Table 5.
Summary of photometric observations.
Source | Station | Epoch | No. of | No. of | HDcomp./ | Passbands |
---|---|---|---|---|---|---|
No. | HJD–2400000 | obs. | nights | HDcheck | used | |
A,G | 106 | 41034.92–49433.90 | 163 | 41 | 93131/93695,92740 | UBV |
G | 106 | 41290.07–43270.11 | 101 | 64 | 93131/93695,92740 | UBV |
B | 105 | 42447.81–42484.70 | 34 | 34 | 93222/ – | λ 5170 Å |
C | 61 | 47885.45–49016.76 | 114 | 31 | Space observations | Hp |
D | 12 | 48682.59–49459.56 | 293 | 20 | 93131/92740,93695 | UBV |
G | 111 | 49106.99–49437.10 | 29 | 18 | 93131 | V |
E | 106 | 49380.90–49422.21 | 87 | 11 | 93695/93131,93737 | UBV |
F | 93 | 51962.71–55168.84 | 682 | 562 | All-sky | V |
G | 11 | 53116.35–53123.32 | 48 | 4 | 93131/ – | UBV |
G | 109 | 54987.00–57837.94 | 120 | 109 | 93131/93222 | BV |
G | 11 | 55568.48–55578.58 | 30 | 5 | 93131/93222 | UBV |
G | 126 | 56811.48–57190.59 | 504 | 27 | 92741 | V |
G | 107 | 56973.15–57288.25 | 55 | 52 | Many | BVRI |
H,G | 100 | 57039.00–57124.08 | 901 | 23 | 93131/93695 | BVR |
G | 108 | 57069.22–57173.09 | 49 | 49 | Many | BVRI |
H,G | 100 | 57441.96–57743.24 | 1174 | 18 | 93131/93695 | BVR |
G | 100 | 57768.96–57808.29 | 426 | 6 | 93131/93695 | BVR |
G | 122 | 57784.56–57806.28 | 199 | 21 | Space observations | BRITE R |
H,G | 124 | 57756.46–57966.21 | 303 | 100 | 93695 | V |
G | 122 | 57806.42–57820.31 | 133 | 14 | Space observations | BRITE R |
G | 122 | 57820.37–57843.09 | 255 | 23 | Space observations | BRITE R |
H,G | 108 | 57822.98–57823.39 | 121 | 1 | Many | V |
G | 122 | 57843.37–57875.92 | 394 | 33 | Space observations | BRITE R |
G | 122 | 57876.00–57936.26 | 635 | 59 | Space observations | BRITE R |
G | 123 | 58165.18–58187.96 | 253 | 23 | Space observations | BRITE R |
G | 123 | 58188.03–58217.97 | 424 | 30 | Space observations | BRITE R |
H,G | 100 | 58194.88–58249.13 | 599 | 10 | 93131/93695 | BVR |
G | 123 | 58218.05–58257.48 | 468 | 40 | Space observations | BRITE R |
G | 122 | 58254.47–58258.38 | 37 | 5 | Space observations | BRITE R |
G | 122 | 58258.99–58315.08 | 477 | 56 | Space observations | BRITE R |
H,G | 124 | 58512.45–59054.18 | 165 | 79 | 93695 | V |
G | 123 | 58512.74–58611.26 | 413 | 39 | Space observations | BRITE R |
H,G | 125 | 58565.92–58680.97 | 986 | 17 | 93131/93695 | V |
G | 110 | 58569.47–58595.64 | 602 | 27 | Space observations | λ 5680–11260 Å |
G | 110 | 58596.83–58623.85 | 620 | 28 | Space observations | λ 5680–11260 Å |
G | 123 | 58611.33–58681.54 | 643 | 58 | Space observations | BRITE R |
G | 122 | 58887.00–58941.78 | 702 | 56 | Space observations | BRITE R |
G | 122 | 58941.85–59004.86 | 638 | 58 | Space observations | BRITE R |
G | 125 | 59015.87–59074.85 | 69 | 18 | 93131/93695 | V |
Notes. Abbreviations of column “Stations” (numbers are running numbers of the observing stations from the Praha/Zagreb data archives): 11. South African Astronomical Observatory 0.5 m reflector Hamamatsu tube; 12. ESO 0.50 m reflector, La Silla; 61. HIPPARCOSHp magnitude transformed to Johnson V after Harmanec (1998); 93. ASAS3 APT; 100. Chester Hill, Sydney, 0.08 m refractor, Canon 600D DSLR camera; 105. ESO La Silla Bochum 0.61 m reflector, cooled tube; 106. Auckland Observatory 0.50 m Cassegrain reflector, EMI 9502S/A tube; 107. The Bright Star Monitor Australia Station, AstroTech AT-72 refractor, Camera: SBIG ST8-XME, owned and operated by Peter Nelson (see https://www.aavso.org/bsm-south); 108. Martin Bruce Berry Bright Star Monitor (see https://www.aavso.org/bsm-berry), Perth, Australia, currently operated by Greg Bolt; 109. Terrence Bohlsen Australia; 110. TESS broad-band space photometry; 111. Harry Williams Milton Road Observatory; 122. BRITE BHr satellite; 123. BRITE BTr satellite; 124. Henley Observatory, 0.150 m refractor, Canon 1300D DSLR camera; 125. Congarinni Observatory, 0.08 m refractor stopped down to 0.05 m; 126. FRAM 0.30 m automatic monitor, Pierre Auger Observatory, Argentina.
References. Abbreviations of column “Source”: A. Walker & Marino (1972); B. Moffat (1977); C. ESA (1997); D. Mayer et al. (1992, 2010) and this paper; E. Mayer et al. (1998) and this paper; F. Pojmanski (2002); G. This paper; H. Blackford et al. (2020).
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