Accurate masses and radii of normal stars: modern results and applications

G Torres, J Andersen, A Giménez - The Astronomy and Astrophysics …, 2010 - Springer
This article presents and discusses a critical compilation of accurate, fundamental
determinations of stellar masses and radii. We have identified 95 detached binary systems …

[HTML][HTML] Binary stars in the new millennium

X Chen, Z Liu, Z Han - Progress in Particle and Nuclear Physics, 2024 - Elsevier
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …

batman: basic transit model calculation in Python

L Kreidberg - Publications of the Astronomical Society of the …, 2015 - iopscience.iop.org
I introduce batman, a Python package for modeling exoplanet transit and eclipse light
curves. The batman package supports calculation of light curves for any radially symmetric …

exoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series

D Foreman-Mackey, R Luger, E Agol, T Barclay… - arxiv preprint arxiv …, 2021 - arxiv.org
" exoplanet" is a toolkit for probabilistic modeling of astronomical time series data, with a
focus on observations of exoplanets, using PyMC3 (Salvatier et al., 2016). PyMC3 is a …

A Distance determination to the Small Magellanic Cloud with an accuracy of better than two percent based on late-type eclipsing binary stars

D Graczyk, G Pietrzyński, IB Thompson… - The Astrophysical …, 2020 - iopscience.iop.org
We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud
(SMC) undertaken with the aim of improving the distance determination to this important …

Physics of eclipsing binaries. V. General framework for solving the inverse problem

KE Conroy, A Kochoska, D Hey, H Pablo… - The Astrophysical …, 2020 - iopscience.iop.org
PHOEBE 2 is a Python package for modeling the observables of eclipsing star systems, but
until now it has focused entirely on the forward model—that is, generating a synthetic model …

Homogeneous studies of transiting extrasolar planets–IV. Thirty systems with space-based light curves

J Southworth - Monthly Notices of the Royal Astronomical …, 2011 - academic.oup.com
I calculate the physical properties of 32 transiting extrasolar planet and brown-dwarf systems
from existing photometric observations and measured spectroscopic parameters. The …

Detailed models of interacting short-period massive binary stars

K Sen, N Langer, P Marchant, A Menon… - Astronomy & …, 2022 - aanda.org
Context. The majority of massive stars are part of binary systems. In about a quarter of these,
the companions are so close that mass transfer occurs while they undergo core hydrogen …

The mass discrepancy in intermediate-and high-mass eclipsing binaries: The need for higher convective core masses

A Tkachenko, K Pavlovski, C Johnston… - Astronomy & …, 2020 - aanda.org
Context. Eclipsing, spectroscopic double-lined binary star systems are excellent laboratories
for calibrating theories of stellar interior structure and evolution. Their precise and accurate …

Homogeneous studies of transiting extrasolar planets–I. Light-curve analyses

J Southworth - Monthly Notices of the Royal Astronomical …, 2008 - academic.oup.com
I present a homogeneous analysis of the transit light curves of 14 well-observed transiting
extrasolar planets. The light curves are modelled using jktebop, random errors are …