Open Access

Table 1

Observing circumstances.

Date Time Object N EXPTIME rh ro α Skymonitor record
(UT) (s) (au) (au) (°)
2019-10-22 15:27-16:04 Vesta 21 2 2.5 1.6 10.4 https://youtu.be/PaU3ign_sdY
2019-11-08(a) 12:24-17:27 Vesta 145 2, 3,4, 5, 10, 30 2.5 1.6 4.1 https://youtu.be/dg5ejH7fPd8
2019-11-21 12:22-16:37 Vesta 165 2 2.6 1.6 5.7 https://youtu.be/_gHz8hH7eXQ
2019-12-18 13:20-14:57 Vesta 67 2, 3 2.6 1.8 15.6 https://youtu.be/ceSwHR12S-s
2020-01-10 13:18-13:59 Vesta 31 2 2.6 2.0 20.7 https://youtu.be/3Wkn83F4Qzg
2020-02-13 09:04-10:00 Vesta 30 2 2.6 2.5 22.5 https://youtu.be/VzwG5y-18ME

2020-06-21 18:30-19:20 Ceres 18 20 3.0 2.5 18.9 https://youtu.be/Y4H6QNyWcp0
2020-10-02(b) 09:19-10:30 Ceres 20 20 3.0 2.2 13.1 https://youtu.be/muyaqzYcnb4
2020-10-18 08:50-09:59 Ceres 22 20 3.0 2.3 16.5 https://youtu.be/6-SD0WrY1No
2021-09-09(c) 16:15-17:45 Ceres 25 20 2.8 2.5 20.8 https://youtu.be/fUuu9HiQT8M
2021-11-07 12:34-22:40 Ceres 31 5 2.8 1.8 8.6 https://youtu.be/W7xduRk5tSM

Notes. Date: the UT date in YYYY-MM-DD. Time: the starting and ending UT time in HH:mm. N: the total number of obtained polarimetric sets (one set consists of four exposures). EXPTIME: the exposure times used. rh: the heliocentric distance to the target. ro: the observer-centric distance to the target. α: the phase angle. Skymonitor record: the NHAO skymonitor camera record archived on YouTube (also available in Appendix D). (a)Unstable weather (refer to the skymonitor record). (b)Most H-band frames are saturated. (c)All H-band frames are saturated.

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