Table 1
Summary of the datasets used in this paper
| Dataset | Ntot ∕N | ⟨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.
References. M09: Mermilliod et al. (2009); K14: Kovács et al. (2014); R17: Rebull et al. (2017); M15: Maxted et al. (2015) + current literature (11 stars); W17: Winn et al. (2017); A01: Abt (2001); Net17: Netopil et al. (2017); M13: Molenda-Zakowicz et al. (2013); N15: Niemczura et al. (2015); N17: Niemczura et al. (2017); N13: Nielsen et al. (2013); R15: Reinhold & Gizon (2015); Mc14: McQuillan et al. (2014).
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