SWIRE ELAIS-S1 IR-peak galaxy IR fluxes (Berta+, 2007)

Details SWIRE ELAIS-S1 IR-peak galaxy IR fluxes (Berta+, 2007) SWIRE ELAIS-S1 IR-peak galaxy IR fluxes (Berta+, 2007)

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34760151b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/476/151. Originally published in: 2007A&A...476..151B

Physics

Galaxies: Ir, Photometry: Infrared

Scientific paper

Main data on the IR-peakers sample in the SWIRE ELAIS-S1 field. For each IR-peak galaxy, we report R band magnitude (AB units, from the ESIS survey, Berta et al., 2006A&A...451..881B), Spitzer SWIRE fluxes (Lonsdale et al., 2003PASP..115..897L, 2004ApJS..154...54L), photometric redshift (based on Hyper-z fit, Bolzonella et al., 2000A&A...363..476B), the stellar mass and its minimal-maximal range. The stellar mass estimate is based on mixed stellar population (MSP) synthesis (Berta et al., 2004A&A...418..913B). The minimal and maximal stellar masses are obtained by exploring the SFH-extinction parameter space with the Adaptive Simulated Annealing algorithm (Ingber et al., 2001, http://www.ingber.com/asa01_lecture.pdf). See the paper associated to these data for more details.
(1 data file).

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