Statistical methods for exoplanet detection with radial velocities

NC Hara, EB Ford - Annual Review of Statistics and Its …, 2023 - annualreviews.org
Exoplanets can be detected with various observational techniques. Among them, radial
velocity (RV) has the key advantages of revealing the architecture of planetary systems and …

The California Legacy Survey. I. A catalog of 178 planets from precision radial velocity monitoring of 719 nearby stars over three decades

LJ Rosenthal, BJ Fulton, LA Hirsch… - The Astrophysical …, 2021 - iopscience.iop.org
We present a high-precision radial velocity (RV) survey of 719 FGKM stars, which host 164
known exoplanets and 14 newly discovered or revised exoplanets and substellar …

Spectrum radial velocity analyser (SERVAL)-High-precision radial velocities and two alternative spectral indicators

M Zechmeister, A Reiners, PJ Amado, M Azzaro… - Astronomy & …, 2018 - aanda.org
Context. The CARMENES survey is a high-precision radial velocity (RV) programme that
aims to detect Earth-like planets orbiting low-mass stars. Aims. We develop least-squares …

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 …

Hot exoplanetary atmospheres in 3D

W Pluriel - Remote Sensing, 2023 - mdpi.com
Hot giant exoplanets are very exotic objects with no equivalent in the Solar System that
allow us to study the behavior of atmospheres under extreme conditions. Their thermal and …

A spectral survey of an ultra-hot Jupiter-Detection of metals in the transmission spectrum of KELT-9 b

HJ Hoeijmakers, D Ehrenreich, D Kitzmann… - Astronomy & …, 2019 - aanda.org
Context. KELT-9 b exemplifies a newly emerging class of short-period gaseous exoplanets
that tend to orbit hot, early type stars–termed ultra-hot Jupiters. The severe stellar irradiation …

[HTML][HTML] The HARPS search for southern extra-solar planets-XXXI. The M-dwarf sample

X Bonfils, X Delfosse, S Udry, T Forveille… - Astronomy & …, 2013 - aanda.org
Context. Searching for planets around stars with different masses helps us to assess the
outcome of planetary formation for different initial conditions. The low-mass M dwarfs are …

Three years of HARPS-N high-resolution spectroscopy and precise radial velocity data for the Sun

X Dumusque, M Cretignier, D Sosnowska… - Astronomy & …, 2021 - aanda.org
Context. The solar telescope connected to HARPS-N has been observing the Sun since the
summer of 2015. Such a high-cadence, long-baseline data set is crucial for understanding …

TESS Hunt for Young and Maturing Exoplanets (THYME): a planet in the 45 Myr Tucana–Horologium association

ER Newton, AW Mann, BM Tofflemire… - The Astrophysical …, 2019 - iopscience.iop.org
Young exoplanets are snapshots of the planetary evolution process. Planets that orbit stars
in young associations are particularly important because the age of the planetary system is …

SOAP 2.0: a tool to estimate the photometric and radial velocity variations induced by stellar spots and plages

X Dumusque, I Boisse, NC Santos - The Astrophysical Journal, 2014 - iopscience.iop.org
ABSTRACT This paper presents SOAP 2.0, a new version of the Spot Oscillation And Planet
(SOAP) code that estimates in a simple way the photometric and radial velocity (RV) …