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Table A.2

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

Telescope Date of Start time End time Nobs Texp Filter Airmass Moon Aperture Scatter
first obs (UT) (UT) (s) illum. radii (px) (mmag)
HAT-P-3
Cassini 2010.06.07 20:12 00:16 107 60–150 Gunn i 1.01 → 1.35 22% 16, 26, 50 1.69
CA 1.23 m 2015.05.01 20:09 03:52 246 85 Cousins I 1.22 → 1.03 → 1.50 96% 17, 40, 60 1.49
CA 1.23 m 2015.05.07 19:45 02:23 178 102–135 Cousins I 1.21 → 1.03 → 1.28 84% 22, 45, 70 0.66
CA 1.23 m 2015.06.02 20:28 03:01 183 98–130 Cousins I 1.04 → 1.03 → 2.20 100% 20, 45, 70 0.83
                     
HAT-P-12
INT 2010.04.29 02:28 05:47 91 100 Gunn r 1.12 → 2.15 97% 20, 40, 60 0.92
CA 2.2 m 2010.05.11 21:11 03:54 151 80–120 Strömgren u 1.07 → 1.03 → 1.74 5% 9, 14, 30 5.97
CA 2.2 m 2010.05.11 21:11 03:54 157 80–120 Gunn g 1.07 → 1.03 → 1.74 5% 25, 35, 60 1.14
CA 2.2 m 2010.05.11 21:11 03:54 146 80–120 Gunn r 1.07 → 1.03 → 1.74 5% 28, 38, 70 1.04
CA 2.2 m 2010.05.11 21:11 03:54 166 80–120 Johnson I 1.07 → 1.03 → 1.74 5% 25, 35, 60 1.32
CA 1.23 m 2012.03.06 23:41 05:33 83 105–130 Cousins R 1.31 → 1.00 → 1.13 97% 24, 45, 70 1.38
Cassini 2012.04.21 01:38 03:24 47 120 Gunn r 1.20 → 1.61 0% 20, 55, 85 1.27
CA 1.23 m 2013.06.15 20:48 01:44 146 70–120 Cousins R 1.00 → 2.05 41% 23, 48, 70 1.22
CA 1.23 m 2014.03.16 00:55 05:23 152 85–100 Cousins I 1.07 → 1.00 → 1.17 100% 28, 50, 72 1.06
CA 1.23 m 2014.04.13 20:58 03:42 156 120–150 Cousins I 1.44 → 1.00 → 1.21 98% 35, 55, 75 0.94
CA 1.23 m 2015.06.24 21:58 01:35 95 120 Cousins R 1.07 → 2.13 55% 26, 54, 80 1.49
CA 1.23 m 2016.07.04 20:33 01:29 164 95 Cousins R 1.04 → 2.66 1% 18, 35, 50 1.62
                     
WASP-60
CA 12.3 m 2014.10.21 18:40 01:57 233 100 Cousins I 1.70 → 1.00 → 1.28 3% 19, 27, 50 0.68

Notes. Nobs is the number of observations, Texp is the exposure time, and “Moon illum.” is the geocentric fractional illumination of the Moon at midnight (UT). The aperture sizes are theradii of the software apertures for the star, inner sky, and outer sky, respectively. Scatter is the rms scatter of the data vs. a fitted model.

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