Open Access

Table A.3.

Optical photometric observations.

Band Telescope ID Start (MJD) Stop (MJD) Observing Nights Covered nights (%) MAG min MAG max
U A3 58270 58755 13 2.7 15.580 12.628
G2 58219 58923 63 8.9 16.214 11.796
SA 58240 58697 14 3.1 18.438 12.087

B 1301 58927 59066 3 2.1 19.204 15.154
1400 58338 59066 62 8.5 19.227 13.429
2300 58295 58912 75 12.1 19.107 12.728
18 58221 58738 31 6.0 14.990 12.368
2T 58274 58729 25 5.5 15.400 13.422
A3 58270 58766 35 7.0 18.080 13.395
G2 58219 58923 67 9.5 18.841 12.362
SA 58240 58740 21 4.2 19.212 12.702

V 1301 58927 59066 7 5.0 19.183 14.802
1400 58338 59066 62 8.5 18.533 13.259
2300 58295 58912 83 13.4 18.422 12.824
18 58221 58738 34 6.6 14.946 12.217
2T 58274 58729 26 5.7 15.184 13.234
A3 58270 58767 48 9.6 17.612 13.178
AAVSO 58198 58432 139 59.1 15.337 11.806
G2 58219 58923 67 9.5 16.802 12.259
SA 58240 58740 21 4.2 18.219 12.577

Clear (to V)* AAVSO 58201 58390 129 67.9 14.753 11.677

R 1301 58927 59066 7 5.0 18.145 14.512
2300 58295 58912 84 13.6 18.073 12.641
18 58221 58738 35 6.8 14.390 11.970
2T 58274 58729 28 6.1 14.844 12.961
A3 58270 58766 37 7.4 17.029 12.914
G2 58219 58923 72 10.2 18.469 11.874
SA 58240 58740 21 4.2 17.529 12.295

Clear (to R)* 18 58580 58723 2 1.4 14.317 13.557
2T 58801 58801 1 100.0 18.200 18.200
3T 58638 58808 14 8.2 18.258 16.942
G2 58364 58923 21 3.8 18.282 13.346

I 18 58221 58738 33 6.4 14.162 11.583
2T 58274 58729 26 5.7 14.430 12.604
A3 58270 58765 35 7.1 16.430 12.640
G2 58219 58923 63 8.9 15.966 11.631
SA 58240 58740 21 4.2 16.732 11.941

g’ 1400 58338 59066 66 9.1 18.921 13.326

r’ 1400 58338 59066 68 9.3 18.251 13.242

i’ 1400 58338 59066 65 8.9 18.191 13.222

*Clear (to V) or Clear (to R) stands for the observations taken in white light (without any filters) and reduced as if they were taken in V or R band.

Notes. The column "Covered nights" shows the percentage of the observed nights over the total number of nights in the interval from the first to the last observation for each band and each Telescope ID (Table A.2).

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