Table 1

Major gaps and events affecting the astrometric solution.

tbeg tend Length Description
1220.400 1225.200 4.800 VPU reset
1316.490 1389.113 72.623 Decontamination #4
1443.800 1444.200 0.400 Refocus (following FoV)
1653.800 1660.000 6.200 PAA anomaly
1820.900 1830.000 9.100 PAA anomaly
2094.000 2099.000 5.000 PDHU anomaly
2179.125 2191.000 11.875 VPU software update
2192.252 2195.218 2.967 Observation gap
2238.000 2242.000 4.000 Unknown
2322.300 2401.559 79.259 Decontamination #5
2405.967 2408.643 2.676 Observation gap
2408.935 2409.968 1.033 Observation gap
2574.640 2575.400 0.760 Refocus (preceding FoV)
2954.200 2958.000 3.800 Moon eclipse
3045.133 3049.000 3.867 PDHU anomaly
3603.250 3605.227 1.976 Observation gap
3646.800 3650.000 3.200 Moon eclipse
3663.700 3667.000 3.300 Moon eclipse
4074.210 4076.063 1.853 Observation gap
4112.463 4180.000 67.537 Decontamination #6
4271.753 4275.200 3.445 PAA anomaly
4477.441 4481.000 3.550 PAA anomaly
4512.502 4515.000 2.498 PAA anomaly
4545.144 4548.000 2.856 PAA anomaly
5078.547 5080.600 2.053 STR anomaly

Notes. The table lists gaps longer than 1 revolution (0.25 day) and some other events of relevance for the calibration model. tbeg and tend are the start and end times of the gap in OBMT revolutions (see Eq. (1)). The third column is the length of the gap in revolutions. Abbreviations: VPU = video processing unit, FoV = field of view, PAA = phased array antenna, PDHU = payload data handling unit, STR = star tracker.

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