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.2:

Observations used for the determination of the zodiacal light emission. The columns are: (1) name of the field; (2), (3) position; (4) wavelength; (5) the ISO identifier number (TDT) of the observation; and (6) time difference between the listed observation and the observation of the EBL raster maps of Table B.1. A time difference is quoted only when the observations were not performed within the same day. Observations at wavelengths below 60 $\mu$ m are made with the ISOPHOT-P detector.
Field	RA	Dec	$\lambda$	AOT	TDT number	$\Delta t$
	(J2000)	(J2000)	( $\mu$ m)			(days)
EBL22	2 26 34.4	-25 53 53	25	PHT05	82101132	+2
			90	PHT25	82101126	+2
			150	PHT25	81901927
			180	PHT25	81901529
EBL26_ZL1¹	1 20 3.0	1 32 30	7.3	PHT05	58600239
			25	PHT05	58600240
			60	PHT25	58600341
			170	PHT25	58600444
EBL26_ZL2	1 19 30.2	1 23 59	3.6	PHT05	58600646
			7.3	PHT05	58600647
			25	PHT05	58600648
			60	PHT25	58600349
			90	PHT25	58600342
			90	PHT25	58600350
			150	PHT25	58600443
			150	PHT25	58600451
			170	PHT25	58600452
			180	PHT25	58600545
			180	PHT25	58600553
NGP_ZL1	13 43 16.3	40 28 47	7.3	PHT05	55800331	-4
			25	PHT05	55800332	-4
			60	PHT25	55800233	-4
			90	PHT25	55800226	-4
			90	PHT25	55800234	-4
			150	PHT25	56200127
			150	PHT25	56200135
			170	PHT25	56200136
			180	PHT25	56300129	+1
			180	PHT25	56300137	+1
NGP_ZL2²	13 43 32.4	40 33 35	7.3	PHT05	55800123	-4
			25	PHT05	55800124	-4
			170	PHT25	56200128

¹ The position is outside the raster maps; ² the position is outside maps other than
the 180 $\mu$ m map consisting of 15 $\times$ 15 rasters (TDT number 21301803).

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