Table D.4.
Journal of available photometry.
| Station | Time interval | No. of | Passbands | Comparison | Check(s) | Source |
|---|---|---|---|---|---|---|
| (RJD) | obs. | HD | HD | |||
| 44 | 36312.98–36492.70 | 78 | V | 184663 | 183227 | 1 |
| 26 | 40448.90–40457.90 | 8 | UBV | 183227 | – | 2 |
| 37 | 43382.63–43755.58 | 2 | 7C→ UBV | all-sky | – | 3 |
| 01 | 44073.40–48128.39 | 425 | UBV | 183324 | 183227, 184663 | 4 |
| 20 | 44773.75–49951.73 | 118 | BV | 183324 | 183227 | 5 |
| 12 | 45249.56–49591.68 | 153 | uvby | 183324 | 183227 | 6 |
| 04 | 45525.50–45573.37 | 5 | UBV | 183227 | 183324 | 4 |
| 61 | 47879.03–48974.17 | 128 | Hp → V | all-sky | – | 7 |
| 30 | 52060.81–52752.94 | 43 | UBV | 183324 | 183227 | 4 |
| 01 | 52076.49–53936.53 | 300 | UBV | 183227 | 184663 | 4 |
| 118 | 52415.55–52424.56 | 63 | uvby | 183227 | 183563 | 11 |
| 93 | 52443.74–55131.52 | 558 | V | all-sky | – | 8 |
| 66 | 52763.49–52764.54 | 9 | UBV | 183324 | 184663 | 4 |
| 89 | 52850.39–53309.29 | 74 | UBV | 183324 | 184663 | 4 |
| 118 | 53565.45–53575.63 | 121 | uvby | 183227 | 183563 | 11 |
| 01 | 53937.50–53937.52 | 3 | UBV | 184663 | 183227 | 4 |
| 01 | 53969.36–56475.46 | 293 | UBV | 183227 | 184663 | 4 |
| 117 | 55696.30–58983.29 | 454 | V | all-sky | – | 9 |
| 117 | 56425.28–58983.29 | 374 | Ic | all-sky | – | 9 |
| 01 | 56747.35–57116.36 | 57 | UBVR | 183227 | 184663 | 4 |
| 114 | 57079.15–58430.69 | 336 | V | all-sky | – | 10 |
| 114 | 58221.90–58986.06 | 821 | g | all-sky | – | 10 |
Notes. Column “Station”: The running numbers of individual observing stations they have in the Prague/Zagreb photometric archives: 01: Hvar 0.65 m, Cassegrain reflector, EMI6256B (1979–1990), EMI6256S (1990–2003), and EMI9789QB (since 2003) tubes; 04: Ondřejov 0.65 m Cassegrain reflector, EMI tube; 12: ESO LaSilla 0.50 m, Bochum 0.61 m, and 0.50 m Danish reflectors; 20: Toronto 0.40 m reflector, DC photometer with EMI6094 tube and Optec SSP-3 solid state photometer after 1994; 26: OHP Chiron station 0.60 m reflector, Lallemand tube; 30: San Pedro Mártir 0.90 m reflector; 37: Jungfraujoch 0.76 m telescope, P3 photometer; 44: Mount Palomar 0.51 m reflector and a photometer with EMI 6094 tube; 61: HIPPARCOS all-sky Hp photometry transformed to Johnson V; 66: Tubitak 0.40 m Cassegrain reflector, Optec SSP5A photometer; 89: Canakkale 0.40 m reflector, Optec SSP5 photometer; 93: ASAS3 photometric survey; 114: ASAS-SN photometric network; 117: Kamogata-Kiso-Kyoto Wide-field Survey (KWS) imager with 0.105 m lens and SBIG ST-8XME CCD Camera; 118: Sierra Nevada 0.90 m reflector, multichannel photometer.
References. Column “Source” gives the source of data: 1: Lynds (1960); 2: Haupt & Schroll (1974) and priv. comm. to PH; 3: Burki (1980), priv. comm. to PH; 4: This paper; 5: Percy et al. (1988, 1997); 6: Manfroid et al. (1991), Sterken et al. (1993), Manfroid et al. (1995), Sterken et al. (1995); 7: Perryman & ESA (1997); 8: Pojmanski (2002); 9: Maehara (2014); 10: Shappee et al. (2014), Kochanek et al. (2017), Jayasinghe et al. (2019); 11: Gutiérrez-Soto et al. (2007).
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