The Angular Correlation Function of Galaxies from Early Sloan Digital Sky Survey Data-Reference-Cited by-同舟云学术

The Angular Correlation Function of Galaxies from Early Sloan Digital Sky Survey Data

Published:2002-11 Issue:1 Volume:579 Page:42-47
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Connolly Andrew J.,Scranton Ryan,Johnston David,Dodelson Scott,Eisenstein Daniel J.,Frieman Joshua A.,Gunn James E.,Hui Lam,Jain Bhuvnesh,Kent Stephen,Loveday Jon,Nichol Robert C.,O’Connell Liam,Postman Marc,Scoccimarro Roman,Sheth Ravi K.,Stebbins Albert,Strauss Michael A.,Szalay Alexander S.,Szapudi Istvan,Tegmark Max,Vogeley Michael S.,Zehavi Idit,Annis James,Bahcall Neta,Brinkmann J.,Csabai Istvan,Doi Mamoru,Fukugita Masataka,Hennessy G. S.,Hindsley Robert,Ichikawa Takashi,Ivezić Željko,Kim Rita S. J.,Knapp Gillian R.,Kunszt Peter,Lamb D. Q.,Lee Brian C.,Lupton Robert H.,McKay Timothy A.,Munn Jeff,Peoples John,Pier Jeff,Rockosi Constance,Schlegel David,Stoughton Christopher,Tucker Douglas L.,Yanny Brian,York Donald G.,

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/579/i=1/a=42/pdf

Reference34 articles.

1. The Edinburgh–Durham Southern Galaxy Catalogue – III. w(θ) from the full survey

2. Evolution of galaxy clustering: new data on the angular correlation function of faint galaxies

3. Csabai, I., etal 2002, AJ, submitted

4. The Three‐dimensional Power Spectrum from Angular Clustering of Galaxies in Early Sloan Digital Sky Survey Data

5. Maximum likelihood estimates of the two- and three-dimensional power spectra of the APM Galaxy Survey

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