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Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
Teppei Okumura, Takahiko Matsubara, Daniel J. Eisenstein +4
We study the large-scale anisotropic two-point correlation function using 46,760 luminous red galaxies at redshifts 0.16 -- 0.47 from the Sloan Digital Sky Survey. We measure the c…
Low Resolution Spectral Templates For Galaxies From 0.2 -- 10 microns
R. J. Assef, C. S. Kochanek, M. Brodwin +11
We built an optimal basis of low resolution templates for galaxies over the wavelength range from 0.2 to 10 m using a variant of the algorithm presented by Budavari et al. (2000…
The Sloan Digital Sky Survey Quasar Lens Search. II. Statistical Lens Sample from the Third Data Release
Naohisa Inada, Masamune Oguri, Robert H. Becker +31
We report the first results of our systematic search for strongly lensed quasars using the spectroscopically confirmed quasars in the Sloan Digital Sky Survey (SDSS). Among 46,420…
The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
Masamune Oguri, Naohisa Inada, Michael A. Strauss +31
We present cosmological results from the statistics of lensed quasars in the Sloan Digital Sky Survey (SDSS) Quasar Lens Search. By taking proper account of the selection function,…
Evidence for a Z < 8 Origin of the Source Subtracted Near Infrared Background
Rodger I. Thompson, Daniel Eisenstein, Xiaohui Fan +2
This letter extends our previous fluctuation analysis of the near infrared background at 1.6 microns to the 1.1 micron (F110W) image of the Hubble Ultra Deep field. When all detect…
Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
Will J. Percival, Shaun Cole, Daniel J. Eisenstein +4
We introduce a method to constrain general cosmological models using Baryon Acoustic Oscillation (BAO) distance measurements from galaxy samples covering different redshift ranges,…