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Table 1

Logbook of the spectroscopic observations – grouped by stars and observing runs.

Instrument N BJD first BJD last S/N S/Ni Texp R Observer (PI)

KIC 3459297
Isis 1 2 456 088.66015 90 [76, 104] 1500 22 000 and 13 750a SB (JS)

KIC 4 930 889
Hermes 1 2 455 484.47403 90 90 1500 85 000 PIP
Hermes 1 2 455 821.53738 100 100 1900 85 000 JFG (EN)
Hermes 3 2 456 903.46202 2 456 907.45660 93 [87, 97] [900, 1200] 85 000 KDS
Hermes 10 2 457 129.71807 2 457 139.62990 80 [73, 86] 1200 85 000 TVR
Hermes 3 2 457 189.56028 2 457 197.63215 94 [93, 97] [1320, 1500] 85 000 MVS
Hermes 8 2 457 201.68442 2 457 208.47316 96 [83, 104] [1200, 1800] 85 000 PIP

KIC 9020774
Isis 2 2 456 090.57710 2 456 090.59895 27 [19, 35] 1800 22 000 and 13 750a SB (JS)

KIC 11971405
Hermes 2 2 455 487.34427 2 455 487.36568 79 [75, 84] 1800 85 000 PIP
Hermes 1 2 457 190.64447 88 88 1800 85 000 MVS
Hermes 2 2 457 201.65336 2 457 203.61089 56 [44, 68] 1200 85 000 PIP

Notes. For each observing run, the instrument, number of spectra N, BJD of the midpoint of the first and last exposure, average S/N level, range of S/N values (where the S/N of one spectrum is calculated as the average of the S/N measurements in several broad line free regions), typical exposure times (in seconds), resolving power of the spectrograph, and initials of the observer (and the PI if different) are given.

(a)

The resolution for the blue and red arms of Isis is different.

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