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 B.3:

The positions and sizes of the observed fields. Columns are: (1) name of the field; (2), (3) equatorial coordinates of the centre of the field; (4), (5) galactic coordinates; (6), (7) ecliptic coordinates; (8) number of raster points; (9) area in square degrees; and (10) additional remarks. All areas were observed at 90, 150, and 180 $\mu$ m. In NGP(N) an additional square map was observed at 180 $\mu$ m only. Details of the individual measurements are listed in Appendix, in Table B.1.
Field	Ra (2000)	Dec (2000)	l	b	$\lambda$ .	$\beta$	Rasters	Area ( $\square\hbox{$^\circ$ }$ )	Notes
EBL22	02 26 34.5	-25 53 43	215.0	-68.7	23.8	-37.9	32 $\times$ 3	0.19
	02 32 48.0	-25 54 06	215.6	-67.3	25.5	-38.5	31 $\times$ 1	0.07	1D scan into a region of higher cirrus
EBL26	01 18 14.5	01 56 40	136.5	-60.2	18.8	-5.9	32 $\times$ 4	0.27
NGP(N)	13 43 53.0	40 11 35	86.5	73.0	184.2	46.5	32 $\times$ 4	0.27
	13 42 32.2	40 29 12	87.9	73.0	183.6	46.6	15 $\times$ 15	0.56	180 $\mu$ m only
NGP(S)	13 49 43.7	39 07 30	81.3	72.9	186.4	46.1	32 $\times$ 4	0.27

Source LaTeX | All tables | In the text

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