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Table 3

Summary of VIRTIS-M dataset processed in this work.

N. Observation Cube Start time End time Phase Incidence Emission Δ LST T
name Parameters (UT) (deg) (deg) (deg) (km) (h) (K)

1 I1_00383518966 432, 256, 158 2015-02-25T21:04:00 2015-02-25T21:30:19 53.02 66.94 41.92 81.51 12.23 203
2 I1_00385906923 432, 256, 70 2015-03-25T12:23:18 2015-03-25T12:46:34 73.49 67.08 45.83 88.23 15.20 197
3 I1_00385885107 432, 256, 70 2015-03-25T06:19:42 2015-03-25T06:42:58 74.47 53.03 31.27 94.06 12.43 218
4 I1_00373462192 432, 256, 86 2014-11-01T11:31:03 2014-11-01T11:45:22 103.07 60.11 43.28 32.39 11.04 168
5 I1_00377182711 432, 256, 80 2014-12-14T12:59:43 2014-12-14T13:13:02 91.77 43.41 52.15 19.44 15.44 188
6 I1_00376302211 432, 256, 80 2014-12-04T08:24:43 2014-12-04T08:38:01 91.07 57.34 70.64 23.49 14.81 179
7 I1_00369356914 432, 256, 109 2014-09-14T23:09:43 2014-09-14T23:45:57 66.89 78.22 30.26 28.16 11.03 163
8 I1_00377184571 432, 256, 74 2014-12-14T13:30:43 2014-12-14T13:43:02 92.66 48.30 54.87 19.92 15.59 158

Notes. For each spot, we report the observations offering the best signal-to-noise conditions with the pixel position (sample and line) reported in Table 4. For each pixel, basic information about observation time, geometry conditions, distance between the Rosetta spacecraft and comet surface (Δ), Local Solar Time (LST), and retrieved temperature (T) are given. The integration time is 3 s for all data reported. The cube parameters indicate the size of the acquisition in bands, sample, line dimensions.

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