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Table B.1

Details of the photometric follow-up observations presented in this work.

Telescope Date of first obs Start time (UT) End time (UT) Nobs Texp (s) Filter Scatter (mmag)
HAT-P-17:
Cassini1.52m 2012.07.15 21:11 01:08 146 60 – 120 Gunn i 0.93
CA1.23m 2014.07.20 00:55 04:05 117 60 – 100 Cousins I 0.79
HAT-P-21:
Cassini1.52m 2012.03.03 21:54 00:47 211 60 Gunn r 4.23
CA1.23m 2012.03.07 00:55 05:10 145 110 – 120 Cousins R 0.99
HAT-P-26:
CA1.23m 2012.03.04 01:21 05:50 67 120 Cousins I 0.69
CA1.23m 2014.04.17 21:54 04:40 209 90 – 120 Cousins I 0.75
CA1.23m 2016.03.14 22:14 03:07 190 110 Cousins I 1.01
CA1.23m 2017.04.22 20:52 04:08 171 120 Cousins I 1.70
CA1.23m 2018.02.26 00:23 06:06 282 45 – 100 Cousins I 0.95
HAT-P-29:
CA1.23m 2011.10.03 22:13 05:07 121 120 Cousins R 0.58
TNG3.58m 2012.10.10 01:05 05:25 783 15 Johnson R 0.33
CA1.23m 2012.11.01 20:37 04:12 180 105 – 180 Cousins R 1.18
IAC80cm 2013.10.16 23:21 04:53 234 60 Cousins R 1.01
Copernico1.80m 2014.10.29 17:54 00:02 2303 7 Sloan r 0.67
Copernico1.80m 2016.01.07 17:20 23:26 2062 7 Sloan r 0.54
CA1.23m 2014.10.23 21:52 05:19 254 95 – 120 Cousins I 0.58
CA1.23m 2020.10.23 21:04 05:40 564 30 – 70 Cousins I 0.95

Notes. Nobs is the number of observations, Texp is the exposure time. Scatter is the rms scatter of the data versus a fitted model.

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