The interface between the stellar wind and interstellar medium around R Cassiopeiae revealed by far-infrared imaging

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Table 1:

Characteristics of the far-IR observations of R Cas with AKARI and *Spitzer*.
Date & time		$\lambda$	$\Delta\lambda$	Pixel scale	Sky coverage	$S_{\nu, {\rm sky}}$	$\sigma _{\rm sky}$	$R_{3\sigma}$	$F_{\nu}$
(UT)	Band	( $\mu$ m)	( $\mu$ m)	(arcsec)	(pixel^-1)	(MJy sr^-1)	(MJy sr^-1)	(arcmin)	(Jy)
AKARI/FIS observations
2007 Jan. 16 10:19	N60	65	22	15	6	8.7	1.2	3.1	121.48 $\pm$ 19.90
	WIDE-S	90	38	15	9	8.6	0.6	3.8	73.42 $\pm$ 10.03
	WIDE-L	140	52	30	15	13.2	1.3	2.0	25.89 $\pm$ 2.09
	N160	160	34	30	10	9.9	1.3	1.8	22.41 $\pm$ 7.47
Spitzer/MIPS observations
2008 Feb. 18 04:02	MIPS70	70	19	4.92	9	10.0	1.1	3.5	...

Source LaTeX | All tables | In the text

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