An excess of damped Lyman α galaxies near quasi-stellar objects

Dave Russell, Sara L. Ellison, Chris R. Benn

Research output: Contribution to journalArticle

Abstract

ABSTRACT We present a sample of 33 damped Lyman α systems (DLAs) discovered in the Sloan Digital Sky Survey (SDSS) whose absorption redshifts (z abs) are within 6000 km s -1 of the quasi-stellar object's (QSO) systemic redshift (z sys). Our sample is based on 731 2.5 < z sys < 4.5 non-broad absorption line (non-BAL) QSOs from Data Release 3 (DR3) of the SDSS. We estimate that our search is ≈100 per cent complete for absorbers with N(H i) ≥ 2 × 10 20 cm -2. The derived number density of DLAs per unit redshift, n(z), within Δv < 6000 km s -1 is higher (3.5σ significance) by almost a factor of 2 than that of intervening absorbers observed in the SDSS DR3, i.e. there is evidence for an overdensity of galaxies near the QSOs. This provides a physical motivation for excluding DLAs at small velocity separations in surveys of intervening 'field' DLAs. In addition, we find that the overdensity of proximate DLAs is independent of the radio-loudness of the QSO, consistent with the environments of radio-loud and radio-quiet QSOs being similar.

Original languageEnglish (US)
Pages (from-to)412-422
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume367
Issue number1
DOIs
StatePublished - Mar 1 2006

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quasars
galaxies
absorbers
radio
loudness
estimates

Keywords

  • Early Universe
  • Quasars: emission lines
  • Quasars: general
  • Radio continuum: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

An excess of damped Lyman α galaxies near quasi-stellar objects. / Russell, Dave; Ellison, Sara L.; Benn, Chris R.

In: Monthly Notices of the Royal Astronomical Society, Vol. 367, No. 1, 01.03.2006, p. 412-422.

Research output: Contribution to journalArticle

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N2 - ABSTRACT We present a sample of 33 damped Lyman α systems (DLAs) discovered in the Sloan Digital Sky Survey (SDSS) whose absorption redshifts (z abs) are within 6000 km s -1 of the quasi-stellar object's (QSO) systemic redshift (z sys). Our sample is based on 731 2.5 < z sys < 4.5 non-broad absorption line (non-BAL) QSOs from Data Release 3 (DR3) of the SDSS. We estimate that our search is ≈100 per cent complete for absorbers with N(H i) ≥ 2 × 10 20 cm -2. The derived number density of DLAs per unit redshift, n(z), within Δv < 6000 km s -1 is higher (3.5σ significance) by almost a factor of 2 than that of intervening absorbers observed in the SDSS DR3, i.e. there is evidence for an overdensity of galaxies near the QSOs. This provides a physical motivation for excluding DLAs at small velocity separations in surveys of intervening 'field' DLAs. In addition, we find that the overdensity of proximate DLAs is independent of the radio-loudness of the QSO, consistent with the environments of radio-loud and radio-quiet QSOs being similar.

AB - ABSTRACT We present a sample of 33 damped Lyman α systems (DLAs) discovered in the Sloan Digital Sky Survey (SDSS) whose absorption redshifts (z abs) are within 6000 km s -1 of the quasi-stellar object's (QSO) systemic redshift (z sys). Our sample is based on 731 2.5 < z sys < 4.5 non-broad absorption line (non-BAL) QSOs from Data Release 3 (DR3) of the SDSS. We estimate that our search is ≈100 per cent complete for absorbers with N(H i) ≥ 2 × 10 20 cm -2. The derived number density of DLAs per unit redshift, n(z), within Δv < 6000 km s -1 is higher (3.5σ significance) by almost a factor of 2 than that of intervening absorbers observed in the SDSS DR3, i.e. there is evidence for an overdensity of galaxies near the QSOs. This provides a physical motivation for excluding DLAs at small velocity separations in surveys of intervening 'field' DLAs. In addition, we find that the overdensity of proximate DLAs is independent of the radio-loudness of the QSO, consistent with the environments of radio-loud and radio-quiet QSOs being similar.

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