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Table 1
Information of our programme stars.
| Object | 2MASS ID | B | V | Proper motions (a) | Parallaxes (a) | Probability (b) | Type of |
|---|---|---|---|---|---|---|---|
| mag | mag | mas yr−1 | mas | % | star (c) | ||
| Y1194 | J08510080+1148527 | 15.28 | 14.61 | −10.878 −2.757 [0.067 0.061] | 1.1164 [0.0369] | 99 | ST |
| Y519 | J08510951+1141449 | 13.50 | 12.75 | −10.333 −3.106 [0.075 0.059] | 1.0848 [0.0431] | 98 | SG |
| Y923 | J08514401+1146245 | 13.50 | 12.75 | −11.100 −2.889 [0.072 0.046] | 1.1190 [0.0415] | 100 | SG |
| Y1844 | J08513540+1157564 | 13.50 | 12.76 | −11.097 −3.008 [0.067 0.044] | 1.1499 [0.0422] | 91 | SG |
| Y535 | J08510131+1141587 | 14.00 | 13.45 | −11.041 −2.813 [0.045 0.031] | 1.1077 [0.0261] | 100 | TO |
| Y1388 | J08505474+1151093 | 14.08 | 13.52 | −10.821 −2.941 [0.046 0.036] | 1.0874 [0.0273] | 99 | TO |
| Y2235 | J08510470+1204193 | 14.06 | 13.50 | −10.944 −2.967 [0.041 0.029] | 1.1506 [0.0262] | 100 | TO |
Notes. (a) Proper motions (in RA and Dec), and parallaxes with uncertainties were taken from Gaia Collaboration (2018). (b) Probability of being a member of M 67, taken from Yadav et al. (2008). (c)Stellar type: subgiant star (SG), turn-off star (TO), solar twin (ST).
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