Determination of the cosmic far-infrared background level with the ISOPHOT instrument

M. Juvela; K. Mattila; D. Lemke; U. Klaas; C. Leinert; Cs. Kiss

doi:10.1051/0004-6361/200811351

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Volume 500 / No 2 (June III 2009)

A&A, 500 2 (2009) 763-768

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Table A.2:

Effective solid angles for the 2 $\times$ 2 pixels of ISOPHOT's C200 array for the 5 filters with central wavelengths $\lambda _{\rm c}$ .
Filter	$\lambda _{\rm c}$	$\Omega^{{\rm C200~pixel}~i}_{\rm eff}$
	( $\mu$ m)	(10^-7 sr)
C_160	170	1.782	1.940	1.895	1.781
C_200	200	1.810	1.996	1.988	1.878
C_180	180	1.792	1.960	1.927	1.815
C_135	150	1.759	1.898	1.825	1.711
C_120	120	1.722	1.843	1.708	1.587

Source LaTeX | All tables | In the text

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