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相关论文: Kepler Eclipsing Binary Stars. VI. Identification …

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We have developed a procedure for the classification of eclipsing binaries from their light-curve parameters and spectral type. The procedure was tested on more than 1000 systems with known classification, and its efficiency was estimated…

太阳与恒星天体物理 · 物理学 2014-09-09 Ekaterina Avvakumova , Oleg Malkov

The Robo-AO \textit{Kepler} Planetary Candidate Survey is observing every \textit{Kepler} planet candidate host star with laser adaptive optics imaging to search for blended nearby stars, which may be physically associated companions and/or…

地球与行星天体物理 · 物理学 2017-01-18 Carl Ziegler , Nicholas M. Law , Tim Morton , Christoph Baranec , Reed Riddle , Dani Atkinson , Anna Baker , Sarah Roberts , David R. Ciardi

Eclipsing binaries are crucial astrophysical laboratories for studying stellar parameters and evolutionary processes. In this study, we constructed a machine-learning-based model for systematic phenomenological classification of eclipsing…

太阳与恒星天体物理 · 物理学 2026-04-30 Shi-Qi Liu , Kai Li , Xiao-Dian Chen , Li-Heng Wang

We present the first results of a Kepler survey of 41 eclipsing binaries that we undertook to search for third star companions. Such tertiaries will periodically alter the eclipse timings through light travel time and dynamical effects. We…

太阳与恒星天体物理 · 物理学 2015-06-04 D. R. Gies , S. J. Williams , R. A. Matson , Z. Guo , S. M. Thomas , J. A. Orosz , G. J. Peters

We report the discovery of 42 white dwarfs in the original Kepler mission field, including nine new confirmed pulsating hydrogen-atmosphere white dwarfs (ZZ Ceti stars). Guided by the Kepler-INT Survey (KIS), we selected white dwarf…

The realistic simulation of variable star populations is fundamental to determine the selection function and contamination in existing and upcoming multi-epoch surveys. We present \ellisa, a simulator that produces an ensemble of mock light…

Gaia provided the largest-ever catalogue of white dwarf stars. We use this catalogue, along with the third public data release of the Zwicky Transient Facility (ZTF), to identify new eclipsing white dwarf binaries. Our method exploits light…

太阳与恒星天体物理 · 物理学 2021-11-18 Pascal M. Keller , Elmé Breedt , Simon Hodgkin , Vasily Belokurov , James Wild , Ignacio García-Soriano , Jacob L. Wise

NASA's Kepler Space Telescope has collected high-precision, high-cadence time series photometry on 781,590 unique postage-stamp targets across 21 different fields of view. These observations have already yielded 2,496 scientific…

Next-generation synoptic photometric surveys will yield unprecedented (for the astronomical community) volumes of data and the processes of discovery and rare-object identification are, by necessity, becoming more autonomous. Such…

太阳与恒星天体物理 · 物理学 2014-04-08 Isaac Shivvers , Joshua S. Bloom , Joseph W. Richards

We present a statistical analysis that demonstrates that the overwhelming majority of Kepler candidate multiple transiting systems (multis) indeed represent true, physically-associated transiting planets. Binary stars provide the primary…

The NASA {\it Kepler} mission has been in science operation since May 2009 and is providing high precision, high cadence light curves of over 150,000 targets. Prior to launch, nine cataclysmic variables were known to lie within {\it…

太阳与恒星天体物理 · 物理学 2015-06-15 Steve B. Howell , Mark E. Everett , Sally A. Seebode , Paula Szkody , Martin Still , Matt Wood , Gavin Ramsay , John Cannizzo , Alan Smale

Inspired by the discovery of the red nova V1309 Sco (Nova Scorpii 2008) and the fact that its progenitor was a binary system with a rapidly decreasing orbital period, we have searched for period changes in OGLE binary stars. We have…

太阳与恒星天体物理 · 物理学 2018-10-24 P. Pietrukowicz , I. Soszynski , A. Udalski , M. K. Szymanski , L. Wyrzykowski , R. Poleski , S. Kozlowski , J. Skowron , P. Mroz , M. Pawlak , K. Ulaczyk

The Kepler mission and subsequent ground-based follow-up observations have revealed a number of exoplanet host stars with nearby stellar companions. This study presents speckle observations of 57 Kepler objects of interest (KOIs) that are…

The Kepler Mission was launched on March 6, 2009 to perform a photometric survey of more than 100,000 dwarf stars to search for Earth-size planets with the transit technique. The reliability of the resulting planetary candidate list relies…

The dynamical influence of binary companions is expected to profoundly influence planetary systems. However, the difficulty of identifying planets in binary systems has left the magnitude of this effect uncertain; despite numerous…

地球与行星天体物理 · 物理学 2016-06-29 Adam L. Kraus , Michael J. Ireland , Daniel Huber , Andrew W. Mann , Trent J. Dupuy

Four candidates of eclipsing multiples, based on new extraneous eclipses found on Kepler binary light curves, are presented and studied. KIC 7622486 is a double eclipsing binary candidate with orbital period of 2.2799960 days and 40.246503…

太阳与恒星天体物理 · 物理学 2017-03-03 Jia Zhang , Sheng-Bang Qian , Jian-Duo He

The combined strength of asteroseismology and empirical stellar basic parameter determinations for in-depth asteroseismic analysis of massive pulsators in eclipsing binaries shows great potential for treating the challenging and mysterious…

太阳与恒星天体物理 · 物理学 2024-03-20 Christian I. Eze , Gerald Handler

Given that Campaign 16 of the K2 mission is one of just two K2 campaigns observed so far in "forward-facing" mode, which enables immediate follow-up observations from the ground, we present a catalog of interesting targets identified…

Ranked near the top of the long list of exciting discoveries made with NASA's Kepler photometer is the detection of transiting circumbinary planets. In just over a year the number of such planets went from zero to seven, including a…

地球与行星天体物理 · 物理学 2015-06-17 William F. Welsh , Jerome A. Orosz , Joshua A. Carter , Daniel C. Fabrycky

Eclipsing binaries (EBs) play an important astrophysical role in studying stellar properties and evolution. By analyzing photometric data in the LAMOST Medium-Resolution Survey field, RA: $23^h$$01^m$$51.00^s$, Dec:…

太阳与恒星天体物理 · 物理学 2024-12-03 Jing-Yi Wang , Kai Li , Xiang Gao , Di-Fu Guo , Li-Heng Wang , Dong-Yang Gao , Ling-Zhi Li , Ya-Ni Guo , Xing Gao , Guo-You Sun