Determining the lensing fraction of SDSS quasars: Methods and results from the early data release

Bart Pindor, Edwin L. Turner, Robert H. Lupton, J. Brinkmann

Research output: Contribution to journalArticle

25 Scopus citations

Abstract

We present an algorithm for selecting gravitational lens candidates from among Sloan Digital Sky Survey (SDSS) quasars. In median Early Data Release (EDR) conditions, the algorithm allows for the recovery of pairs of equal flux point sources down to separations of ∼0″.7 or with flux ratios up to ∼10:1 at a separation of 1″.5. The algorithm also recovers a wide variety of plausible quad geometries. We also present a method for determining the selection function of this algorithm through the use of simulated SDSS images and introduce a method for calibrating our simulated images through truth testing with real SDSS data. Finally, we apply our algorithm and selection function to SDSS quasars from the EDR to get an upper bound on the lensing fraction. We find 13 candidates among 5120 z > 0.6 SDSS quasars, implying an observed lensing fraction of not more than 4 × 10 -3. There is one likely lens system in our final sample, implying an observed lensing fraction of not less than 3 × 10-5 (95% confidence levels).

Original languageEnglish (US)
Pages (from-to)2325-2340
Number of pages16
JournalAstronomical Journal
Volume125
Issue number5 1769
DOIs
StatePublished - May 2003

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Gravitational lensing
  • Quasars: general

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