Rotation periods for cool stars in the open cluster NGC 3532 - The transition from fast to slow rotation

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Table 2.

Description of the columns of the table with the measured rotation periods.

Name	Unit	Description
ID	–	ID in this work and F19
Designation	–	ID from Gaia DR2
CLWH	–	ID from Clem et al. (2011)
RA	deg	Right ascension from Clem et al. (2011)
Dec	deg	Declination from Clem et al. (2011)
Vmag	mag	V magnitude from Clem et al. (2011)
BV0	mag	(B − V)₀ colour from Clem et al. (2011)⁽¹⁾
VK0	mag	(V − K_s)₀ colour with K_s from 2MASS
Prot	d	Rotation period
dProt	d	Uncertainty on rotation period
Amp	mag	Light curve amplitude
Class	–	Classification of period [0, 1, 2, 3] ⁽²⁾
Binary	–	Binary status (True/False)

Notes.

⁽¹⁾

Dereddened with E_{(B − V)} = 0.034, E_{(V − K_s)} = 0.095 (F19).

⁽²⁾

Classes are 0: possible alias, 1: first class, 2: algorithmic periods, 3: activity-informed periods.

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