Mathematics – Logic
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21742105l&link_type=abstract
American Astronomical Society, AAS Meeting #217, #421.05; Bulletin of the American Astronomical Society, Vol. 43, 2011
Mathematics
Logic
Scientific paper
Understanding the contribution of infrared (IR) galaxies to the total star formation rate (SFR) is an important topic in galaxy formation. The earlier work by Nagamine et al. (2005) showed a reasonable agreement between cosmological simulations and observations regarding the space density of star-forming galaxies. Here we estimate the IR spectral energy distributions (SEDs) from the simulated high-redshift galaxies by coupling the cosmological SPH simulation output from GADGET-3 with the GRASIL (the population synthesis code by Silva et al., 1998). We compute the luminosity function (LF), galaxy number counts, and redshift distribution in IRAC and MIPS bands of Spitzer observations.
Choi Jaedong
Lee Tae Song
Nagamine Kentaro
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