首页    期刊浏览 2024年11月28日 星期四
登录注册

文章基本信息

  • 标题:Gaia Data Release 2
  • 其他标题:First stellar parameters from Apsis
  • 本地全文:下载
  • 作者:René Andrae ; Morgan Fouesneau ; Orlagh Creevey
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2018
  • 卷号:616
  • DOI:10.1051/0004-6361/201732516
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:The secondGaiadata release (GaiaDR2) contains, beyond the astrometry, three-band photometry for 1.38 billion sources. One band is theGband, the other two were obtained by integrating theGaiaprism spectra (BP and RP). We have used these three broad photometric bands to infer stellar effective temperatures,Teff, for all sources brighter thanG= 17 mag withTeffin the range 3000–10 000 K (some 161 million sources). Using in addition the parallaxes, we infer the line-of-sight extinction,AG, and the reddening,E(BP − RP), for 88 million sources. Together with a bolometric correction we derive luminosity and radius for 77 million sources. These quantities as well as their estimated uncertainties are part ofGaiaDR2. Here we describe the procedures by which these quantities were obtained, including the underlying assumptions, comparison with literature estimates, and the limitations of our results. Typical accuracies are of order 324 K (Teff), 0.46 mag (AG), 0.23 mag (E(BP − RP)), 15% (luminosity), and 10% (radius). Being based on only a small number of observable quantities and limited training data, our results are necessarily subject to some extreme assumptions that can lead to strong systematics in some cases (not included in the aforementioned accuracy estimates). One aspect is the non-negativity contraint of our estimates, in particular extinction, which we discuss. Yet in several regions of parameter space our results show very good performance, for example for red clump stars and solar analogues. Large uncertainties render the extinctions less useful at the individual star level, but they show good performance for ensemble estimates. We identify regimes in which our parameters should and should not be used and we define a “clean” sample. Despite the limitations, this is the largest catalogue of uniformly-inferred stellar parameters to date. More precise and detailed astrophysical parameters based on the full BP/RP spectrophotometry are planned as part of the thirdGaiadata release.
  • 关键词:Key wordsenstars: fundamental parametersmethods: data analysismethods: statisticalsurveyscatalogs
国家哲学社会科学文献中心版权所有