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Table 1

Summary of the datasets used in this paper

Dataset NtotN v sin i σ(v sin i)⟩ Source
Praesepe 120/113 8.4 1.5 M09, K14, R17
HJhost 39/39 4.0 0.6 M15
KOIhost 61/61 6.2 1.1 W17
Field (A) 97/91 51.3 20.0 A01
Field (B) 193/179 46.1 14.8 Net17
Field (C) 55/46 24.8 1.6 M13, N15, N17
N13, R15, Mc14

Notes. HJhost and KOIhost stand for the two separate sets of extrasolar planet host stars (mostly with hot Jupiters and various Kepler planets, respectively). Field (A,B,C) stand for three sets of Galactic field stars. ⟨v sin i ⟩ and ⟨σ(v sin i)⟩, respectively, denote the averages of the v sin i values and the averages of their errors given in the source for v sin i. The total number of items and the number actually used in this work are denoted by Ntot and N, respectively.See Sect. 2.2 for the description of the selection criteria.

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