The GAPS programme with HARPS-N at TNG-XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting …

AS Bonomo, S Desidera, S Benatti, F Borsa… - Astronomy & …, 2017 - aanda.org
We carried out a Bayesian homogeneous determination of the orbital parameters of 231
transiting giant planets (TGPs) that are alone or have distant companions; we employed …

TESS transit timing of hundreds of hot Jupiters

ES Ivshina, JN Winn - The Astrophysical Journal Supplement …, 2022 - iopscience.iop.org
We provide a database of transit times and updated ephemerides for 382 planets based on
data from the NASA Transiting Exoplanet Survey Satellite (TESS) and previously reported …

TESS Hunt for Young and Maturing Exoplanets (THYME). IV. Three Small Planets Orbiting a 120 Myr Old Star in the Pisces–Eridanus Stream

ER Newton, AW Mann, AL Kraus… - The Astronomical …, 2021 - iopscience.iop.org
Young exoplanets can offer insight into the evolution of planetary atmospheres,
compositions, and architectures. We present the discovery of the young planetary system …

ExoClock Project. II. A large-scale integrated study with 180 updated exoplanet ephemerides

A Kokori, A Tsiaras, B Edwards… - The Astrophysical …, 2022 - iopscience.iop.org
The ExoClock project is an inclusive, integrated, and interactive platform that was developed
to monitor the ephemerides of the Ariel targets to increase the mission efficiency. The project …

Statistical characterization of hot Jupiter atmospheres using Spitzer's secondary eclipses

E Garhart, D Deming, A Mandell… - The Astronomical …, 2020 - iopscience.iop.org
We report 78 secondary eclipse depths for a sample of 36 transiting hot Jupiters observed at
3.6 and 4.5 μm using the Spitzer Space Telescope. Our eclipse results for 27 of these …

On correlated-noise analyses applied to exoplanet light curves

P Cubillos, J Harrington, TJ Loredo… - The Astronomical …, 2016 - iopscience.iop.org
Time-correlated noise is a significant source of uncertainty when modeling exoplanet light-
curve data. A correct assessment of correlated noise is fundamental to determine the true …

An emission spectrum for WASP-121b measured across the 0.8–1.1 μm wavelength range using the Hubble Space Telescope

T Mikal-Evans, DK Sing, JM Goyal… - Monthly Notices of …, 2019 - academic.oup.com
WASP-121b is a transiting gas giant exoplanet orbiting close to its Roche limit, with an
inflated radius nearly double that of Jupiter and a dayside temperature comparable to a late …

Mass loss from the exoplanet WASP-12b inferred from Spitzer phase curves

TJ Bell, M Zhang, PE Cubillos, L Dang… - Monthly Notices of …, 2019 - academic.oup.com
The exoplanet WASP-12b is the prototype for the emerging class of ultrahot, Jupiter-mass
exoplanets. Past models have predicted–and near-ultraviolet observations have shown–that …

An Open-source Bayesian Atmospheric Radiative Transfer (BART) Code. I. Design, Tests, and Application to Exoplanet HD 189733b

J Harrington, MD Himes, PE Cubillos… - The Planetary …, 2022 - iopscience.iop.org
We present the open-source Bayesian Atmospheric Radiative Transfer (BART) retrieval
package, which produces estimates and uncertainties for an atmosphere's thermal profile …

An open-source Bayesian atmospheric radiative transfer (BART) code. II. The transit radiative transfer module and retrieval of HAT-P-11b

PE Cubillos, J Harrington, J Blecic… - The Planetary …, 2022 - iopscience.iop.org
This and companion papers by Harrington et al. and Blecic et al. present the Bayesian
Atmospheric Radiative Transfer (bart) code, an open-source, open-development package to …