Quasars narrow absorption lines from SDSS : J/MNRAS/450/3904


Authors : Chen Z.-F. orcid , Gu Q.-S., Chen Y.-M. (hide) , Gu Q.-S., Chen Y.-M. et..al

Bibcode : 2015MNRAS.450.3904C (ADS) (Simbad) (Objects) (hide)

CDS Keywords : QSOs; Photometry, SDSS; Redshifts; Equivalent widths
UAT : Quasars, Optical astronomy, Sloan photometry, Redshifted, Line intensities

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Inserted into VizieR : 18-Dec-2017
Last modification : 14-Aug-2024

Narrow absorption lines with two observations from the Sloan Digital Sky Survey. (2015)

Keywords : catalogues - surveys - quasars absorption lines - quasars: general

Abstract:We assemble 3524 quasars from the Sloan Digital Sky Survey (SDSS) with repeated observations to search for variations of the narrow C IV {lambda}{lambda}1548, 1551 and Mg II {lambda}{lambda}2796, 2803 absorption doublets in spectral regions shortward of 7000{AA} in the observed frame, which corresponds to time-scales of about 150-2643d in the quasar rest frame. In these quasar spectra, we detect 3580 CIV absorption systems with z_abs_=1.5188-3.5212 and 1809 MgII absorption systems with z_abs_=0.3948-1.7167. In term of the absorber velocity ({beta}) distribution in the quasar rest frame, we find a substantial number of CIV absorbers with {beta}<0.06, which might be connected to absorption of quasar outflows. The outflow absorption peaks at ...(more)
Abstract: (hide)
The Baryon Oscillation Spectroscopic Survey (BOSS: Eisenstein et al. 2011AJ....142...72E; Paris et al. 2012, Cat. VII/269) is the main dark-time legacy survey of the third stage of the SDSS, which used the same 2.5-m telescope (Gunn et al. 2006AJ....131.2332G; Ross et al. 2012, J/ApJS/199/3) as the first and second stages of the SDSS (hereafter SDSS-I/II). SDSS-I/II spectra have a wavelength coverage from 3800-9200{AA} with a spectral resolution of 1800-2200 (e.g. York et al. 2000AJ....120.1579Y). BOSS spectra span a range from 3600-10500{AA} at a resolution of 1300-2500 (Paris et al. 2012, Cat. VII/269). During the first two years, BOSS detected 87822 quasars over an area of 3275 deg^2^, including 7932 quasars that were observed by SDSS-I/II as well. Quasars observed by both SDSS-I/II and BOSS provide a remarkable chance to study the variabilities of absorption lines in a large population. Throughout this work, we take the quasar emission redshifts provided by Hewett & Wild (2010, J/MNRAS/405/2302, http://das.sdss.org/va/Hewett_Wild_dr7qso_newz/) directly.

  • VII/269 : SDSS Quasar Catalog, DR9Q (Paris+, 2012)
  • VII/279 : SDSS quasar catalog
  • J/ApJ/613/129 : Equivalent widths of QSOs (Wise+, 2004)
  • J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)
  • J/ApJS/199/3 : The quasars MMT-BOSS pilot survey (Ross+, 2012)
  • J/MNRAS/434/163 : QSOs narrow absorption line variability (Hacker+, 2013)
  • J/ApJS/210/7 : BOSS narrow CIV absorption lines. I. zem<=2.4 (Chen+, 2014)
  • J/ApJS/215/12 : BOSS narrow CIV absorption lines. II. zem>2.4 (Chen+, 2014)

                
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