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Table 4

Proposed cycle periods using alone for stars without CARMENES data detections or literature values.

Karmn Name SpT(a) No. of spec. Time baseline (a) cycle (a) Visual inspection
J10251−102 BD-09 3070 M1.0 62 9.0 2.3 6.1 a CARMENES baseline, weak trend in Ca, Hα
J11054+435 BD+44 2051A M1.0 125 8.1 1.8 data gap, 2.7 a in Ca, Hα(b)
J14010−026 HD 122303 M1.0 226 11.7 2.6 1.3 a CARMENES baseline, no trend
J20533+621 HD 199305 M1.0 73 14.1 7.8 3.8 a CARMENES baseline, 3.2 a in Hα(b)
J23492+024 BR Psc M1.0 207 14.2 27.3 5.6 a CARMENES baseline, maybe trend in Hα
J20450+444 BD+44 3567 M1.5 80 6.7 7.2 3.7 a in Ca, Hα(b)
J10289+008 BD+01 2447 M2.0 204 12.9 3.3 3.1 a in Ca, Hα(b)
J14294+155 Ross 130 M2.0 52 7.7 1.9 too few CARMENES data
J11421+267 Ross 905 M2.5 302 15.2 17.2 2.3 a CARMENES baseline, no trend

Notes. (α)Spectral (sub-)type of M. (b)Periods given correspond to the highest peak in the periodogram, regardless of the assigned FAP.

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