Pyxis  C0906-370 
RA: 9:07:57.8  DEC: -37:13:17  (J2000)

(Most recent updates: 
Membership probability flag - 2024; Remaining data - October 2015)
============================================================
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
=========================================================================
No known variables
========================================================================
Supplementary Notes 

Pyxis is a distant globular cluster, located approximately 40 kpc from 
the Galactic centre.  A CM diagram published by Dotter et al. (2011),
based on HST photometry, shows a prominent red HB.  Harris (1996) 
lists [Fe/H] = -1.20 in the 2010 update to his catalogue. 

========================================================================
References

Dotter, A., Sarajedini, A., Anderson, J. 2011, ApJ, 738, 74

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

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

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