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The redshift of a lensing galaxy in PMN J0134 - 0931

  • Patrick B. Hall
  • , Gordon T. Richards
  • , Donald G. York
  • , Charles R. Keeton
  • , David V. Bowen
  • , Donald P. Schneider
  • , David J. Schlegel
  • , J. Brinkmann

Research output: Contribution to journalReview articlepeer-review

Abstract

The Sloan Digital Sky Survey (SDSS) automatically targeted as a quasar candidate the recently discovered, gravitationally lensed, extremely reddened z = 2.2 quasar PMN 0134-0931. The SDSS spectrum exhibits Ca II absorption at z = 0.76451, which we identify as the redshift of a lensing galaxy. Hubble Space Telescope imaging shows that components C, D, and E of the system are significantly redder than components A or B and detects faint galaxy emission between D and A+B. The redshift of the dust responsible for the reddening remains unconstrained with current data. However, we outline a model wherein lensing and differential reddening by a z = 0.76451 galaxy pair can entirely explain this system.

Original languageEnglish (US)
Pages (from-to)L51-L54
JournalAstrophysical Journal
Volume575
Issue number2 II
DOIs
StatePublished - Aug 20 2002

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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