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KL Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early SDSS Data
SDSS Collaboration, Alexander S. Szalay, Bhuvnesh Jain +25
We present measurements of parameters of the 3-dimensional power spectrum of galaxy clustering from 222 square degrees of early imaging data in the Sloan Digital Sky Survey. The pr…
The Angular Correlation Function of Galaxies from Early SDSS Data
SDSS Collaboration, Andrew Connolly, Ryan Scranton +22
The Sloan Digital Sky Survey is one of the first multicolor photometric and spectroscopic surveys designed to measure the statistical properties of galaxies within the local Univer…
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data
Scott Dodelson, Vijay K. Narayanan, Max Tegmark +22
Early photometric data from the Sloan Digital Sky Survey (SDSS) contain angular positions for 1.5 million galaxies. In companion papers, the angular correlation function and…
A Limit on the Large Angular Scale Polarization of the Cosmic Microwave Background
Brian G. Keating, Christopher W. O'Dell, Angelica de Oliveira-Costa +5
We present an upper limit on the polarization of the Cosmic Microwave Background at 7 degree angular scales in the frequency band between 26 and 36 GHz, produced by the POLAR exper…
The Angular Power Spectrum of Galaxies from Early SDSS Data
SDSS Collaboration, Max Tegmark, Scott Dodelson +21
We compute the angular power spectrum C_l from 1.5 million galaxies in early SDSS data on large angular scales, l<600. The data set covers about 160 square degrees, with a characte…
Analysis of Systematic Effects and Statistical Uncertainties in Angular Clustering of Galaxies from Early SDSS Data
SDSS Collaboration, Ryan Scranton, David Johnston +21
The angular distribution of galaxies encodes a wealth of information about large scale structure. Ultimately, the Sloan Digital Sky Survey (SDSS) will record the angular positions…