Table 4: Globular/Open Clusters, literature values. The selection constraints applied for identification of likely members are labeled with *.
Cluster ${\rm RA, Dec}$ (epoch J2000) ${\rm RA^*}$ ${\rm Dec^*}$ ${\rm [Fe/H]}$ age m-M RV RV*
    (degree) (degree) (dex) (Gyr)   ${\rm (km~s^{-1})}$ ${\rm (km~s^{-1})}$
${\rm M~15}$ $21^{\rm h}29^{\rm m}58.3^{\rm s}$, $+12^\circ10\hbox{$^\prime$ }01\hbox{$^{\prime\prime}$ }$ 322.25,322.75 11.90,12.40 -2.22 13.2 14.93 -110 -126,-100
${\rm M~13}$ $16^{\rm h}41^{\rm m}41.5^{\rm s}$, $+36^\circ27\hbox{$^\prime$ }37\hbox{$^{\prime\prime}$ }$ 250.00,250.90 36.10,36.90 -1.70 12.7 14.07 -250 -262,-243
${\rm M~2}$ $21^{\rm h}33^{\rm m}29.3^{\rm s}$, $-00^\circ49\hbox{$^\prime$ }23\hbox{$^{\prime\prime}$ }$ 323.10,323.60 -1.05,-0.60 -1.53 13.0 10.49 0 -20,20
${\rm NGC~2420}$ $07^{\rm h}38^{\rm m}24.0^{\rm s}$, $+21^\circ34\hbox{$^\prime$ }27\hbox{$^{\prime\prime}$ }$ 114.40,115.10 21.20,22.10 -0.50 3/4 11.40 73 50,86


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