Evolution of the dusty infrared luminosity function from z = 0 to z = 2.3 using observations from Spitzer

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Volume 528 (April 2011)

A&A, 528 (2011) A35

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Table B.1

MIPS sources in GOODS-N with .

Name	IRAC position	F_24 μm			Cov_24 μm	F_70 μm			Cov_70 μm
	α_J2000 δ_J2000	μJy	μJy	μJy	s	mJy	mJy	mJy	s

MIPSJ123539.5+621129.0	12:35:39.48 +62:11:29.02	42.6	5.6	6.7	10873	< 2.9	...	...	5601
MIPSJ123539.5+621243.8	12:35:39.54 +62:12:43.78	54.0	4.6	6.7	10239	< 2.2	...	...	4747
MIPSJ123539.9+621324.8	12:35:39.94 +62:13:24.79	52.2	4.2	6.7	9512	< 2.4	...	...	3728
MIPSJ123540.2+621224.2	12:35:40.17 +62:12:24.16	107.1	7.2	8.2	11518	< 3.5	...	...	5453
MIPSJ123540.7+621218.9	12:35:40.70 +62:12:18.93	107.1	5.8	8.2	11934	< 3.5	...	...	5711
MIPSJ123541.0+621136.1	12:35:41.00 +62:11:36.13	139.8	4.1	8.3	12437	< 4.6	...	...	6409
MIPSJ123541.4+621217.4	12:35:41.39 +62:12:17.37	419.5	5.2	11.7	12395	2.6	0.3	0.6	6102
MIPSJ123541.4+621316.5	12:35:41.41 +62:13:16.51	41.3	4.1	6.6	12733	< 1.6	...	...	4483
MIPSJ123541.6+621151.0	12:35:41.60 +62:11:51.01	44.7	3.5	6.7	12662	< 4.2	...	...	6771
MIPSJ123541.7+621223.5	12:35:41.73 +62:12:23.54	64.0	5.2	7.0	12853	< 2.4	...	...	6014

Notes. The second and third columns list the prior position from IRAC. Fourth column lists the 24 μm flux density. Fifth and sixth columns give the 24 μm flux uncertainty derived from the residual map and from our Monte-Carlo simulations respectively (see text for detail). Seventh column indicates the integration time on the source. Columns 8 to 11 repeat Cols. 4–7 for 70 μm.

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