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Table A.3
Ingress and egress times derived from the Huya occultation light curves.
#chord | Observatory, Country | Ingress (UT) | Egress (UT) | Chord size (km) |
---|---|---|---|---|
1 | TUBITAK National Observatory-1, Turkey | 00:52:34.387±2.592 | 00:53:00.703±0.142 | 212.4±22.1 |
2 | TUBITAK National Observatory-2, Turkey | 00:52:30.407±5.500 | 00:52:52.439±5.500 | 177.8±88.8 |
3 | Romanian Acad., Astron. Obs. Cluj, Feleacu Sta., Romania | 00:53:51.515±0.115 | 00:54:37.293±0.089 | 369.4±1.7 |
4 | ROASTERR-1 Observatory, Romania | No data | 00:54:38.748±0.030 | — |
5 | W-FAST-Wise Observatory, Israel | 00:51:21.416±0.016 | 00:52:07.918±0.023 | 375.3±0.3 |
6 | C18 at Wise Observatory, Israel | 00:51:21.110±0.040 | 00:52:07.851±0.040 | 377.2±0.7 |
7 | Astronomical Inst. Romanian Academy-1, Romania | 00:53:30.014±0.998 | 00:54:18.863±0.098 | 394.2±8.8 |
8 | Astronomical Inst. Romanian Academy-2, Romania | 00:53:31.111±0.041 | 00:54:18.814±0.041 | 385.0±0.7 |
9 | ISTEK Belde Observatory, Turkey | 00:52:59.908±0.062 | 00:53:50.451±0.083 | 407.9±1.2 |
10 | Amateur Observatory-1, Romania | 00:53:33.562±0.444 | 00:54:23.630±0.174 | 404.1±5.0 |
11 | St. George Observatory, Romania | 00:53:34.446±0.083 | 00:54:24.868±0.077 | 406.9±1.3 |
12 | Amateur Observatory-2, Romania | 00:53:30.484±0.020 | 00:54:21.217±0.200 | 409.4±1.8 |
13 | Stardust Observatory, Romania | 00:53:38.100±0.150 | 00:54:29.800±1.850 | 417.2±16.1 |
14 | Stardreams Observatory, Romania | 00:53:37.111±0.098 | 00:54:29.122±0.099 | 419.7±1.6 |
15 | Martin S. Kraar Obs., Israel | 00:51:30.046±0.100 | 00:52:23.578±1.148 | 432.0±10.1 |
* | Amateur Observatory-3, Romania | 00:00:00.000±0.007 | 00:00:43.218±0.007 | 348.8±0.1 |
16 | Amateur Observatory-4, Romania | 00:53:33.840±0.027 | 00:54:25.060±0.027 | 413.4±0.4 |
17 | Bacau Observatory, Romania | 00:53:46.520±3.400 | 00:54:33.919±0.083 | 382.5±28.1 |
18 | Galati Observatory-1 and 2, Romania | 00:53:40.500±0.440 | 00:54:25.420±0.440 | 362.5±7.1 |
19 | Barlad Observatory, Romania | 00:53:51.192±0.047 | 00:54:31.753±0.073 | 327.3±1.0 |
Sites are sorted by their distance to the center of the predicted shadow path, from west to east. The chord marked with * was not used in the final analysis of the occultation (see Section 3).
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