Table 2:

WMAP peak flux densities in the Magellanic Clouds.

	LMC								SMC
Posa	1+2+3	4	6	7	8	9	10	12	1	2	3
Nameb	30 Dorc	N 206	N 77-94	Bar	N 11	N 44	N 48	N 57	Wing	NE	SW
	Flux densities
(GHz)	Jy
23	55 (72)	3.3	6.4	5.2	6.6	4.1	3.2	4.8	2.5	7	7
31	57 (72)	3.6	6.6	5.2	7.5	4.5	2.9	5.1	3	9	8
41	57 (71)	4.2	6.9	5.5	7.9	4.9	2.8	5.3	4	10	10
61	58 (74)	6.7	8.7	6.5	10.5	6.8	2.8	6.7	8	16	16
93	101 (198)	13.1	19.1	10.5	19.3	13.3	4.0	11.5	19	34	35

Notes. ^a Position numbers correspond to DIRBE position numbers in Table 3, but area covered is not identical. ^b Object identifies the most prominent feature within the aperture, usually an HII region complex. ^c Numbers in the first column are flux densities with local background level subtracted; numbers in the second column, between parentheses, are flux densities as measured by integrating over the aperture without background subtraction.