The CARMENES search for exoplanets around M dwarfs - Spectroscopic orbits of nine M-dwarf multiple systems, including two triples, two brown dwarf candidates, and one close M-dwarf–white dwarf binary

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Fig. 4.

Best orbital fit to the RVs of GJ 912 from CARMENES (blue circles), HARPS (red triangles), and FEROS (green squares) as a function of time. Residuals from the best fit are depicted in the bottom panel. Those corresponding to the FEROS observations are outside the Y-axis scale.

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