UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)

Details UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011) UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21930030b&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/193/30. Originally published in: 2011ApJS..193...30B

Physics

Redshifts, Galaxies: Ir, Models

Scientific paper

The present work is based on the multi-wavelength catalog of IRAC 3.6+4.5um selected galaxies in the EGS (RA=14h14m, DEC=+53°30') presented in Paper I (Barro et al. 2011, Cat. J/ApJS/193/13). We cross-correlated our IRAC-selected catalog with the X-ray (Chandra) and radio (VLA/20cm) catalogs of Laird et al. (2009, Cat. J/ApJS/180/102) and Ivison et al. (2007ApJ...660L..77I), and with all the spectroscopic redshifts from DEEP2 DR3 and a small sample of 238 spectroscopically confirmed Lyman break galaxies (LBGs) from Steidel et al. (2003, Cat. J/ApJ/592/728).
(3 data files).

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