New Data added in the Database in May and June 2001
This page informs on the progress made in the inclusion of new data in the database.
Data added in 2001:
March - April |
January - February |
Data added in 2000:
November - December |
September - October |
July - August |
May - June |
March - April |
January - February
2001 June 6
Data from Sanner J., et al. 2001, Astron. Astrophys. 369, 511
Note : The old numbering system adopted so far in the databse has been temporarily kept. 10000 has been added to the
new star numbers from Sanner et al., which are like 1xxxx, where xxxx are Sanner's numbers.
2001 June 5
Data from Marco A., et al. 2001, Astron. J. 121, 2075
Note : The uvby ß CCD photometry of the standard fields in NGC 869, 884, 1039, 2169 and 6910 has also
been included in the database.
2001 June 1
Data from Sanner J., et al. 2001, Astron. Astrophys. 369, 511
Data from Sanner J., et al. 2001, Astron. Astrophys. 369, 511
Note : The numbering system of Sanner et al. (1431 stars) has been adopted. It replaces that of Moffat and Vogt (18 stars).
2001 May 31
Data from Kim S.-L., et al. 2001, Astron. Astrophys. 371, 571
Note :Double entries in the cross-reference table have been removed. This introduced corrections in the
rectangular X,Y position-, membership probability-, and RGU photometry files.
2001 May 29
Data from Gonzalez J.F., Lapasset E. 2001, Astron. J. 121, 2657
2001 May 22
Data from Carraro G., Patat F., Baumgardt H. 2001,
Astron. Astrophys. 371, 107
2001 May 21
Data from Piatti A.E., Clariá J.J. 2001,
Astron. Astrophys. 370, 931
Note :The numbering system of Piatti and Claria (356 stars) has been adopted and replace that by Sher (96 stars) and the
extended numbering system developed.
Data from Piatti A.E., Clariá J.J. 2001,
Astron. Astrophys. 370, 931
Note :The numbering system of Piatti and Claria (233 stars) has been adopted and replace that by Feinstein (17 stars) and the
extended numbering system developed.
2001 May 18
Data from Piatti A.E., Clariá J.J. 2001,
Astron. Astrophys. 370, 931
Note :The numbering system of Piatti and Claria (343 stars) has been adopted and replace that by Moffat and Fitzgerald (11 stars).
Data from Piatti A.E., Clariá J.J. 2001,
Astron. Astrophys. 370, 931
Note : The authors conclude that Ruprecht 140 is not a genuine cluster. Therefore, no cluster parameters have been tabulated.
Jean-Claude.Mermilliod@obs.unige.ch
Last Update: 5 June 2001