A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

作者: Matthieu Béthermin , Emanuele Daddi , Georgios Magdis , Mark T. Sargent , Yashar Hezaveh

DOI: 10.1088/2041-8205/757/2/L23

关键词:

摘要: We reproduce the mid-infrared to radio galaxy counts with a new empirical model based on our current understanding of evolution main-sequence (MS) and starburst (SB) galaxies. rely simple Spectral Energy Distribution (SED) library Herschel observations: single SED for MS another one SB, getting warmer redshift. Our is able recent measurements performed Herschel, including per redshift slice. This agreement demonstrates power 2 Star-Formation Modes (2SFM) decomposition describing statistical properties infrared sources their cosmic time. discuss relative contribution SB galaxies number at various wavelengths flux densities. also show that are responsible bump in 1.4 GHz around 50 {\mu}Jy. Material (predictions, library, mock catalogs...) available online this http URL

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