Table 1
GTO M dwarfs excluded from the analysis.
Karmn | Name | Reason |
---|---|---|
J00162+198W | EZ Psc AB | (1) |
J01056+284 | GJ 1029 AB | (1) |
J02486+621 | 2MASS J02483695+6211228 | (3) |
J02573+765 | G 245-61 | (3) |
J04198+425 | LSR J0419+4233 | (4) |
J04219+213 | K2-155 | (3) |
J05394+406 | LSR J0539+4038 | (4) |
J05532+242 | Ross 59 AB | (1) |
J07001−190 | 2MASS J07000682−1901235 AB | (1) |
J08536−034 | LP 666-009 | (4) |
J10182−204 | NLTT 23956 AB | (1) |
J10354+694 | LP 037-179 AB | (1) |
J14155+046 | GJ 1182 AB | (1) |
J15412+759 | UU UMi AB | (1) |
J15474−108 | LP 743-031 ABC | (2) |
J16343+571 | CM Dra Aab | (5) |
J18356+329 | LSR J1835+3259 | (4) |
J19169+051S | V1298 Aql | (4) |
J19255+096 | LSPM J1925+0938 | (4) |
J20198+229 | LP 395-008 AB | (1) |
J20556−140N | GJ 810 Aab | (1) |
J23064−050 | 2MUCD 12171 (Trappist-1) | (4) |
J23585+076 | Wolf 1051 ABC | (2) |
References. (1) Double-line spectroscopic (SB2) binary (Baroch et al. 2018, 2021). (2) Triple-line spectroscopic triple systems (Baroch et al. 2021). (3) Conspicuous artefacts in the CARMENES template spectra. (4) Spectral type M8.0 V or later. (5) Eclipsing binary (Morales et al. 2009).
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