The evolution of the dust temperatures of galaxies in the SFR–M∗ plane up to z ~ 2

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Table 1

Main properties of the PEP/HerMES fields used in this study.

		100 μm		160 μm		250 μm		350 μm		500 μm

Field		Eff. area	3σ	Eff. area	3σ^a	Eff. area	3σ^a	Eff. area	3σ^a	Eff. area	3σ^a
		arcmin²	mJy	arcmin²	mJy	arcmin²	mJy	arcmin²	mJy	arcmin²	mJy

GOODS-S	03^h32^m, − 27°48′	200	1.2	200	2.4	400	7.8	400	9.5	400	12.1
GOODS-N	12^h36^m, + 62°14′	200	3.0	200	5.7	900	9.2	900	12	900	12.1
COSMOS	00^h00^m, + 02°12′	7344	5.0	7344	10.2	7225	8.1	7225	10.7	7225	15.4

Notes.

^(a)

In the deep 160, 250, 350 and 500 μm observations, rms values include confusion noise.

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