NGC 6325 / C1714-237
RA: 17:17:59.21  DEC: -23:45:57.6 (J2000) 

(Most recent updates: 
Membership probability flag - 2024; Remaining data - April 2016)
============================================================
Bytes  Format      Explanation
1-8      A8        Star ID
10-32  A11,1x,A11  Position
34-35    A2        Membership probability flag based on data published
                   by Prudil & Arellano Ferro (2024)
                    m1: prob >=0.85;  m2: prob >=0.7 and <0.85;
                    m3: prob >= 0.5 and <0.7; f: prob <0.5
                    u:  no data available
37-44   F8.4       Period  (days)
46-51   F6.3       Mean magnitude (or maximum magnitude if "max" 
                      is indicated in the remarks column)
53-57   F5.3       Light amplitude (range of variability)
59      A1         Colour for mean magnitude and amplitude
                    e.g.  B, V, R, I, J, K
                    or P (for photographic).
61-65   A5         Type of variable (draft 2006 GCVS classifications)
                      CST denotes non variable stars previously designated
                      as variables
67-80   A19        Notes and Remarks  (f denotes field star)
 
 "--" or "----" indicates no data available
=========================================================================
ID       Position               Mem   Period <mag>  ampl  C Type  Notes/
         RA          Dec        Flag                              Remarks
=========================================================================
1        17:18:02.5  -23:45:45   m1  12.516  11.02  0.36  K CW
2        17:17:57.8  -23:46:36   m1  10.744  11.22  0.24  K CW 
===============================================================
Supplementary Notes 

This cluster is embedded in a crowded field in the Galactic bulge.
According to the 2010 version of the Harris (1996) catalogue, it is a
core collapsed cluster with [Fe/H] = -1.25. 
BVI photometry by Ortolani et al. (2003) shows a prominent blue HB
with evidence for a blue tail.

The data for V1 and 2 are from the discovery paper by Matsunaga et al.
(2006).
===================================================================
Discovery of the variable stars in NGC 6325

V1-2 
  Matsunaga et al. (2006) with RA and dec
===================================================================
References

Harris, W. E. 1996, AJ, 112, 1487

Matsunaga, N., Fukushi, H., Nakada, Y., Tanabe, T., Feast, M. W.,
Menzies, J. W., Ita, Y. and 7 coauthors, 2006, MNRAS, 370, 1979

Ortolani, S., Bica, E., Barbuy, B. 2003, A&A, 402, 565 

Prudil Z., Arellano Ferro, A. 2024, MNRAS, 534, 3654

=================================================================