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Table 9:

The same as in Table 8 but for the CA2 stars. The identifier ID$_{\rm BR}$ is from Bragaglia et al. (1997).
ID$_{\rm BR}$ ID$_{\rm MO}$ RA Dec V B-V RV P [Fe/H] $\pm $ err Status
    (J2000) (J2000)     (km s-1) %    
2509 45412 254.816479 -52.707251 12.664 1.259 -28.71 93 +0.45 $\pm $ 0.11 clump, M
2885 45410 254.722210 -52.698323 12.629 1.289 -28.13 91 +0.47 $\pm $ 0.14 clump, M
4510 45414 254.775449 -52.665473 12.713 1.268 -27.44 91 +0.42 $\pm $ 0.12 clump, M
2508 45413 254.766037 -52.707004 12.666 1.241 -20.60 91 - clump, M, bin?
3595 45407 254.774389 -52.684524 12.360 1.252 -28.76 93 +0.48 $\pm $ 0.09 clump, M

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