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19932026
most citedDetection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

4.6k citations · 60.4k across the 464 of their papers we have counts for

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Showing 2002Show all

10 papers · 1 filter

astro-ph2002★ 188 cited

The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies

Roberto De Propris, M. Colless, S. Driver +27

We have determined the composite luminosity function (LF) for galaxies in 60 clusters from the 2dF Galaxy Redshift Survey. The LF spans the range , and is…

astro-ph2002★ 816 cited

The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe

E. Hawkins, S. Maddox, S. Cole +27

We present a detailed analysis of the two-point correlation function, from the 2dF Galaxy Redshift Survey (2dFGRS). We estimate the redshift-space correlation function, xi(s), from…

astro-ph2002★ 100 cited

The Hawaii-AAO K-band Galaxy Redshift Survey -- Paper I: The Local K-band Luminosity Function

J. -S. Huang, K. Glazebrook, L. L. Cowie +1

We present the K-band local luminosity function derived froma sample of 1056 bright (K<15) K-selected galaxies from the Hawaii-AAO K-band redshift survey. The Hawaii-AAO K-band red…

astro-ph2002★ 349 cited

Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra

Will J. Percival, Will Sutherland, John A. Peacock +24

We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data from the cosmic microwave background (CMB) and from the 2dF Galaxy Redshift Surv…

astro-ph2002★ 2 cited

Studying large-scale structure with the 2dF Galaxy Redshift Survey

J. A. Peacock, M. Colless, I. Baldry +25

The 2dF Galaxy Redshift Survey is the first to observe more than 100,000 redshifts. This allows precise measurements of many of the key statistics of galaxy clustering, in particul…

astro-ph2002★ 181 cited

A new upper limit on the total neutrino mass from the 2dF Galaxy Redshift Survey

O. Elgaroy, O. Lahav, W. J. Percival +27

We constrain f_nu = Omega_nu / Omega_m, the fractional contribution of neutrinos to the total mass density in the Universe, by comparing the power spectrum of fluctuations derived…