[HTML][HTML] Gaia Data Release 3-All-sky classification of 12.4 million variable sources into 25 classes

L Rimoldini, B Holl, P Gavras, M Audard… - Astronomy & …, 2023 - aanda.org
Context. Gaia DR3 contains 1.8 billion sources with G-band photometry, 1.5 billion of which
with G BP and G RP photometry, complemented by positions on the sky, parallax, and …

Highlights of Discoveries for δ Scuti Variable Stars From the Kepler Era

JA Guzik - Frontiers in Astronomy and Space Sciences, 2021 - frontiersin.org
The NASA Kepler and follow-on K2 mission (2009–2018) left a legacy of data and
discoveries, finding thousands of exoplanets, and also obtaining high-precision long time …

SOPHIE velocimetry of Kepler transit candidates-XVII. The physical properties of giant exoplanets within 400 days of period

A Santerne, C Moutou, M Tsantaki, F Bouchy… - Astronomy & …, 2016 - aanda.org
While giant extrasolar planets have been studied for more than two decades now, there are
still some open questions as to their dominant formation and migration processes, as well as …

A unifying explanation of complex frequency spectra of γ Dor, SPB and Be stars: combination frequencies and highly non-sinusoidal light curves

DW Kurtz, H Shibahashi, SJ Murphy… - Monthly Notices of …, 2015 - academic.oup.com
Abstract There are many Slowly Pulsating B (SPB) stars and γ Dor stars in the Kepler
mission data set. The light curves of these pulsating stars have been classified …

Turbulent convection and pulsation stability of stars – II. Theoretical instability strip for δ Scuti and γ Doradus stars

DR Xiong, L Deng, C Zhang… - Monthly Notices of the …, 2016 - academic.oup.com
By using a non-local and time-dependent convection theory, we have calculated radial and
low-degree non-radial oscillations for stellar evolutionary models with M= 1.4–3.0 M⊙. The …

K2 variable catalogue–II. Machine learning classification of variable stars and eclipsing binaries in K2 fields 0–4

DJ Armstrong, J Kirk, KWF Lam… - Monthly Notices of …, 2015 - academic.oup.com
We are entering an era of unprecedented quantities of data from current and planned survey
telescopes. To maximize the potential of such surveys, automated data analysis techniques …

TESS stellar rotation up to 80 days in the southern continuous viewing zone

ZR Claytor, JL van Saders, L Cao… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The Transiting Exoplanet Survey Satellite (TESS) mission delivers time-series
photometry for millions of stars across the sky, offering a probe into stellar astrophysics …

Periodic variable AF spectral type stars in the northern TESS continuous viewing zone-I. Identification and classification

M Skarka, J Žák, M Fedurco, E Paunzen… - Astronomy & …, 2022 - aanda.org
Context. In the time of large space surveys that provide tremendous amounts of precise data,
it is highly desirable to have a commonly accepted methodology and system for the …

Catalogue and properties of δ Scuti stars in binaries

A Liakos, P Niarchos - Monthly Notices of the Royal …, 2016 - academic.oup.com
The catalogue contains 199 confirmed cases of binary systems containing at least one
pulsating component of δ Sct type. The sample is divided into subgroups in order to describe …

The astrophysics of visible-light orbital phase curves in the space age

A Shporer - Publications of the Astronomical Society of the Pacific, 2017 - iopscience.iop.org
The field of visible-light continuous time series photometry is now at its golden age,
manifested by the continuum of past (CoRoT, Kepler), present (K2), and future (TESS …