Sara Seager

Prof. Sara Seager

Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
orcid

Research Focus & Metrics

Academic Career Length

25Years (2002-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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24 October 2014 in Journal of Astronomical Telescopes, Instruments, and Systems
Verified
Journal Article
Open access
PDF file
GRGeorge R. Ricker
George R. Ricker
JWJoshua N. Winn
Joshua N. Winn
RVRoland Vanderspek
Roland Vanderspek
DLDavid W. Latham
David W. Latham
GBGáspár Á. Bakos
Gáspár Á. Bakos
JVJoel Villasenor
Joel Villasenor
The study of exoplanets—planets outside our solar system—is one of the most exciting and rapidly advancing fields of science. Especially valuable are systems in which a planet’s orbit carries it directly across the face of its host star. For such a “transiting” planet, it is possible to determine the planet’s mass and radius, its orbital parameters, and its atmospheric properties.1

9 September 2019 in The Astronomical Journal
Verified
Journal Article
Closed access
KSKeivan G. Stassun
Keivan G. Stassun
RORyan J. Oelkers
Ryan J. Oelkers
MPMartin Paegert
Martin Paegert
GTGuillermo Torres
Guillermo Torres
JPJoshua Pepper
Joshua Pepper
JWJoshua N. Winn
Joshua N. Winn
We describe the catalogs assembled and the algorithms used to populate the revised TESS Input Catalog (TIC), based on the incorporation of the Gaia second data release. We also describe a revised ranking system for prioritizing stars for 2 minute cadence observations, and we assemble a revised Candidate Target List (CTL) using that ranking. The TIC is available on the Mikulski Archive for Space Telescopes server, and an enhanced CTL is available through the Filtergraph data visualization portal system at http://filtergraph.vanderbilt.edu/tess_ctl.

1 June 2021 in The Astrophysical Journal Supplement Series
Verified
Journal Article
Closed access
NGNatalia M. Guerrero
Natalia M. Guerrero
Sara SeagerSara Seager
Sara Seager
CHChelsea X. Huang
Chelsea X. Huang
AVAndrew Vanderburg
Andrew Vanderburg
ASAylin Garcia Soto
Aylin Garcia Soto
JWJoshua N. Winn
Joshua N. Winn
We present 2241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its 2 yr Prime Mission. We list these candidates in the TESS Objects of Interest (TOI) Catalog, which includes both new planet candidates found by TESS and previously known planets recovered by TESS observations. We describe the process used to identify TOIs, investigate the characteristics of the new planet candidates, and discuss some notable TESS planet discoveries. The TOI catalog includes an unprecedented number of small planet candidates around nearby bright stars, which are well suited for detailed follow-up observations. The TESS data products for the Prime Mission (sectors 1–26), including the TOI catalog, light curves, full-frame images, and target pixel files, are publicly available at the Mikulski Archive for Space Telescopes.

23 March 2005 in Nature
Verified
Journal Article
Closed access
LDL. Drake Deming
L. Drake Deming
Sara SeagerSara Seager
Sara Seager
LRL. Jeremy Richardson
L. Jeremy Richardson
JHJoseph Harrington
Joseph Harrington

14 September 2020 in Nature Astronomy
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Journal Article
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JGJane S. Greaves
Jane S. Greaves
ARAnita M. S. Richards
Anita M. S. Richards
WBWilliam Bains
William Bains
Paul RimmerPaul Rimmer
Paul Rimmer
HSHideo Sagawa
Hideo Sagawa
JHJim Hoge
Jim Hoge

3 May 2013 in Science
Verified
Journal Article
Closed access
PDF file
Sara SeagerSara Seager
Sara Seager
The search for exoplanets includes the promise to eventually find and identify habitable worlds. The thousands of known exoplanets and planet candidates are extremely diverse in terms of their masses or sizes, orbits, and host star type. The diversity extends to new kinds of planets, which are very common yet have no solar system counterparts. Even with the requirement that a planet’s surface temperature must be compatible with liquid water (because all life on Earth requires liquid water), a new emerging view is that planets very different from Earth may have the right conditions for life. The broadened possibilities will increase the future chances of discovering an inhabited world.