97 datasets found

Keywords: Subdwarf stars

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  • 3-D selection of 167 sub-stellar companions

    We analyze 5108 AFGKM stars with at least five high-precision radial velocity points, as well as Gaia and Hipparcos astrometric data, utilizing a novel pipeline developed in...
  • Hot subdwarf candidates from LAMOST DR7

    Hot subdwarf stars are a particular type of star that is crucial for studying binary evolution and atmospheric diffusion processes. In recent years, identifying hot subdwarfs by...
  • Grid of synthetic spectra for subdwarfs

    A new grid of detailed atmosphere model spectra for hot and moderately cool subdwarf stars is presented. High-resolution spectra and synthetic photometry are calculated in the...
  • Hot subdwarf stars with Gaia DR2 and LAMOST DR7 data

    Based on the Gaia DR2 catalog of hot subdwarf star candidates, we identified 1587 hot subdwarf stars with spectra in LAMOST DR7. We present atmospheric parameters for these...
  • NIR proper motion survey using 2MASS

    We have conducted a 4030deg^2^ near-infrared proper motion survey using multi-epoch data from the Two Micron All-Sky Survey (2MASS). We find 2778 proper motion candidates, 647...
  • SDSS4 confirmed white dwarfs catalog

    We present a catalog of 9316 spectroscopically confirmed white dwarfs from the Sloan Digital Sky Survey Data Release 4. We have selected the stars through photometric cuts and...
  • Variable hot subdwarf from Gaia DR2 and TESS

    Hot subdwarf stars are mostly stripped red giants that can exhibit photometric variations due to stellar pulsations, eclipses, the reflection effect, ellipsoidal modulation, and...
  • Chemical properties of the local disk & halo. II.

    We present a model-fit pipeline to determine the stellar parameters of M-type dwarfs, which is an improvement on our previous work described in Hejazi+ (Paper I; J/AJ/159/30)....
  • Hot subdwarf stars from Gaia with LAMOST sp. II. RVs

    Combining LAMOST radial velocities with Gaia parallaxes and proper motions, we present 3D Galactic space motions and the orbits of 182 single-lined hot subdwarf stars. These...
  • Hot subdwarf stars from Gaia DR2 & LAMOST DR6+7. I.

    182 single-lined hot subdwarf stars are identified by using spectra from the sixth and seventh data releases (DR6 and DR7) of the Large Sky Area Multi-Object Fibre Spectroscopic...
  • Hot subdwarf stars from LAMOST DR5 & Gaia DR2

    Combing Gaia DR2 with LAMOST DR5, we spectroscopically identified 924 hot subdwarf stars, among which 32 stars exhibit strong double-lined composite spectra. We measured the...
  • Hot subdwarf stars from Gaia DR2 and LAMOST DR5. II.

    Three hundred and eighty eight hot subdwarf stars have been identified by using the Hertzsprung-Russell (HR) diagram built from the second data release of the Gaia mission. By...
  • Hot subdwarf stars from Gaia DR2 and LAMOST DR5

    We selected 4593 hot subdwarf candidates from the Gaia DR2 Hertzsprung-Russell (HR) diagram. By combining the sample with Large Sky Area Multi-Object Fibre Spectroscopic...
  • Rapidly pulsating sdB stars search with GALEX

    NASA's Galaxy Evolution Explorer (GALEX) provided near- and far-UV observations for approximately 77% of the sky over a 10-year period; however, the data reduction pipeline...
  • Hot subdwarf stars in LAMOST DR1

    We present a catalog of 166 spectroscopically identified hot subdwarf stars from LAMOST DR1, 44 of which show the characteristics of cool companions in their optical spectra....
  • Periodicities in KIC 3527751 from 3yr Kepler data

    We analyze 3yr of nearly continuous Kepler spacecraft short cadence observations of the pulsating subdwarf B (sdB) star KIC 3527751. We detect a total of 251 periodicities, most...
  • Robo-AO observed cool subdwarf companions

    Cool subdwarfs are the oldest members of the low-mass stellar population. Mostly present in the galactic halo, subdwarfs are characterized by their low-metallicity. Measuring...
  • Candidate halo wide binaries

    We present an improved catalog of halo wide binaries compiled from an extensive literature search. Most of our binaries stem from the common proper motion binary catalogs by...
  • FUSE spectra analysis of hot subdwarf stars

    When the neutral interstellar medium is exposed to extreme-ultraviolet and soft X-ray radiation, the argon atoms in it are far more susceptible to being ionized than the...
  • Discovery of hot subdwarf companion to FY CMa

    The rapid rotation of Be stars may be caused in some cases by past mass and angular momentum accretion in an interacting binary in which the mass donor is currently viewed as a...
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