An Optical Catalog of Galaxy Clusters Obtained from an Adaptive Matched Filter Finder Applied to SDSS DR6

TL;DR

This paper introduces a new galaxy cluster catalog from SDSS DR6 using an adaptive matched filter, providing detailed properties, cross-catalog comparisons, and correlations with X-ray data to enhance understanding of galaxy clusters.

Contribution

The paper presents a novel adaptive matched filter method for galaxy cluster detection and provides a comprehensive catalog with detailed properties and cross-matching with other surveys.

Findings

Identified 69,173 galaxy clusters in SDSS DR6.

Found strong correlations between optical and X-ray properties.

Achieved 30-50% matching with other cluster catalogs.

Abstract

We present a new cluster catalog extracted from the Sloan Digital Sky Survey Data Release 6 (SDSS DR6) using an adaptive matched filter (AMF) cluster finder. We identify 69,173 galaxy clusters in the redshift range 0.045 $\le z <$ 0.78 in 8420 sq. deg. of the sky. We provide angular position, redshift, richness, core and virial radii estimates for these clusters, as well as an error analysis for each of these quantities. We also provide a catalog of more than 205,000 galaxies representing the three brightest galaxies in the $r$ band which are possible BCG candidates. We show basic properties of the BCG candidates and study how their luminosity scales in redshift and cluster richness. We compare our catalog with the maxBCG and GMBCG catalogs, as well as with that of Wen, Han, and Liu. We match between 30% and 50% of clusters between catalogs over all overlapping redshift ranges. We find that the percentage of matches increases with the richness for all catalogs. We cross match the AMF catalog with available X-ray data in the same area of the sky and find 539 matches, 119 of which with temperature measurements. We present scaling relations between optical and X-ray properties and cluster center comparison. We find that both $\Lambda_{200}$ and $R_{200}$ correlate well with both $L_X$ and $T_X$, with no significant difference in trend if we restrict the matches to flux-limited X-ray samples.