The far-infrared/radio correlation and radio spectral index of galaxies in the SFR–M∗ plane up to z~2

B. Magnelli; R. J. Ivison; D. Lutz; I. Valtchanov; D. Farrah; S. Berta; F. Bertoldi; J. Bock; A. Cooray; E. Ibar; A. Karim; E. Le Floc’h; R. Nordon; S. J. Oliver; M. Page; P. Popesso; F. Pozzi; D. Rigopoulou; L. Riguccini; G. Rodighiero; D. Rosario; I. Roseboom; L. Wang; S. Wuyts

doi:10.1051/0004-6361/201424937

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Volume 573 (January 2015)

A&A, 573 (2015) A45

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Table 1

Main properties of the PEP/GOODS-H/HerMES observations used in this study.

		PACS			SPIRE

Field		Eff. area	100 μm 3σ^a	160 μm 3σ^a	Eff. area	250 μm 3σ^a	350 μm 3σ^a	500 μm 3σ^a
		arcmin²	mJy	mJy	arcmin²	mJy	mJy	mJy

GOODS-S^b	03^h32^m, −27°48′	200 (100)	1.0 (0.6)	2.1 (1.3)	400	7.8	9.5	12.1
ECDFS	03^h32^m, −27°48′	900	4.4	8.3	900	7.8	9.1	11.9
GOODS-N	12^h36^m, + 62°14′	200	1.0	2.1	900	9.2	12	12.1
COSMOS	00^h00^m, + 02°12′	7344	5.0	10.2	7225	8.1	10.7	15.4

Notes.

^(a)

rms values include confusion noise.

^(b)

Values in parentheses correspond to the PACS ultradeep part of the GOODS-S field, as obtained by combining GOODS-H and PEP observations (Magnelli et al. 2013).

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