The R-Process Alliance: Analysis of limited-r stars

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Table 1.

Basic data for the sample stars.

Stellar ID	RA	Dec	B	V	J	H	K	E(B − V)	BC_v	ϖ	D
			mag	mag	mag	mag	mag	mag	mag	mas	pc
2MASSJ00385967+2725516	00:39:00.2	+27:25:33.9	12.18	11.44	9.87	9.40	9.35	0.04	−0.37	0.78±0.02	1236 $_{- 32}^{+ 42}$ $^{+42}_{-32}$
2MASSJ20313531−3127319	20:31:35.0	−31:27:24.3	14.36	13.57	11.94	11.47	11.37	0.08	−0.49	0.38±0.02	2365 $_{- 114}^{+ 76}$ $^{+76}_{-114}$
2MASSJ21402305−1227035	21:40:23.3	−12:26:59.8	11.94	11.04	9.23	8.76	8.62	0.05	−0.51	0.34±0.03	2669 $_{- 185}^{+ 197}$ $^{+197}_{-185}$

References. The B and V magnitudes were taken from APASS (Henden et al. 2018), and the 2MASS JHK magnitudes were taken from Cutri et al. (2003). E(B − V) was calculated using the dust maps from Schlafly & Finkbeiner (2011), the bolometric corrections, BC_v, are based on Casagrande & VandenBerg (2014), the distances, D, were taken from Bailer-Jones et al. (2018), and the parallaxes, ϖ, from Gaia Collaboration (2023).

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