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Table 1

Details of the observations presented in this work.

Telescope Date Start/End times N obs t exp Filter Airmass Moon Aperture Scatter PSF β

Kuiper 2009 10 22 04:03 → 09:10 1083 5 Cousins I 1.00 → 1.9 25% 10, 20, 25 1.54
Loiano 2009 11 12 16:52 → 22:09 103 118 Gunn r 1.02 → 1.01 → 1.55 23% 25, 45, 60 1.15 1963 1.4
INT 2010 08 28 20:44 → 04:02 131 140 Strömgren y 2.04 → 1.00 → 1.18 84% 45, 65, 90 0.47 3217 1.7
Loiano 2011 10 05 18:01 → 02:29 469 50 Gunn i 1.12 → 1.01 → 1.45 61% 19, 40, 60 1.15 908 1.4
CA 1.23 m 2011 10 05 19:27 → 03:07 166 70 Johnson R 1.08 → 1.05 → 1.54 61% 26, 38, 55 0.83 1662 1.0
CA 2.2 m 2012 08 26 20:31 → 04:48 160 80 sdss u 1.52 → 1.00 → 1.55 77% 25, 55, 75 2.37 2827 1.0
CA 2.2 m 2012 08 26 20:31 → 04:48 157 80 Gunn g 1.52 → 1.00 → 1.55 77% 30, 50, 70 0.97 2463 1.2
CA 2.2 m 2012 08 26 20:31 → 04:48 159 80 Gunn r 1.52 → 1.00 → 1.55 77% 30, 60, 90 0.71 2642 1.5
CA 2.2 m 2012 08 26 20:31 → 04:48 162 80 Gunn z 1.52 → 1.00 → 1.55 77% 28, 55, 80 0.92 1662 1.1
Loiano 2012 10 02 17:45 → 02:32 232 70 Johnson I 1.03 → 1.00 → 1.92 92% 23, 40, 65 0.79 2521 1.0
CA 1.23 m 2012 10 02 20:07 → 03:35 373 50 Johnson I 1.11 → 1.00 → 2.16 92% 35, 60, 90 1.69 2290 1.8

Notes. Nobs is the number of observations, Moon is the fractional illumination of the Moon at the midpoint of the transit, and texp is the exposure time in seconds. The aperture sizes are the radii in pixels of the software apertures for the star, inner sky and outer sky, respectively. Scatter is the rms scatter of the data versus a fitted model, in mmag. Target mean PSF area in px2 is also reported for each dataset. Times and dates are in UT. β is the ratio between the noise levels due to Poisson noise and to combined Poisson and red noise.

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