DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands

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Volume 609 (January 2018)

A&A, 609 (2018) A37

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Table 1

Details of each band for which we have data.

Facility	Effective	Band	Imagery	Photometry	Pixel	Resolution	Calibration
	wavelength	name	present	present	width	FWHM	uncertainty

					(′′)	(′′)	(%)

GALEX	153 nm	FUV	797	794	3.2	4.3	4.5	}a
GALEX	227 nm	NUV	832	830	3.2	5.3	2.7	}a
SDSS	353 nm	u	655	655	0.45	1.3	1.3	}b
SDSS	475 nm	g	655	655	0.45	1.3	0.8
SDSS	622 nm	r	655	655	0.45	1.3	0.8
SDSS	763 nm	i	655	655	0.45	1.3	0.7
SDSS	905 nm	z	655	655	0.45	1.3	0.8
DSS1	450 nm	B	794	–	1–1.7	1.9 (1.5–3.0)	–
DSS1	660 nm	R	794	–	1–1.7	1.9 (1.5–3.0)	–
DSS2	450 nm	B	861	–	1–1.7	1.9 (1.5–3.0)	–
DSS2	660 nm	R	861	–	1–1.7	1.9 (1.5–3.0)	–
2MASS	1.24 μm	J	875	875	1	2.0	1.7	}c
2MASS	1.66 μm	H	875	875	1	2.0	1.9
2MASS	2.16 μm	K _S	875	875	1	2.0	1.9
WISE	3.4 μm	(W1)	875	875	1.375	6.1	2.9	}d
WISE	4.6 μm	(W2)	875	875	1.375	6.4	3.4
WISE	12 μm	(W3)	875	875	1.375	6.5	4.6
WISE	22 μm	(W4)	875	875	1.375	12	5.6
Spitzer	3.6 μm	(IRAC-1)	644	623	0.75	1.66	3	}e
Spitzer	4.5 μm	(IRAC-2)	804	777	0.75	1.72	3
Spitzer	5.8 μm	(IRAC-3)	392	374	0.6	1.88	3
Spitzer	8.0 μm	(IRAC-4)	411	392	0.6	1.98	3
Spitzer	24 μm	(MIPS-1)	491	477	2.4–2.6	6	5	}f
Spitzer	70 μm	(MIPS-2)	198	177	4	18	10
Spitzer	160 μm	(MIPS-3)	184	171	8	38	12
PACS	70 μm	–	255	244	2	9 (5.8–12.2)	7	}g
PACS	100 μm	–	716	701	3	10 (6.9–12.7)	7
PACS	160 μm	–	771	753	4	13 (12.1–15.7)	7
SPIRE	250 μm	(PSW)	844	844	6	18	5.5	}h
SPIRE	350 μm	(PMW)	844	844	8	25	5.5
SPIRE	500 μm	(PLW)	844	844	12	36	5.5

Planck	350 μm	(857 GHz)	875	394	102.1	278	6.4	}i
Planck	550 μm	(545 GHz)	875	279	102.1	290	6.1
Planck	850 μm	(353 GHz)	875	197	102.1	296	0.78
Planck	1.38 mm	(217 GHz)	875	97	102.1	301	0.16
Planck	2.10 mm	(143 GHz)	875	29	102.1	438	0.07
Planck	3.00 mm	(100 GHz)	875	19	205.7	581	0.09
Planck	4.26 mm	(70 GHz)	875	11	205.7	799	0.20	}j
Planck	6.81 mm	(44 GHz)	875	18	205.7	1630	0.26
Planck	10.60 mm	(30 GHz)	875	35	205.7	1940	0.35

IRAS	12 μm	–	–	598	–	270	20	}k
IRAS	25 μm	–	–	578	–	276	20
IRAS	60 μm	–	–	675	–	282	20
IRAS	100 μm	–	–	682	–	300	20

Notes. For FUV-K_S bands, we refer to each band by its listed “Band name”; otherwise we refer to bands by wavelength. The “Imagery present” and “Photometry present” columns give the number of galaxies in each band for which we present imagery and photometry (there are some targets for which we present imagery, but where photometry was not possible; see Sect. 3.6). For supplementary photometry, we give the number of galaxies in each band for which photometry was available from IRAS SCANPI and Planck CCS2 (see Sect. 5). References for calibration uncertainties are provided below. For bands with significantly varying resolutions, a typical value is given, followed by the full range in parentheses.

Reference.

^(a)

Morrissey et al. (2007);

^(b)

SDSS DR12 Data Release Supplement: https://www.sdss3.org/dr12/scope.php;

^(c)

Cohen et al. (2003);

^(d)

WISE All-Sky Release Explanatory Supplement: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec4_4h.html;

^(e)

IRAC Instrument Handbook https://irsa.ipac.caltech.edu/data/SPITZER/docs/irac/iracinstrumenthandbook/17/#_Toc410728305;

^(f)

MIPS Instrument Handbook: https://irsa.ipac.caltech.edu/data/SPITZER/docs/mips/mipsinstrumenthandbook/42/#_Toc288032317;

^(g)

PACS Instrument & Calibration Wiki: http://herschel.esac.esa.int/twiki/bin/view/Public/PacsCalibrationWeb;

^(h)

SPIRE Instrument & Calibration Wiki: http://herschel.esac.esa.int/twiki/bin/view/Public/SpireCalibrationWeb;

⁽ⁱ⁾

Planck Collaboration VII (2016);

^(j)

Planck Collaboration V (2016);

^(k)

Sanders et al. (2003), Miville-Deschênes et al. (2005).

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