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The 2dF QSO redshift survey - Selection function

Abstract:
We report the determination of the 2dF spectroscopic selection function as a function of both redshift and magnitude per observed field. Variations in number densities between fields due to intrinsic clustering in the QSO population can then be disentangled from those caused by varying completenesses in fields observed under differing weather conditions.
Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
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Journal:
NEW ERA OF WIDE FIELD ASTRONOMY
Volume:
232
Pages:
73-74
Publication date:
2001-01-01
Event title:
International Conference on the New Era of Wide Field Astronomy
ISBN:
158381065X
Keywords:
Pubs id:
pubs:4426
UUID:
uuid:1db4d069-95b9-4c29-bfe8-05d1e9d4674e
Local pid:
pubs:4426
Source identifiers:
4426
Deposit date:
2012-12-19

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