A TWO-PARAMETER MODEL FOR THE INFRARED/SUBMILLIMETER/RADIO SPECTRAL ENERGY DISTRIBUTIONS OF GALAXIES AND ACTIVE GALACTIC NUCLEI

被引:329
作者
Dale, Daniel A. [1 ]
Helou, George [2 ]
Magdis, Georgios E. [3 ]
Armus, Lee [4 ]
Diaz-Santos, Tanio [4 ]
Shi, Yong [5 ]
机构
[1] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA
[2] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA
[3] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[4] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[5] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
基金
美国国家航空航天局;
关键词
dust; extinction; galaxies: active; galaxies: star formation; infrared: ISM; STAR-FORMING GALAXIES; SPITZER-SPACE-TELESCOPE; POLYCYCLIC AROMATIC-HYDROCARBONS; ULTRALUMINOUS INFRARED GALAXIES; HIGH-REDSHIFT; NEARBY GALAXIES; MIDINFRARED SPECTRUM; LUMINOSITY FUNCTIONS; RADIATIVE-TRANSFER; INTERSTELLAR DUST;
D O I
10.1088/0004-637X/784/1/83
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A two-parameter semi-empirical model is presented for the spectral energy distributions of galaxies with contributions to their infrared-submillimeter-radio emission from both star formation and accretion disk-powered activity. This model builds upon a previous one-parameter family of models for star-forming galaxies, and includes an update to the mid-infrared emission using an average template obtained from Spitzer Space Telescope observations of normal galaxies. Star-forming/active galactic nucleus (AGN) diagnostics based on polycyclic aromatic hydrocarbon equivalent widths and broadband infrared colors are presented, and example mid-infrared AGN fractional contributions are estimated from model fits to the Great Observatories All-Sky LIRG Survey sample of nearby U/LIRGS and the Five mJy Unbiased Spitzer Extragalactic Survey sample of 24 mu m selected sources at redshifts 0 less than or similar to z less than or similar to 4.
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