Planck intermediate results - XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations

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Volume 586 (February 2016)

A&A, 586 (2016) A132

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Table 1

Description of the data used.

Band	λ ^a	FWHM ^b	Calibration	CIB	Removed CIB	Removed
			uncertainty^c	anisotropies^d	monopole	offset
	[μm]	[arcmin]	[ % ]	[MJy sr^-1]	[MJy sr^-1]	[MJy sr^-1]

Planck 100 GHz^e	3000	9.68	0.09		0.0030	−0.000240
Planck 143 GHz^e	2098	7.30	0.07		0.0079	0.000694
Planck 217 GHz^e	1283	5.02	0.16		0.033	−0.0032
Planck 353 GHz	850	4.94	0.78	0.016	0.13	−0.007616
Planck 545 GHz	550	4.83	6.1	0.044	0.35	0.0004581
Planck 857 GHz	350	4.64	6.4	0.010	0.64	−0.04284
DIRBE 240 μm	248	42.0	11.6			0.975961
DIRBE 140 μm	148	42.0	10.6			1.16576
DIRBE 100 μm	100	42.0	13.6			0.87963
IRAS 100 μm	100	4.3	13.5	0.010		−0.06381
IRAS 60 μm	60	4.0	10.4			0.112
WISE 12 μm	12	0.25	10.0			0.0063

Notes.

^(a)

Central wavelength of the spectral band.

^(b)

Angular resolution (FWHM) of the original map.

^(c)

Assumed calibration uncertainty as a percentage of the image intensity.

^(d)

Root mean square (rms) of the CIB anisotropies in the band at 5′ resolution.

^(e)

Planck 217, Planck 143, Planck 100 and DIRBE bands are not used to constraint the current dust model.

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