In the selected data directories, the data have been split into ubvccd and vicccd, while under OGLE, the files have the format No Ref V B-V V-I sV sB-V sV-I Original_number.
The SMC database contains now data for 265 clusters.
Note : I am very grateful to G. Pietrzynski who provided me with these data. The availability of X,Y positions now permits to identify the stars.
In the selected data directories, the data have been split into ubvccd and vicccd, while under OGLE, the files have the format No Ref V B-V V-I Original_number.
The SMC database contains now data for 265 clusters.
The contents page dislays the type of data included sofar.
The principle is slightly different of that used for the galactic open clusters. Because the work of obtaining cross-identifications would be very important and that there are many difficulties with groundbased and HST spatial observations, it was decided to collect the data according to each author and numbering system.
For each cluster, there are selected data, i.e. a field reasonnably large around the cluser and the corresponding data. Complete data can be found under each author link on the cluster page. The facilities offered by WEBDA are similar: plot of the chart, search, and so on.
Additional data will be added to the database, especially for NGC 330, and content files will be improved. Files on integrated colours and archive data will also be enlarged.
Please send me your comments if you find something not working. I have tried to update most database facilities. I may have missed the modification of some scripts. Thanks for your comments.
epaunzen@physics.muni.cz