论文标题
斯隆数字天空调查类星体目录:第十六个数据发布
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
论文作者
论文摘要
我们介绍了最终的Sloan数字天空调查IV(SDSS-IV)的类星体目录,该目录从扩展的Baryon振荡光谱调查(EBOSS)的数据发行16中。该目录包括迄今为止最大的光谱确认的类星体选择。完整的目录包括两个子催化:一个针对类星体的所有SDSS-IV/EBOSS对象的“超集”,其中包含1,440,615个观测和一个仅类型的目录,其中包含750,414个类星体,其中包括225,082个新的类型的SDSS释放,以及首次出现在SDS量中的新产品。 SDSS-I/II/III。我们提供这些类星体的自动识别和红移信息以及320,161个光谱的视觉检查数据。估计仅类星体目录为99.8%,污染为0.3%至1.3%。自动检查和视觉检查红移是通过主成分分析和发射线得出的红移补充的。我们包括H $α$,H $β$,Mg II,C III],C IV和LY $α$的发射线红移。自动化算法产生的识别和关键特征介绍了99,856个广泛的吸收线类星体和35,686个阻尼的Lyman alpha carsars。除了SDSS光度数据外,我们还提供了来自Galex,Ukidss,Wise,First,Rosat/2RXS,XMM-Newton和Gaia的数量数据的多波长数据。这些类星体的校准数字光谱可以从SDSS Science Archive Server获得。
We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog comprises the largest selection of spectroscopically confirmed quasars to date. The full catalog includes two sub-catalogs: a "superset" of all SDSS-IV/eBOSS objects targeted as quasars containing 1,440,615 observations and a quasar-only catalog containing 750,414 quasars, including 225,082 new quasars appearing in an SDSS data release for the first time, as well as known quasars from SDSS-I/II/III. We present automated identification and redshift information for these quasars alongside data from visual inspections for 320,161 spectra. The quasar-only catalog is estimated to be 99.8% complete with 0.3% to 1.3% contamination. Automated and visual inspection redshifts are supplemented by redshifts derived via principal component analysis and emission lines. We include emission line redshifts for H$α$, H$β$, Mg II, C III], C IV, and Ly$α$. Identification and key characteristics generated by automated algorithms are presented for 99,856 Broad Absorption Line quasars and 35,686 Damped Lyman Alpha quasars. In addition to SDSS photometric data, we also present multi-wavelength data for quasars from GALEX, UKIDSS, WISE, FIRST, ROSAT/2RXS, XMM-Newton, and Gaia. Calibrated digital optical spectra for these quasars can be obtained from the SDSS Science Archive Server.