CARMENES input catalog of M dwarfs - VII. New rotation periods for the survey stars and their correlations with stellar activity

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Table 1.

Overview of sources of light curve data for the targets in the CARMENES survey.

Survey	Location	Instrument configuration	Band	No. of
				light curves ^(a)
SuperWASP	Roque de los Muchachos, Spain	8 × Andor DW436	Clear, Broad (0.4–0.7 μm)	112 (99)
	Sutherland, South Africa		Broad (0.4–0.7 μm)
AstroLAB IRIS	Zillebeke, Belgium	0.68 m Keller	B, V, R	6 (6)
		+ SBIG STL-6303E
OSN	Observatorio de Sierra Nevada, Spain	0.90 m, 1.50 m	B, V, R, I	22 (14)
LCOGT	Las Cumbres Observatory, Chile	0.40 m	B, V, i	13 (9)
TJO	Montsec Observatory, Spain	0.80 m + LAIA	R	5 (3)
TESS	Space	4 × 0.10 m + CCID-80	T (0.6–1.0 μm)	240

Notes.

^(a)

The number of light curves with > 25 nightly-binned epochs, i.e., deemed admissible for analysis, are given in parentheses. Applicable only to ground-based data sets.

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