Journal
ASTRONOMICAL JOURNAL
Volume 128, Issue 3, Pages 1017-1045Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/423038
Keywords
galaxies : clusters : general; methods : numerical; surveys
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We present an optically selected galaxy cluster catalog from similar to 2700 deg(2) of the digitized Second Palomar Observatory Sky Survey (DPOSS), spanning the redshift range 0.1less than or similar tozless than or similar to0.5, providing an intermediate-redshift supplement to the previous DPOSS cluster survey. This new catalog contains 9956 cluster candidates and is the largest resource of rich clusters in this redshift range to date. The candidates are detected using the best DPOSS plates based on seeing and limiting magnitude. The search is further restricted to high galactic latitude (\b\ > 50degrees), where stellar contamination is modest and nearly uniform. We also present a performance comparison of two different detection methods applied to this data, the adaptive kernel and Voronoi tessellation techniques. In the regime where both catalogs are expected to be complete, we find excellent agreement, as well as with the most recent surveys in the literature. Extensive simulations are performed and applied to the two different methods, indicating a contamination rate of similar to 5%. These simulations are also used to optimize the algorithms and evaluate the selection function for the final cluster catalog. Redshift and richness estimates are also provided, making possible the selection of subsamples for future studies.
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