Open clusters in APOGEE and GALAH - Combining Gaia and ground-based spectroscopic surveys

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Table 2.

131 OCs in common between APOGEE DR14 and Cantat-Gaudin et al. (2018).

Cluster	Star	RV	σ_RV	e_RV	Nr	RV_lit	σ_RV, lit	Nr_lit	RV_GDR2^b	σ_GDR2	Nr_GDR2	[Fe/H]	σ_[Fe/H]	e_[Fe/H]	Nr	[Fe/H]_lit	σ_[Fe/H],lit	Nr_lit	Ref.
	type^a		(km s⁻¹)			(km s⁻¹)			(km s⁻¹)				(dex)		(dex)
Alessi 20	MS	−14.89		0.37	1	−11.5	0.01	2	−5.04	3.3	7								1
ASCC 124	MS	−23.35	0.54	0.38	2
ASCC 16	MS	17.41		0.62	1				23.18	3.4	15
ASCC 21	MS	16.30	5.66	1.30	19	18.57	2.12	9	18.7	4.45	9	0.01	0.09	0.03	10				2
Basel 11b	RGB	2.68	0.06	0.04	2				3.43	1.46	3	0.014	0.05	0.04	2
Berkeley 17	RGB	−73.34	0.41	0.13	9	−73.4	0.4	7	−71.95	1.77	7	−0.10	0.04	0.01	9	−0.11	0.03	7	3
Berkeley 19	RGB	17.44	0.0	0.08	1				17.65	0.42	1	−0.22		0.01	1
Berkeley 29	RGB	25.27	0.53	0.30	3	24.8	1.13	11	50.58	0.94	1								1
Berkeley 31	RGB	57.87	0.65	0.46	2	61.0	3.75	17				−0.305	0.037	0.026	2	−0.31	0.06	2	1,12
Berkeley 33	RGB	77.80	0.56	0.28	4	76.6	0.5	5	78.82	1.12	4	−0.23	0.11	0.05	4				2
Berkeley 43	RGB	29.712		0.136	1				29.15	1.42	9	0.00		0.01	1
Berkeley 53	RGB	−35.77	0.82	0.29	8	−36.3	0.5	4	−34.9	1.81	7	−0.02	0.03	0.01	6	0.00	0.02	5	3

Notes.

^(a)

Type of stars used in the analysis: (RGB) red giant branch, (MS) main sequence, or both.

^(b)

From Soubiran et al. (2018). The entire version is available at the CDS.

References. (1) Kharchenko et al. (2013); (2) Dias et al. (2002); (3) Donor et al. (2018); (4) Casamiquela et al. (2016); (5) Carrera et al. (2017); (6) Donati et al. (2015b); (7) Magrini et al. (2017); (8) Schiappacasse-Ulloa et al. (2018); (9) Blanco-Cuaresma et al. (2015); (10) Heiter et al. (2014); (11) Začs et al. (2011); (12) Friel et al. (2010); (13) Monroe & Pilachowski (2010).

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