Bibcode
Lyke, Brad W.; Higley, Alexandra N.; McLane, J. N.; Schurhammer, Danielle P.; Myers, Adam D.; Ross, Ashley J.; Dawson, Kyle; Chabanier, Solène; Martini, Paul; Busca, Nicolás G.; Mas des Bourboux, Hélion du; Salvato, Mara; Streblyanska, Alina; Zarrouk, Pauline; Burtin, Etienne; Anderson, Scott F.; Bautista, Julian; Bizyaev, Dmitry; Brandt, W. N.; Brinkmann, Jonathan; Brownstein, Joel R.; Comparat, Johan; Green, Paul; Macorra, Axel de la; Gutiérrez, Andrea Muñoz; Hou, Jiamin; Newman, Jeffrey A.; Palanque-Delabrouille, Nathalie; Pâris, Isabelle; Percival, Will J.; Petitjean, Patrick; Rich, James; Rossi, Graziano; Schneider, Donald P.; Smith, Alexander; Vivek, M.; Weaver, Benjamin Alan
Bibliographical reference
The Astrophysical Journal Supplement Series
Advertised on:
9
2020
Citations
338
Refereed citations
292
Description
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 subcatalogs (the current versions are DR16Q_v4 and DR16Q_Superset_v3 at https://data.sdss.org/sas/dr16/eboss/qso/DR16Q/): 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%-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 Hα, Hβ, Mg II, C III], C IV, and Lyα. 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 multiwavelength data for quasars from the Galaxy Evolution Explorer, UKIDSS, the Wide-field Infrared Survey Explorer, FIRST, ROSAT/2RXS, XMM-Newton, and Gaia. Calibrated digital optical spectra for these quasars can be obtained from the SDSS Science Archive Server.
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Morphology and dynamics of the Milky Way
This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way pretends to provide a data base for the stellar distribution in the most remote and heavily obscured regions of our Galaxy, through the development of semiempirical models based on the
Martín
López Corredoira