- Abstract:
-
We cross-correlate APM and SDSS galaxies with background QSOs from the 2dF QSO Redshift Survey, and detect a significant (2.8sigma) anti-correlation. The lack of a signal between 2dF stars and our galaxy samples suggests the anti-correlation is not due to a systematic error. The possibility that dust in the foreground galaxies could produce the anti-correlation is marginally rejected, at the 2sigma level through consideration of QSO colours. It is possible that dust that obscures QSOs without...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2005.08955.x
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- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 359
- Issue:
- 2
- Pages:
- 741-754
- Publication date:
- 2005-02-23
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:8eaaa428-5897-48fa-8b73-6d851fda7080
- Source identifiers:
-
28862
- Local pid:
- pubs:28862
- Language:
- English
- Keywords:
- Copyright date:
- 2005
- Notes:
- 15 pages, 10 figures, accepted for publication in MNRAS
Journal article
On Statistical Lensing and the Anti-Correlation Between 2dF QSOs and Foreground Galaxies
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