Table 3:

COBE-DIRBE peak flux densities in the Magellanic Clouds.

	LMC												SMC
Pos.a	1	2	3	4	5	6	7	8	9	10	11	12	1	2	3
Nameb	30 Dor	N 159	Ridge	N 206	-	N 77-94	Bar	N 11	N 44	N 48	N 63	N 57	Wing	NW	SW
Pixel	24, 32	22, 32	19, 33	18, 30	17, 20	22, 19	23, 26	31, 18	27, 27	33, 27	33, 30	29, 30	-	-	-
	Flux densities
(m)	kJy
1.25	0.174	0.228	0.121	0.113	0.031	0.090	0.315	0.053	0.085	0.047	0.064	0.059	0.102	0.177	0.315
2.2	0.154	0.196	0.098	0.088	0.022	0.076	0.251	0.048	0.066	0.040	0.059	0.046	0.077	0.133	0.238
3.5	0.116	0.126	0.056	0.049	0.013	0.049	0.143	0.032	0.043	0.025	0.035	0.030	0.042	0.071	0.128
4.9	0.084	0.077	0.031	0.028	0.008	0.030	0.081	0.019	0.027	0.015	0.018	0.019	0.023	0.040	0.072
12	0.78	0.41	0.106	0.068	0.026	0.128	0.21	0.095	0.140	0.063	0.040	0.081	0.028	0.060	0.091
25	3.16	1.08	0.114	0.095	0.020	0.25	0.35	0.21	0.29	0.099	0.068	0.186	0.066	0.138	0.180
60	24.9	12.9	1.56	1.74	0.307	3.05	6.04	2.63	4.36	1.43	0.99	2.92	1.21	2.74	3.94
100	35.6	22.1	5.26	4.23	1.24	7.21	11.5	6.39	9.04	3.98	2.69	6.33	3.06	6.06	8.51
140	39.0	26.6	7.92	5.48	2.33	9.03	13.1	7.35	11.1	5.07	3.20	7.17	3.62	6.98	9.47
240	19.2	13.8	5.32	3.19	2.04	6.06	6.79	4.68	6.71	3.36	2.30	4.42	2.68	4.1	5.18
	Luminosity (107 )
1-240	15.6	11.4	3.32	2.74	0.90	3.37	7.29	2.44	4.23	1.77	1.57	2.92	3.21	5.68	8.99
12-240	12.9	8.4	1.79	1.35	0.43	2.14	3.78	1.74	3.07	1.14	0.82	2.05	1.52	2.86	4.07
12-100	9.0	5.3	9.02	0.75	0.18	1.23	2.36	1.02	1.83	0.62	0.46	1.22	8.71	1.69	2.44

Notes. ^(a) Position numbers correspond to WMAP position numbers in Table 2, but area covered is not identical.^(b) The objects refer to the most prominent features included in the aperture. These are the giant HII region complex 30 Doradus (1); the very bright HII region complex N159 south of 30 Dor (2); the prominent ridge of radiating dust and molecular gas south of 30 Dor and N159 (3); the bright but isolated HII region complex N206 south of the LMC Bar (4); a very extended HII region complex, containing N77, N79, N83, N87, N90, N93, N94 at the southwestern corner of the LMC (6); the LMC Bar itself (7); the second brightest HII region complex N11 at the northwestern corner of the LMC (8); the third brightest HII region complex N44 north of the Bar (9); the HII region complexes N48, N63, and N57, delineating Shapley Constellation III (10, 11, 12).