Galaxy clustering and bias in the 2dF redshift survey

Details Galaxy clustering and bias in the 2dF redshift survey Galaxy clustering and bias in the 2dF redshift survey

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.2405x&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #24.05; Bulletin of the American Astronomical Society, Vol. 33, p.1347

Astronomy and Astrophysics

Astronomy

Scientific paper

The power spectrum and redshift space distortions are measured from the 2dF galaxy redshift survey using a Karhunen-Loeve eigenmode analysis, allowing model-independent constraints to be placed on P(k), galaxy velocities and bias. The power spectrum is also computed for samples subdivided by luminosity and spectral type jointly, allowing the first measurement of how bias depends on luminosity and type jointly.

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