopez, Vardan Adibekyan +91

The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of plan…

astro-ph.EP2020★ 32 cited

Three Short Period Jupiters from TESS

L. D. Nielsen, R. Brahm, F. Bouchy +74

We report the confirmation and mass determination of three hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HIP 65Ab (TOI-129, TIC-201248411) is…

astro-ph.EP2019★ 125 cited

Phosphine as a Biosignature Gas in Exoplanet Atmospheres

Clara Sousa-Silva, Sara Seager, Sukrit Ranjan +4

A long-term goal of exoplanet studies is the identification and detection of biosignature gases. Beyond the most discussed biosignature gas O, only a handful of gases have been…

astro-ph.EP2019★ 64 cited

Habitability and Spectroscopic Observability of Warm M-dwarf Exoplanets Evaluated with a 3D Chemistry-Climate Model

Howard Chen, Eric T. Wolf, Zhuchang Zhan +1

Planets residing in circumstellar habitable zones (CHZs) offer our best opportunities to test hypotheses of life's potential pervasiveness and complexity. Constraining the precise…

astro-ph.EP2019★ 64 cited

An Eccentric Massive Jupiter Orbiting a Sub-Giant on a 9.5 Day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images

Joseph E. Rodriguez, Samuel N. Quinn, Chelsea X. Huang +71

We report the discovery of TOI-172 b from the Transiting Exoplanet Survey Satellite (TESS) mission, a massive hot Jupiter transiting a slightly evolved G-star with a 9.48-day orbit…

astro-ph.EP2019★ 339 cited

Stellar Flares from the First Tess Data Release: Exploring a New Sample of M-dwarfs

Maximilian N. Günther, Zhuchang Zhan, Sara Seager +21

We perform a study of stellar flares for the 24,809 stars observed with 2 minute cadence during the first two months of the TESS mission. Flares may erode exoplanets' atmospheres a…

astro-ph.EP2019★ 79 cited

TESS delivers its first Earth-sized planet and a warm sub-Neptune

Diana Dragomir, Johanna Teske, Maximilian N. Gunther +48

The future of exoplanet science is bright, as TESS once again demonstrates with the discovery of its longest-period confirmed planet to date. We hereby present HD 21749b (TOI 186.0…

astro-ph.EP2018★ 27 cited

A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17

Ian J. M. Crossfield, Natalia Guerrero, Trevor David +38

We produce light curves for all ~34,000 targets observed with K2 in Campaign 17 (C17), identifying 34 planet candidates, 184 eclipsing binaries, and 222 other periodic variables. T…