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Table 3

OSIRIS NAC and WAC filter characteristics and Vega observations.

Filter Central λ FWHM T exp Mean count rate +err -err Observations Aperture
nm nm s DN/s % % px

NAC-F15 267.5 53 0.400 2.571e+005 1.07 0.95 6 68
NAC-F16 368.5 33 0.0200.256 1.415e+006 0.59 0.75 30 810*
NAC-F22 648.5 83 0.020 7.172e+006 1.19 0.93 5 911
NAC-F23 535.5 61 0.020 7.265e+006 0.80 0.69 5 1012
NAC-F24 481.0 72 0.020 9.369e+006 0.15 0.30 5 1011
NAC-F27 700.5 21 0.080 1.366e+006 1.29 0.91 5 910
NAC-F28 742.0 62 0.025 3.447e+006 0.27 0.22 5 911
NAC-F32 648.5 83 0.040 7.496e+006 0.41 0.83 5 1314
NAC-F33 535.5 61 0.040 7.581e+006 1.38 1.25 5 1315
NAC-F38 742.0 62 0.060 3.565e+006 1.10 0.61 4 1314
NAC-F41 880.0 62 0.100 9.906e+005 1.76 1.03 5 1011
NAC-F51 804.5 39 0.100 9.895e+005 1.16 0.79 5 910
NAC-F58 790.5 23 1.000 7.631e+004 0.50 0.34 6 910
NAC-F61 929.5 39 0.350 3.223e+005 0.71 1.15 5 1315
NAC-F71 987.0 38 0.800 1.092e+005 1.43 1.50 5 1617
NAC-F82 650.5 81 0.0701.297 1.941e+005 0.58 0.76 32 911*
NAC-F83 535.5 59 0.500 2.033e+005 1.32 0.80 5 89
NAC-F88 742.0 60 0.500 1.752e+005 1.37 1.43 5 910
WAC-F12 627.0 154 0.0100.150 1.169e+006 1.39 1.35 66 811*
WAC-F13 375.0 8 6.000 1.875e+004 1.23 0.85 8 1112
WAC-F14 387.0 4 6.000 1.588e+004 1.21 0.93 9 1012
WAC-F15 571.0 10 1.500 8.142e+004 0.73 0.53 9 911
WAC-F16 589.5 3 3.500 3.030e+004 0.77 0.55 8 910
WAC-F17 630.5 3 3.500 2.029e+004 0.85 0.97 9 79
WAC-F18 611.5 9 0.2331.900 8.288e+004 0.52 1.14 29 810*
WAC-F21 535.5 61 0.200 5.910e+005 0.68 0.28 9 911
WAC-F31 245.5 13 15.000 5.308e+003 0.85 1.27 9 1213
WAC-F41 258.0 4 50.000 1.749e+003 1.05 0.84 8 1214
WAC-F51 295.0 10 25.000 3.060e+003 2.79 1.79 6 1213
WAC-F61 308.5 3 60.000 1.273e+003 1.77 1.85 8 1113
WAC-F71 325.5 9 20.000 4.376e+003 1.11 1.36 9 1213
WAC-F81 335.0 4 80.000 1.422e+003 0.86 0.69 8 1112

Notes. This table refers to the observations of Vega during different mission phases, from the Mars swing-by in 2007 to the Lutetia fly-by in 2010. For each filter we report the central wavelength of the whole instrumental and filter passband in nm; the FWHM of each instrumental and filter passband in nm; the exposure time needed for the Vega observation, and for the four investigated filters, the linearity interval in seconds; the average count rate in DN s-1 for Vega observations; the positive and negative maximum deviation (expressed in %) with respect to the mean value; the total number of observations; the typical values of the apertures among all observations;

(*)

for each of the four additional filters, this refers only to observations performed with a single particular exposure time within the interval specified in the fourth column.

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