The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds

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Volume 655 (November 2021)

A&A, 655 (2021) A98

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Table 7.

Flux densities from the stacked data.

Filter	λ_eff	LBVs	LBVs	x-AGBs
			(w/o RMC143)
	(μm)	(Jy)	(Jy)	(Jy)
J^(a)	1.235	3.430 ± 0.068	3.330 ± 0.066	5.951 ± 0.595
H^(a)	1.662	2.761 ± 0.070	2.680 ± 0.068	16.128 ± 1.613
K_s ^(a)	2.159	2.430 ± 0.050	2.370 ± 0.050	32.604 ± 3.260
IRAC3.6 ^(a)	3.550	0.776 ± 0.024	0.735 ± 0.023	83.965 ± 8.397
IRAC4.5 ^(a)	4.493	0.604 ± 0.017	0.574 ± 0.016	93.59 ± 9.36
IRAC5.8 ^(a)	5.731	0.470 ± 0.013	0.447 ± 0.012	104.07 ± 10.42
IRAC8.0 ^(a)	7.872	0.541 ± 0.018	0.500 ± 0.020	104.18 ± 10.42
WISE3 ^(a)	11.56	0.996 ± 0.082	0.795 ± 0.080	–
MIPS24 ^(b)	23.675	12.4 ± 1.7	11.7 ± 1.5	44.95 ± 4.64
MIPS70 ^(b)	71.42	4.3 ± 2.6	4.1 ± 0.8	7.2 ± 1.6
PACS100 ^(b)	100.0	2.34 ± 0.31	1.66 ± 0.220	4.1 ± 1.4
PACS160 ^(b)	160.0	0.82 ± 0.40	>0.41 ± 0.16 ^(c)	<4.26 ^(d)
SPIRE250 ^(b)	250.0	>0.122 ± 0.037 ^(c)	–	–

Notes.

^(a)

Summed photometry from catalogues.

^(b)

Photometry of point-source at the centre of stacked images.

^(c)

Lower limit fluxes are measured fluxes from stacks of subsets of the least confused or brightest sources (see text).

^(d)

3σ statistical upper limit from the noise in the stacked image.

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