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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 2005Show all

11 papers · 1 filter

astro-ph2005★ 97 cited

Universal fitting formulae for baryon oscillation surveys

Chris Blake, David Parkinson, Bruce Bassett +3

The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred sca…

astro-ph2005★ 485 cited

The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation

S. Savaglio, K. Glazebrook, D. Le Borgne +10

We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4<z<1.0 from the Gemini Deep Deep Survey and Canada-France Redshift Survey. Deep K and z' band photomet…

astro-ph2005★ 22 cited

The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey

Matt Hilton, Chris Collins, Roberto De Propris +25

The ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey and the 2dF Galaxy Redshift Survey (2dFGRS) respectively comprise the largest, homogeneous X-ray selected cluster ca…

astro-ph2005★ 1.1k cited

The Fourth Data Release of the Sloan Digital Sky Survey

J. K. Adelman-McCarthy et al.

This paper describes the fourth data release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through June 2004. The data release includes five-band…

astro-ph2005★ 11 cited

Dark Energy and Cosmic Sound: w(z) Surveys with the Gemini/Subaru Wide-Field Multi-Object Spectrograph

Karl Glazebrook, Daniel Eisenstein, Arjun Dey +2

This white paper gives an overview of the proposed Gemini/Subaru Wide-Field Multi-Object Spectrograph (WFMOS) and the proposed redshift surveys of 2.6 million galaxies with 0.5<z<3…

astro-ph2005★ 99 cited

Measuring the cosmic evolution of dark energy with baryonic oscillations in the galaxy power spectrum

Karl Glazebrook, Chris Blake

We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation-of-state w(z), usin…