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Table 2

Key characteristics of the velocity standard stars.

Designation RA
J2016
Dec Spectral type Barycentric [km s-1] LOS velocity
BD +24 1843 8h04m42.70936675s 24° 19′49.47351216″ G 25.168 ±0.004
BD +31 1781 8h18m10.42693323s 30°35′49.7809604″ K 13.457 ±0.019
BD +34 1955 9h12m37.57008557s 33°36′01.09932489″ K 1.539 ±0.004
WDS J07277+2420A 7h27m39.94289657s 24°20′09.97879538″ K –18.559 ±0.208
BD +26 1647 7h46m58.48254722s 26°01′28.79033441″ G 13.109 ±0.008
BD +31 1684 7h53m33.99666092s 30°35′48.89008376″ G –234.195 ±0.013
BD +30 1501 7h26m19.81197854s 29°58′07.98205929″ K –36.684 ±0.044
TYC 2461-988-1 7h32m44.21719125s 33°50′06.07594227″ F 23.187 ±0.020
BD +36 1823 8h27m18.62972372s 35°49′01.65250699″ F 9.282 ±0.043
BD +35 1801 8h19m27.87619964s 35°01′21.76871662″ F –23.908 ±0.013

Notes. The data were sourced from Gaia Collaboration (2023) except the barycentric LOS velocities that are from Soubiran et al. (2018). We used the same approach for the designations as noted in Table 1. The equatorial coordinates are also in the International Celestial Reference System. Spectral types are from the Extended Stellar Parametrizer for Hot Stars module as part of Gaia DR3 Astrophysical parameters inference system (Creevey et al. 2023).

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