VizieR Online Data Catalog: Rotation periods of Group X candidate members (Messina+, 2022)

Group X is a nearby moving group (d~101pc; Tang et al., 2018ApJ...862..106T, Cat. J/ApJ/862/106).

We have explored the rotational properties of the late-type candidate members of the recently discovered moving group Group X, which has a total of 218 candidate members. All the candidate members were observed by TESS in one or more sectors, and we extracted the light curves from the FFIs using the PATHOS pipeline. The rotation period search was done using three different methods, GLS, CLEAN, and ACF, which provided rotation period measurements for 168 stars (150 with grade A and 18 with grade B).

(1 data file).