Millimeter and submillimeter excess emission in M 33 revealed by Planck and LABOCA

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Table 1

Summary of the observations used in this study.

Telescope	Instrument	λ ₀	ν ₀	FWHM	Δ_CAL	Band name	References
	or filter	μm	GHz		%

GALEX	FUV	0.154	1 946 704		10	GALEX FUV	Thilker et al. (2005)
	NUV	0.232	1 292 209		10	GALEX NUV	Thilker et al. (2005)

Sloan	u	0.355	844 486		2	Sloan u-band	This paper.
	g	0.469	639 216		1	Sloan g-band	This paper.

KPNO	Hα	0.657	456 305		15	Hα	Greenawalt (1998)

Spitzer	IRAC	3.55	84 449		2	IRAC 3.6 μm	Verley et al. (2007)
	IRAC	4.49	66 769		2	IRAC 4.5 μm	Verley et al. (2007)
	MIPS	23.7	12 650		4	MIPS 24 μm	This paper.

Herschel	PACS	70.0	4 283		10	PACS 70 μm	Boquien et al. (2015)
	PACS	100	2 998		10	PACS 100 μm	Boquien et al. (2011)
	PACS	160	1 874		20	PACS 160 μm	Boquien et al. (2011)
	SPIRE	250	1 199		5	SPIRE 250 μm	Xilouris et al. (2012)
	SPIRE	363	826		5	SPIRE 350 μm	Xilouris et al. (2012)
	SPIRE	517	580		5	SPIRE 500 μm	Xilouris et al. (2012)

APEX	LABOCA	870	345		10	LABOCA 870 μm	Albrecht et al. (in prep.)

Planck	HFI	350	857		10	PLANCK 350 μm	This paper.
	HFI	550	545		10	PLANCK 550 μm	This paper.
	HFI	850	353		3	PLANCK 850 μm	This paper.
	HFI	1 380	217		3	PLANCK 1.4 mm	This paper.
	HFI	2 096	143		3	PLANCK 2.1 mm	This paper.
	HFI	3 000	100		3	PLANCK 3.0 mm	This paper.
	LFI	10 000	30		3	PLANCK 10 mm	This paper.

Effelsberg	S 36 mm	35 903	8.35		^*	S 36 mm	Tabatabaei et al. (2007b)

Notes.

^(*)

Only the total error is reported in Tabatabaei et al. (2007b).

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