Large-scale distributions of mid- and far-infrared emission from the center to the halo of M 82 revealed with AKARI

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Volume 514 (May 2010)

A&A, 514 (2010) A14

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Table 2:

Flux densities of M 82.
Band	Center ( $d\leq 1'$ )	Center ( $d\leq 2'$ )	Center ( $d\leq 4'$ )^a	Total ( $d\leq 8'$ )	Total ( $d\leq$ 12 $.\mkern -4mu^\prime$ 5)	Halo ( $d\leq 4'$ )^a
	(Jy)	(Jy)	(Jy)	(Jy)	(Jy )	(Jy)
IRC S7 7 $\mu$ m	54.1 $\pm$ 1.2^b	64.2 $\pm$ 1.5	72.7 $\pm$ 1.7	75.3 $\pm$ 1.7	...	0.045 $\pm$ 0.001
IRC S11 11 $\mu$ m	43.7 $\pm$ 1.0	53.8 $\pm$ 1.3	62.8 $\pm$ 1.5	65.5 $\pm$ 1.5	...	0.048 $\pm$ 0.001
IRC L15 15 $\mu$ m	112.0 $\pm$ 3.2	128.0 $\pm$ 3.6	137.0 $\pm$ 3.9	140.8 $\pm$ 4.0	...	0.091 $\pm$ 0.002
IRC L24 24 $\mu$ m	307 $\pm$ 14	342 $\pm$ 16	361 $\pm$ 17	365 $\pm$ 17	...	0.21 $\pm$ 0.01
FIS N60 65 $\mu$ m	...	630 $\pm$ 130	1530 $\pm$ 310	1700 $\pm$ 340	1920 $\pm$ 380	16.4 $\pm$ 3.3
FIS WIDE-S 90 $\mu$ m	...	529 $\pm$ 110	1550 $\pm$ 310	1840 $\pm$ 370	2040 $\pm$ 410	16.0 $\pm$ 3.2
FIS WIDE-L 140 $\mu$ m	...	520 $\pm$ 160	1580 $\pm$ 480	2000 $\pm$ 600	2250 $\pm$ 670	26.2 $\pm$ 7.9
FIS N160 160 $\mu$ m	...	360 $\pm$ 110	1270 $\pm$ 380	1580 $\pm$ 470	1940 $\pm$ 580	47 $\pm$ 14

Notes. ^(a) The sizes and positions of the aperture regions are indicated by the dashed circles in Figs. 2a and 3d.
^(b) The flux density errors include both systematic effects associated with the detectors and absolute calibration uncertainties (Lorente et al. 2007; Verdugo et al. 2007).

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