Open Access

Table 2.

Our observations of HD 63433.

Date UT HJD ncyc Instrument texp S/N σLSD
[dd-mm-yyyy] [hh:mm:ss] [−2 450 000] [s] [10−5Ic]
12-09-2022 15:01:01.380 9835.12079 −27.17 ESPaDOnS 4 × 340 743 4.83
23-12-2022 05:32:01.248 9936.73575 −11.42 HARPSpol 4 × 900 394 13.70
25-12-2022 05:23:12.480 9938.72971 −11.11 HARPSpol 4 × 900 327 201.53
06-02-2023 04:22:00.480 9981.68718 −4.45 HARPSpol 4 × 900 245 11.42
06-03-2023 20:55:29.485 10 010.37541 0.00 Neo-Narval 4 × 900 520 9.60
07-04-2023 19:46:09.397 10 042.32441 4.95 Neo-Narval 4 × 900 556 11.70
08-04-2023 20:17:03.480 10 043.34576 5.11 Neo-Narval 4 × 900 465 8.71
16-04-2023 19:25:34.170 10 051.30923 6.35 Neo-Narval 4 × 900 494 9.83
02-05-2023 19:49:12.432 10 067.32409 8.83 Neo-Narval 4 × 900 381 13.60
05-05-2023 20:45:55.940 10 070.36319 9.30 Neo-Narval 4 × 900 417 9.44

Notes. The following quantities are listed: (1) and (2) date and time of the observation; (3) Heliocentric Julian date; (4) cycle number based on the ephemeris in Eq. (1); (5) instrument used; (6) exposure time per polarimetric sequence; (7) S/N per polarimetric sequence at 650 nm per CCD pixel of unpolarised spectrum; and (8) RMS noise level of Stokes V signal in units of unpolarised continuum.

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