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Table 1

Relevant parameters of our observations.

Date Telescope σres N CAD Ttot χmax,min β Δpix Δs TC
yyyy.mm.dd (ppt) (s) (h) (maxx,y) (pix)
2015.03.30 CASLEO 1.8 597 25 4.31 1.53,1.23 2.33 40 3 OIBEO
2015.04.12 NOT 0.8 843 18 4.24 2.33,1.10 2.00 4 3 OIBEO
2015.04.16 CASLEO 1.6 307 74 6.28 1.94,1.23 2.15 50 6 OIBEO
2015.05.20 NOT 1.8 482 19 2.67 1.82,1.13 1.62 3 2 OIBE–
2015.06.06 NOT 3.1 943 15 3.91 2.95,1.12 1.19 4 4 OIBEO
2015.06.23 NOT 2.0 977 14 3.81 2.33,1.10 1.47 2 2 OIBEO
2016.05.14 CASLEO 1.9 372 36 3.77 2.13,1.23 1.51 120 8 –IBEO
2017.05.13 CASLEO 3.3 289 63 5.12 2.03,1.23 2.59 52 3 OIBEO
2017.05.30 CASLEO 1.8 742 22 4.58 1.94,1.23 2.84 35 3 OIBEO
2017.06.16 CASLEO 1.9 174 52 2.53 1.31,1.23 1.42 30 3 OIB–
2018.07.01 STELLA 1.2 141 112 4.42 1.98,1.09 1.75 350 6 –BEO

Notes. From left to right: the date corresponding to the beginning of the local night in yyyy.mm.dd, the telescope performing the observations, the standard deviation of the residual light curves in parts per thousand, σres, the number of data points per light curve, N, the average cadence in seconds, CAD, the total observing time, Ttot, in hours, the airmass range, χmax,min, showing maximum and minimum values, the β factor, to quantify correlated noise, the maximum variability in pixel position, Δpix, considering both x and y shifts, and the maximum variability in seeing, Δs, in pixels. Both values are rounded up. Last column shows the transit coverage, TC; a description of the transit coding is detailed in the footnote of this table. The letter code to specify the transit coverage during each observation is the following: O: out of transit, before ingress. I: ingress. B: flat bottom. E: egress. O: out of transit, after egress.

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