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Table 1

Observing conditions of the Wosret region for the NAC images.

Day UT Δ α res Slope Filters
(km) (°) (m px−1) %/(100 nm)
21/02/2015 12h52 69.5 44.3 1.31 15.31 ± 1.62 F22, F24, F41
25/03/2015 02h37 99.1 77.6 1.87 16.20 ± 1.92 F22, F23, F24, F41
13/04/2015 05h59 151.8 79.2 2.86 15.87 ± 1.42 F22, F24, F41
02/05/2015 10h42 123.9 61.2 2.32 15.49 ± 1.50 all
02/05/2015 11h42 123.9 61.1 2.32 15.44 ± 1.57 all
22/05/2015 15h34 129.0 61.1 2.43 15.37 ± 1.60 all
26/07/2015 15h10 166.9 90.1 3.14 16.78 ± 1.49 all
01/08/2015 07h38 215.2 90.0 4.05 16.70 ± 2.16 all
01/08/2015 13h51 211.5 89.8 3.98 16.33 ± 2.11 all
01/08/2015 18h13 209.6 89.8 3.95 16.48 ± 2.65 all
22/08/2015 22h16 329.7 88.7 6.20 15.90 ± 1.30 all
23/08/2015 10h19 333.3 87.8 6.27 15.64 ± 1.62 all
30/08/2015 08h09 404.7 70.3 7.62 14.94 ± 1.13 all
30/08/2015 12h21 404.2 70.2 7.61 15.29 ± 0.94 all
30/08/2015 18h13 402.7 70.2 7.58 14.92 ± 1.15 all
31/08/2015 00h34 403.1 70.2 7.59 15.34 ± 0.92 all
11/10/2015 18h53 524.7 61.2 9.88 14.89 ± 0.80 all
20/10/2015 00h02 420.9 64.4 7.92 14.99 ± 0.86 all
31/10/2015 12h46 302.0 62.8 5.68 15.32 ± 0.92 all
31/10/2015 16h07 297.2 62.4 5.59 15.29 ± 0.60 all
31/10/2015 19h07 293.3 62.1 5.52 15.36 ± 0.76 all
31/10/2015 22h49 288.4 61.7 5.43 15.25 ± 0.85 all
19/11/2015 20h06 125.9 78.2 2.37 16.10 ± 0.88 F22, F24, F41
20/11/2015 05h16 130.0 82.3 2.45 15.78 ± 1.90 F22, F24, F41
22/11/2015 11h41 128.6 89.6 2.41 16.58 ± 1.24 F22, F24, F41
22/11/2015 19h51 126.5 89.5 2.38 17.29 ± 0.64 F22, F24, F41
23/11/2015 00h13 125.7 89.5 2.37 16.65 ± 1.06 F22, F24, F41
28/11/2015 19h04 125.0 90.4 2.35 17.31 ± 1.70 all
07/12/2015 01h13 97.9 89.7 1.84 17.07 ± 1.18 F22, F24, F41
10/12/2015 01h31 101.6 89.8 1.91 17.11 ± 1.48 F22, F24, F41
12/12/2015 23h51 99.8 89.9 1.87 16.84 ± 1.46 all
17/12/2015 22h56 93.4 90.4 1.75 16.59 ± 2.74 F22, F24, F41
17/12/2015 23h56 94.0 90.4 1.76 16.90 ± 1.82 F22, F24, F41
18/12/2015 11h09 95.1 90.5 1.78 16.76 ± 2.74 F22, F24, F41
18/12/2015 12h09 96.0 90.5 1.80 17.01 ± 2.48 F22, F24, F41
09/01/2016 15h05 76.5 90.5 1.44 19.14 ± 2.36 all
23/01/2016 17h03 74.2 62.4 1.40 16.66 ± 2.13 F22, F24, F41
27/01/2016 18h20 69.0 62.8 1.30 16.49 ± 1.63 F22, F23, F24, F27, F28, F41, F71, F61, F16
27/01/2016 21h22 68.1 62.7 1.28 16.58 ± 1.01 F22, F23, F24, F27, F28, F41, F71, F61, F16
10/02/2016 19h20 46.9 65.2 0.88 17.52 ± 2.39 all
10/02/2016 08h06 48.9 66.3 0.91 17.68 ± 1.85 all
10/02/2016 07h06 49.0 66.5 0.92 17.34 ± 2.17 all
09/04/2016 17h33 32.7 40.8 0.62 16.20 ± 1.32 all
16/05/2016 22h23 7.8 101.6 0.15 18.68 ± 4.79 F22, F23, F24, F16, F41
28/05/2016 12h26 4.9 101.0 0.09 19.76 ± 3.15 F22, F23, F24, F16, F41
12/06/2016 22h28 27.5 81.4 0.52 18.13 ± 2.09 F22, F24, F41
13/06/2016 11h31 27.6 69.6 0.52 17.52 ± 2.10 F22, F24, F41
13/06/2016 23h15 27.0 61.1 0.51 17.32 ± 2.15 F22, F24, F41
14/06/2016 10h29 26.7 54.0 0.50 17.17 ± 2.07 F22, F24, F41
25/06/2016 12h16 16.1 91.4 0.30 18.28 ± 1.56 F22, F23, F24, F16, F41
25/06/2016 13h31 15.9 93.5 0.30 18.64 ± 1.51 F22, F23, F24, F16, F41
02/07/2016 15h22 14.3 92.6 0.27 18.99 ± 1.90 F22, F23, F24, F16, F41
03/07/2016 12h43 7.1 102.1 0.13 18.86 ± 2.32 F22, F24, F41
03/07/2016 13h03 3.0 102.3 0.06 18.80 ± 3.20 F22, F24, F41
09/07/2016 15h33 12.1 99.0 0.23 19.04 ± 2.69 F22, F23, F24, F16, F41, F27, F71
09/07/2016 16h03 12.0 98.5 0.22 19.11 ± 2.59 F22, F23, F24, F16, F41, F27, F71
09/07/2016 16h33 11.9 97.8 0.22 19.00 ± 2.94 F22, F23, F24, F16, F41, F27, F71
16/07/2016 16h39 9.3 105.7 0.17 18.43 ± 3.11 F22, F23, F24, F16, F41, F27, F71
24/08/2016 18h17 3.9 91.5 0.07 18.52 ± 3.06 F22, F24, F41

Notes. α is the phase angle, Δ is the distance between comet and spacecraft, and “res” the spatial resolution. The time refers to the start time of the first image of an observing sequence. Filters: F22 (649.2 nm, reference), F23 (535.7 nm), F24 (480.7 nm), F16 (360.0 nm), F27 (701.2 nm), F28 (743.7 nm), F41 (882.1 nm), F51 (805.3 nm), F61 (931.9 nm), F71 (989.3 nm), and F15 (269.3 nm). The spectral slope was evaluated in the 535–882 nm range after normalization at 535 nm using the F23 filter image when present, and otherwise an artificial 535 nm image was created from the interpolation of the observations acquired at 480 nm and 649 nm.

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