The Clustering of 12 and 22 micron Star Forming Galaxies from WISE/SDSS Surveys

Details The Clustering of 12 and 22 micron Star Forming Galaxies from WISE/SDSS Surveys The Clustering of 12 and 22 micron Star Forming Galaxies from WISE/SDSS Surveys

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21743201d&link_type=abstract

American Astronomical Society, AAS Meeting #217, #432.01; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The Wide-Field Infrared Survey Explorer (WISE) satellite has surveyed the entire sky at 12 and 22 microns down to a flux limit of 1 and 6 mJy, respectively. By cross-matching this data with the SDSS, we derive a large sample of star forming galaxies. Herein, we present a comprehensive study of the clustering of these sources via the projected cross-correlation function, w(rp), and matched control samples. This allows us to trace the clustering relative bias of the population as function of the star formation rate, and characterize in detail the typical environments of star forming galaxies in the local universe.

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