Table C.1.
Journal of photometric observations.
| Station | Time interval | No. of | Passbands | HD of comparison | Source |
|---|---|---|---|---|---|
| (HJD−2400000) | obs. | / check star | |||
| 61 | 47909.64–48695.02 | 70 | Hp | – | Perryman & ESA (1997) |
| 1 | 54116.25–54134.40 | 35 | UBV | 21686/21933 | This paper |
| 1 | 54468.34–54720.57 | 13 | UBV | 21686/21933 | This paper |
| 1 | 54862.31–54862.32 | 3 | UBV | 21686/21933 | This paper |
| 1 | 55545.35–55545.36 | 3 | UBV | 21686/21933 | This paper |
| 1 | 55574.25–55849.64 | 238 | UBV | 21686/21933 | This paper |
| 1 | 55850.37–55850.54 | 9 | UBV | 21933/21686 | This paper |
| 1 | 55851.40–55852.47 | 21 | UBV | 21686/21933 | This paper |
| 1 | 55853.37–55850.50 | 12 | UBV | 21933/21686 | This paper |
| 1 | 55854.49–55945.33 | 97 | UBV | 21686/21933 | This paper |
| 128 | 56222.00–56238.03 | 18510 | MOST | – | Nemravová et al. (2016) |
| 1 | 56520.59–56527.60 | 9 | UBVR | 21686/21933 | This paper |
| 1 | 56882.61–56882.63 | 3 | UBVR | 21686/21933 | This paper |
| 1 | 57634.55–57656.64 | 9 | UBVR | 21686/21933 | This paper |
| 1 | 57775.27–58079.35 | 20 | UBVR | 21686/21933 | This paper |
| 128 | 58044.20–58058.55 | 12179 | MOST | – | This paper |
| 1 | 58132.30–58402.48 | 64 | UBVR | 21686/21933 | This paper |
| 1 | 58490.21–58490.32 | 21 | UBVR | 21686/21933 | This paper |
| 1 | 58858.24–58865.42 | 42 | UBVR | 21686/21933 | This paper |
| 110 | 59144.53–59169.94 | 1630 | TESS | – | This paper |
| 110 | 59447.71–59473.15 | 1706 | TESS | – | This paper |
| 110 | 59474.18–59498.88 | 1590 | TESS | – | This paper |
| 110 | 59500.20–59524.44 | 1592 | TESS | – | This paper |
| 110 | 60208.55–60230.89 | 2466 | TESS | – | This paper |
| 110 | 60237.00–60259.49 | 2479 | TESS | – | This paper |
| 1 | 59594.27–59594.40 | 22 | UBVR | 21686/21933 | This paper |
| 1 | 60323.28–60323.41 | 22 | UBVR | 21686/21933 | This paper |
Notes. In the column “Station", the individual observing stations are identified by the running numbers from the Praha/Zagreb photometric archives: 1 .. Hvar 0.65-m reflector, EMI tubes; 61 .. Hipparcos Hp photometry transformed into Johnson V after Harmanec (1998); 110 .. TESS satellite broad-band photometry, sectors 31, 42, 43, 44, 70, and 71; 128 .. MOST satellite broadband photometry.
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