Multi-wavelength properties of Spitzer selected starbursts at z ~ 2

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Volume 508 / No 1 (December II 2009)

A&A, 508 1 (2009) 117-132

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Table 2:

Related *Spitzer*-selected $z\sim 2$ ULIRGs samples.
Sample	N	$F_{\rm 24~\mu m}$	$\langle F_{\rm {24~\mu m}}\rangle$	IR color selection	r	density
		$\mu$ Jy	$\mu$ Jy		Vega	deg^-2
This work	33	400	566	$F_{\rm {3.6~\mu m}}$ $F_{\rm {4.5~\mu m}}$ $F_{\rm {5.8~\mu m}}$ $F_{\rm {8.0~\mu m}}$	23	65
Lonsdale et al. (2008)	61	400	819	$F_{\rm {3.6~\mu m}}$ $F_{\rm {4.5~\mu m}}$ $F_{\rm {5.8~\mu m}}$ $F_{\rm {8.0~\mu m}}$	23	55
Farrah et al. (2008)	32	500	726	$F_{\rm {3.6~\mu m}}$ $F_{\rm {4.5~\mu m}}$ $F_{\rm {5.8~\mu m}}$ and $F_{\rm {4.5~\mu m}}$ $F_{\rm {8.0~\mu m}}$	23	34
Huang et al. (2009)^a	12	500	689	0 [3.6]-[4.5] 0.4
				-0.7 [3.6]-[8.0] 0.5
Magliocchetti et al. (2007)	793	350			25.5	200
Yan et al. (2005)	52	900		$\log_{10}(\nu f_{\nu}(\rm {24~\mu m})/\nu {\textit f}_{\nu}(\rm {8~\mu m}))$ 0.5
				$\log_{10}(\nu f_{\nu}(\rm {24~\mu m})/\nu {\textit f}_{\nu}(\rm {0.7~\mu m})$ ) 1.0

^a The sample of Huang et al. (2009) differs by only one source from the one of Younger et al. (2009).

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