[HTML][HTML] The astrobiology primer v2. 0

SD Domagal-Goldman, KE Wright, K Adamala… - Astrobiology, 2016 - ncbi.nlm.nih.gov
Astrobiology is the science that seeks to understand the story of life in our universe.
Astrobiology includes investigation of the conditions that are necessary for life to emerge …

Observations of exoplanet atmospheres

IJM Crossfield - Publications of the Astronomical Society of the …, 2015 - iopscience.iop.org
Detailed characterization of an extrasolar planet's atmosphere provides the best hope for
distinguishing the makeup of its outer layers, and the only hope for understanding the …

Probabilistic forecasting of the masses and radii of other worlds

J Chen, D Kipping - The Astrophysical Journal, 2016 - iopscience.iop.org
Mass and radius are two of the most fundamental properties of an astronomical object.
Increasingly, new planet discoveries are being announced with a measurement of one of …

A revised exoplanet yield from the transiting exoplanet survey satellite (TESS)

T Barclay, J Pepper, EV Quintana - The Astrophysical Journal …, 2018 - iopscience.iop.org
Abstract The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small
planets orbiting stars bright enough for mass determination via ground-based radial velocity …

Mass–radius relation for rocky planets based on PREM

L Zeng, DD Sasselov, SB Jacobsen - The Astrophysical Journal, 2016 - iopscience.iop.org
Several small dense exoplanets are now known, inviting comparisons to Earth and Venus.
Such comparisons require translating their masses and sizes to composition models of …

Inferring probabilistic stellar rotation periods using Gaussian processes

R Angus, T Morton, S Aigrain… - Monthly Notices of …, 2018 - academic.oup.com
Variability in the light curves of spotted, rotating stars is often non-sinusoidal and quasi-
periodic–spots move on the stellar surface and have finite lifetimes, causing stellar flux …

Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities-No excess of cold Jupiters in small planet …

AS Bonomo, X Dumusque, A Massa, A Mortier… - Astronomy & …, 2023 - aanda.org
The exoplanet population characterized by relatively short orbital periods (P< 100 d) around
solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets …

A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS

TG Wilson, E Goffo, Y Alibert, D Gandolfi… - Monthly Notices of …, 2022 - academic.oup.com
We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-
dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey …

Probabilistic mass–radius relationship for sub-Neptune-sized planets

A Wolfgang, LA Rogers, EB Ford - The Astrophysical Journal, 2016 - iopscience.iop.org
ABSTRACT The Kepler Mission has discovered thousands of planets with radii< 4${R} _
{\oplus} $, paving the way for the first statistical studies of the dynamics, formation, and …

275 candidates and 149 validated planets orbiting bright stars in K2 campaigns 0–10

AW Mayo, A Vanderburg, DW Latham… - The Astronomical …, 2018 - iopscience.iop.org
Abstract Since 2014, NASA's K2 mission has observed large portions of the ecliptic plane in
search of transiting planets and has detected hundreds of planet candidates. With …