Flares in open clusters with K2 - II. Pleiades, Hyades, Praesepe, Ruprecht 147, and M 67

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Table B.1.

Non-exhaustive literature overview over OC parameters.

Cluster	Source	Distance [pc]	Age [Myr]	[Fe/H]
Pleiades	Adopted in this work:	135.6		−0.037 ± 0.026
	Bossini et al. (2019)^(a)
	Cantat-Gaudin et al. (2018)	135.6
	Gossage et al. (2018)
	Yen et al. (2018)	126.3
	Chelli & Duvert (2016)	139
	Netopil et al. (2016)			-0.01
	Dahm (2015)
	Scholz et al. (2015)	130	120
	Conrad et al. (2014)			−0.037 ± 0.026
	Melis et al. (2014)	136
	Bell et al. (2012)	135	125

Hyades	Adopted in this work: ^(c)			0.13 ± 0.02
	Gaia Collaboration (2018a)
	Gossage et al. (2018)		680
	Liu et al. (2016)			±0.02
	Netopil et al. (2016)			0.13
	Taylor & Joner (2005)			0.103 ± 0.008
	Salaris et al. (2004)		650	0.15
	Perryman et al. (1998)

Praesepe	Adopted in this work:	185.5		0.16
	Bossini et al. (2019)
	Cantat-Gaudin et al. (2018)	185.5
	Gossage et al. (2018)		590
	Yen et al. (2018)	183
	Netopil et al. (2016)			0.16
	Scholz et al. (2015)	187	832
	Boesgaard et al. (2013)			0.12
	Boudreault et al. (2012)	160	630
	Salaris et al. (2004)	175	650

Ruprecht 147	Adopted in this work:	305		0.08 ± 0.07
	Bragaglia et al. (2018)			0.08 ± 0.07
	Cantat-Gaudin et al. (2018)	305
	Gaia Collaboration (2018a)	309
	Torres et al. (2018)	283
	Curtis (2016)^(b)			0.10 ± 0.02
	Scholz et al. (2015)	270	1953
	Curtis et al. (2013)	300		0.07 ± 0.03

M 67	Adopted in this work:	908		−0.102 ± .081
	Bossini et al. (2019)
	Netopil et al. (2016)			0.03
	Barnes et al. (2016)
	Scholz et al. (2015)
	Conrad et al. (2014)			−0.102 ± .081
	Dias et al. (2012)	908	4300
	Önehag et al. (2011)	880	4200	0.02
	Salaris et al. (2004)			0.02 ± 0.06

Notes.

^(a)

Bossini et al. (2019) noted some caveats for their determination of ages of young clusters, for which they used Gaia DR2 photometry for isochrone fitting.

^(b)

Curtis (2016) reanalysed HIRES spectra using an improved spectroscopic method as compared to Curtis (2016).

^(c)

We did not adopt a mean value for the Hyades distance because the cluster members are on average closer than 50 pc.

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