期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 406, 期 4, 页码 2235-2248出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2010.16848.x
关键词
quasars: absorption lines; dust; extinction
资金
- Agence Nationale de la Recherche [ANR-08-BLAN-0316-01]
- Alfred P. Sloan Foundation
- National Science Foundation
- U.S. Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- American Museum of Natural History
- Astrophysical Institute Potsdam
- University of Basel
- University of Cambridge
- Case Western Reserve University
- University of Chicago
- Drexel University
- Fermilab
- Institute for Advanced Study
- Japan Participation Group
- Johns Hopkins University
- Joint Institute for Nuclear Astrophysics
- Kavli Institute for Particle Astrophysics and Cosmology
- Korean Scientist Group
- Chinese Academy of Sciences (LAMOST)
- Los Alamos National Laboratory
- Max-Planck-Institute for Astronomy (MPIA)
- Max-Planck-Institute for Astrophysics (MPA)
- New Mexico State University
- Ohio State University
- University of Pittsburgh
- University of Portsmouth
- Princeton University
- United States Naval Observatory
- University of Washington
- Agence Nationale de la Recherche (ANR) [ANR-08-BLAN-0316] Funding Source: Agence Nationale de la Recherche (ANR)
We searched for evidence of the reddening of background quasi-stellar object (QSO) spectra from the Sloan Digital Sky Survey (SDSS) due to dust in intervening damped Lyman alpha systems (DLAs). We utilize the two Data Releases DR5 and DR7 to arrive at sample sizes of 475 (DR5) and 676 (DR7) absorbers, based on two different published lists of SDSS DLAs. Both samples span roughly the redshift range of 2.2 < z(abs) < 5.2, with a mean of z similar to 3.0, and the majority of the DLAs (75 per cent) below z = 3.3. We construct geometric mean spectra in the absorber rest frames ranging from 1240 to similar to 2800 A, and composite spectra of samples matching the 'DLA' QSOs in i-band magnitude and emission redshift z(em), but without absorption lines. By comparing the slopes of these composite spectra with their matched counterparts, we find no sign of reddening in the ensemble of the absorbers from these samples. Owing to both the unprecedently large sizes of the DLA samples themselves and the non-DLA SDSS QSO sample, from which we can draw our matching spectra, we can place very tight limits for this non-detection (<< E(B - V)>> = -0.0013 +/- 0.0025 (DR5) and << E(B - V)>> = -0.0017 +/- 0.0022 (DR7). Interestingly, when applying our technique to the samples of York et al., Vanden Berk et al. (intervening and intrinsic Mg ii absorbers) and the smaller DLA subsample and pool of comparison QSOs of Vladilo et al., we do recover their results, i.e. detect the same amount of reddening as these authors do. Furthermore, we have tested whether subsamples of our large sample in categories involving the absorbers (H i column densities, presence or absence of accompanying metal absorption, absorber redshift) or the background quasars (emission redshift, brightness) do reveal dust extinction, but found no trends. These results are at odds with both detections of dust reddening from previous studies and expectations from observations of high-redshift galaxies.
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