Table 2: Log of observations of NGC 6791 from three campaigns. The columns contain the adopted abbreviation of the campaign, the name of the telescope, the duration of the campaign, the number of useful nights (n), the median seeing in the V filter, and the number of images obtained in each of the BVRI filters. The last column gives information on which reduction technique we have used. Note that we have not reduced the MOCH01 data set, but we have obtained the light curves of the variable stars published by Mochejska et al. (2002).
Number of images Reduction

Campaign Telescope Dates UT n [''] N_B N_V N_R N_I Method

NOT01 2.5 m NOT 9/7-17/7 01 7 1 $.\!\!^{\prime\prime}$ 0 58 264 - 444 ALLFRAME/ ISIS

MOCH01 1.2 m FLWO 6/7-1/8 01 18 2 $.\!\!^{\prime\prime}$ 1 - 36 204 - Not Reduced

SMR95 1.0 m JKT 11/7-24/7 95 14 1 $.\!\!^{\prime\prime}$ 6 - 601 - 153 ALLFRAME

**Table 2:** Log of observations of NGC 6791 from three campaigns. The columns contain the adopted abbreviation of the campaign, the name of the telescope, the duration of the campaign, the number of useful nights (n), the median seeing in the V filter, and the number of images obtained in each of the *BVRI* filters. The last column gives information on which reduction technique we have used. Note that we have not reduced the *MOCH01* data set, but we have obtained the light curves of the variable stars published by Mochejska et al. (2002).
					Number of images	Reduction
Campaign	Telescope	Dates UT	n	['']	N_B	N_V	N_R	N_I	Method
NOT01	2.5 m NOT	9/7-17/7 01	7	1 $.\!\!^{\prime\prime}$ 0	58	264	-	444	ALLFRAME/ ISIS
MOCH01	1.2 m FLWO	6/7-1/8 01	18	2 $.\!\!^{\prime\prime}$ 1	-	36	204	-	Not Reduced
SMR95	1.0 m JKT	11/7-24/7 95	14	1 $.\!\!^{\prime\prime}$ 6	-	601	-	153	ALLFRAME

Source LaTeX | All tables | In the text