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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

$\nu$
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.


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