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A glance at the host galaxy of high-redshift quasars using strong damped lyman-α systems as coronagraphs

  • Hayley Finley
  • , Patrick Petitjean
  • , Isabelle Pâris
  • , Pasquier Noterdaeme
  • , Jonathan Brinkmann
  • , Adam D. Myers
  • , Nic Ross
  • , Donald P. Schneider
  • , Dmitry Bizyaev
  • , Howard Brewington
  • , Garrett Ebelke
  • , Elena Malanushenko
  • , Viktor Malanushenko
  • , Daniel Oravetz
  • , Kaike Pan
  • , Audrey Simmons
  • , Stephanie Snedden

Research output: Contribution to journal › Article › peer-review

Abstract

We searched quasar spectra from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) for the rare occurrences where a strong damped Lyman-Á absorber (DLA) blocks the Broad Line Region emission from the quasar and acts as a natural coronagraph to reveal narrow LyÁ emission from the host galaxy. We define a statistical sample of 31 DLAs in Data Release 9 (DR9) with log N(H i) iÝ 21.3 cm.2 located at less than 1500 km s.1 from the quasar redshift. In 25% (8) of these DLAs, a strong narrow LyÁ emission line is observed with flux i"25 iÁ 10.17 erg s.1 cm.2 on average. For DLAs without this feature in their troughs, the average 3-Ò upper limit is.

Original languageEnglish
Article numberA111
JournalAstronomy & Astrophysics
Volume558
DOIs
Publication statusPublished - 2013

Keywords / Materials (for Non-textual outputs)

  • Quasars: absorption lines
  • Quasars: emission lines

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