The origin and evolution of multiple star systems
SSR Offner, M Moe, KM Kratter, SI Sadavoy… - arXiv preprint arXiv …, 2022 - arxiv.org
Observational advances over the last decade have enabled high-resolution, interferometric
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
[HTML][HTML] Binary stars in the new millennium
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 …
astrophysicists because that they allow us to determine the masses of the stars independent …
TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26
In this paper we present a catalog of 4584 eclipsing binaries observed during the first two
years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary …
years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary …
Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set
ABSTRACT The primary Kepler Mission provided nearly continuous monitoring of∼
200,000 objects with unprecedented photometric precision. We present the final catalog of …
200,000 objects with unprecedented photometric precision. We present the final catalog of …
The Transiting Exoplanet Survey Satellite: simulations of planet detections and astrophysical false positives
PW Sullivan, JN Winn… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored
Explorer mission that will perform a wide-field survey for planets that transit bright host stars …
Explorer mission that will perform a wide-field survey for planets that transit bright host stars …
Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample
A McQuillan, T Mazeh, S Aigrain - The Astrophysical Journal …, 2014 - iopscience.iop.org
We analyzed three years of data from the Kepler space mission to derive rotation periods of
main-sequence stars below 6500 K. Our automated autocorrelation-based method detected …
main-sequence stars below 6500 K. Our automated autocorrelation-based method detected …
The NASA exoplanet archive: data and tools for exoplanet research
RL Akeson, X Chen, D Ciardi, M Crane… - Publications of the …, 2013 - iopscience.iop.org
We describe the contents and functionality of the NASA Exoplanet Archive, a database and
toolset funded by NASA to support astronomers in the exoplanet community. The current …
toolset funded by NASA to support astronomers in the exoplanet community. The current …
The false positive rate of Kepler and the occurrence of planets
F Fressin, G Torres, D Charbonneau… - The Astrophysical …, 2013 - iopscience.iop.org
The Kepler mission is uniquely suited to study the frequencies of extrasolar planets. This
goal requires knowledge of the incidence of false positives such as eclipsing binaries in the …
goal requires knowledge of the incidence of false positives such as eclipsing binaries in the …
The PLATO 2.0 mission
H Rauer, C Catala, C Aerts, T Appourchaux… - Experimental …, 2014 - Springer
PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …
Target selection for the sdss-iv apogee-2 survey
G Zasowski, RE Cohen, SD Chojnowski… - The Astronomical …, 2017 - iopscience.iop.org
APOGEE-2 is a high-resolution, near-infrared spectroscopic survey observing∼ 3× 10 5
stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digital Sky …
stars across the entire sky. It is the successor to APOGEE and is part of the Sloan Digital Sky …