The AKARI FU-HYU galaxy evolution program: first results from the GOODS-N field

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Table 1:

Photometric filter band definitions for the three cameras of the IRC.
Camera	Array Area^*	Pixel scale	Band	$\lambda_{\rm ref}$	$\Delta \lambda$
	(pixels)	(arcsec)		( $\mu$ m)	( $\mu$ m)
NIR	319 $\times$ 412	1.46 $\times$ 1.46	N2	2.4	1.9-2.8
			N3	3.2	2.7-3.8
			N4	4.1	3.6-5.3
MIR-S	233 $\times$ 256	2.34 $\times$ 2.34	S7	7.0	5.9-8.4
			S9W	9.0	6.7-11.6
			S11	11.0	8.5-13.1
MIR-L	246 $\times$ 239	2.51 $\times$ 2.39	L15	15.0	12.6-19.4
			L18W	18.0	13.9-25.6
			L24	24.0	20.3-26.5

Notes. ^(*) This is the effective imaging area of the array.

Source LaTeX | All tables | In the text

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