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THE CLUSTERING CHARACTERISTICS OF H I-SELECTED GALAXIES FROM THE 40% ALFALFA SURVEY
The 40% Arecibo Legacy Fast ALFA survey catalog ( alpha .40) of ~10, 150 H I-selected galaxies is used to analyze the clustering properties of gas-rich galaxies. By employing the Landy-Szalay estimator and a full covariance analysis for the two-point galaxy-galaxy correlation function, we obtain the...
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Published in: | The Astrophysical journal 2012-05, Vol.750 (1), p.1-11 |
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creator | MARTIN, Ann M GIOVANELLI, Riccardo HAYNES, Martha P GUZZO, Luigi |
description | The 40% Arecibo Legacy Fast ALFA survey catalog ( alpha .40) of ~10, 150 H I-selected galaxies is used to analyze the clustering properties of gas-rich galaxies. By employing the Landy-Szalay estimator and a full covariance analysis for the two-point galaxy-galaxy correlation function, we obtain the real-space correlation function and model it as a power law, [xi](r) = (r/r sub(0)) super(- gamma ), on scales |
doi_str_mv | 10.1088/0004-637X/750/1/38 |
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The robust measurement of the correlation function for gas-rich galaxies obtained via the alpha .40 sample constrains models of the distribution of H I in simulated galaxies, and will be employed to better understand the role of gas in environmentally dependent galaxy evolution.</abstract><cop>Bristol</cop><pub>IOP</pub><doi>10.1088/0004-637X/750/1/38</doi><tpages>11</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Alfalfa ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Clustering COMPUTERIZED SIMULATION Correlation analysis CORRELATION FUNCTIONS DISTANCE Earth, ocean, space Exact sciences and technology GALACTIC EVOLUTION GALAXIES GALAXY CLUSTERS Legacy Mathematical models Occupation RED SHIFT Small scale UNIVERSE |
title | THE CLUSTERING CHARACTERISTICS OF H I-SELECTED GALAXIES FROM THE 40% ALFALFA SURVEY |
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