GOODS–Herschel: an infrared main sequence for star-forming galaxies
Citations
3,104 citations
1,626 citations
Cites background from "GOODS–Herschel: an infrared main se..."
...In a joint analysis of the IR SED properties of both nearby and high redshift IR-luminous galaxies, Elbaz et al. (2011) provided an explanatory framework for these observations in terms of the distinction between a majority population of galaxies obeying a “main sequence” correlation between their…...
[...]
...Elbaz et al. (2011) construct a “universal” main sequence SED from the ensemble of high-z Spitzer and Herschel photometry for galaxies in the GOODS fields at 0.3 < z < 2.5....
[...]
1,336 citations
Additional excerpts
...…et al. 2009 (P09); Santini et al. 2009 (S09); Oliver et al. 2010 (O10); Magdis et al. 2010 (M10); Lee et al. 2011 (L11); Rodighiero et al. 2011 (R11); Elbaz et al. 2011 (E11); Karim et al. 2011 (K11); Shim et al. 2011 (S11); Bouwens et al. 2012 (B12); Whitaker et al. 2012 (W12); Zahid et al.…...
[...]
...Elbaz et al. (2011) (E11)....
[...]
1,041 citations
986 citations
References
10,983 citations
"GOODS–Herschel: an infrared main se..." refers methods in this paper
...The GOODSSpitzerIRAC catalogs were created using SExtractor (Bertin & Arnouts 1996),detecting sources in a weighted combination of the 3.6 and 4.5µm images, with matched-aperture photometry in the four IRAC bands, using appropriate aperture corrections to total flux....
[...]
8,607 citations
"GOODS–Herschel: an infrared main se..." refers methods in this paper
...We use below a cosmology withH0=70 kms−1Mpc−1,ΩM = 0.3, ΩΛ = 0.7 and we assume a Salpeter initial mass function (IMF, Salpeter 1955) when deriving SFRs and stellar masses....
[...]
6,640 citations
5,665 citations
5,441 citations
"GOODS–Herschel: an infrared main se..." refers methods in this paper
...Our local galaxy sample was cross-matched with the NRAO VLA Sky Survey (NVSS, Condon et al. 1998) and the Faint Images of the Radio Sky at Twenty-cm (FIRST, Becker, White & Helfand 1995), both obtained with the VLA at 20 cm....
[...]