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Table 2

Selected observations of Dione by CIRS FP1 within the ROI.

# Name Start UTC Stop UTC Npo lt FOV extent D
CIRS_revDI_name (°) min-max (°) (au)
1 016DI_TARGFLYBY001 2005-284T15:45:36 2005-284T17:42:36 117 138 ± 3 2–8 9.09
2 050DI_FP1AMATA001 2007-273T03:00:00 2007-273T03:20:00 98 275 ± 12 27–33 9.24
3 050DI_VIMSRIDER001 2007-273T03:50:00 2007-273T04:50:00 699 288 ± 8 19–23 9.24
4 137DI_DIONE001 2010-246T07:13:00 2010-246T10:40:00 406 122 ± 12 15–31 9.55
5 165DI_DIONE001 2012-123T20:02:00 2012-124T00:11:00 68 111 ± 3 15–36 9.72
6 214DI_FP3SCAN001 2015-101T22:00:00 2015-101T23:00:00 149 198 ± 1 46–58 9.97
7 214DI_REGMAP001 2015-101T23:00:00 2015-102T00:00:00 37 189 ± 2 45–61 9.97
8 219DI_DIONE001 2015-207T22:00:00 2015-207T22:40:00 76 99 ± 8 29–44 9.99
9 219DI_DIONE002 2015-207T22:40:00 2015-208T00:00:00 271 111 ± 8 26–33 9.99
10 219DI_DIONE003 2015-208T00:00:00 2015-208T00:40:00 50 87 ± 9 25–29 9.99
11 219DI_DIONE004_PIE 2015-208T00:40:00 2015-208T02:20:00 9 92 ± 8 25–31 9.99

Notes. Npo is the number of spectra (pointings) that are located in the ROI (Fig. 1). It is the average local time at the centre of the FOVs during the observation. Local time is 0° at midnight. The spectral resolution is 15.5 cm−1, except for observation #1, which has a resolution of 2.85 cm−1. The FOV extent provides the minimum and maximum latitudinal widths of the FP1 footprints. D is the heliocentric distance expressed in astronomical units.

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