The USNO A-V1.0 Catalogue and this Service

The Catalogue provided here on-line through a web interface is described in detail in the following README files contained on the CD-ROM's:

Some technical details

The catalogue is kept on-line on a dedicated harddisk. The server called behind the scenes is a C-program written at ESO. This program does not use the index files provided by the USNO but uses a single index file instead, which has been produced at ESO. This index file contains all information needed to access the complete catalogue in chunks of 50.000 objects or less. The USNO index in contrary is built up as a set of files (one for each data file) and they have a fixed spacing in RA of 0.25 h. The number of stars in a chunk of 0.25 h x 7.5 deg might be rather high at low galactic latitudes and thus the access in those regions might take a long time just to retrieve some stars. This was the main reason for us to produce a new index file.

Additions to the data contained in the catalogue

The output of the server is slightly modified with respect to the data contained in the catalogue. The most obvious difference is the existence of an ID. This ID-number is an artificial unique number built up by a zone number and a running number in that zone (similar to the numbering scheme used with the GSC). The zone numbers are build as a 4 digit string from 0000 to 1725 representing the distance in 0.1deg to the South Pole (step widht is 75). These zone numbers are derived from the original splitting of the catalogue. The running numbers are build as a 8 digit string (with leading zeros), they represent the number of the object in the respective zone (i.e. file).

The column 'gsc', if present, contains a '+' for objects which are also in the GSC and a '-' for all other objects. This is just the opposit of what is contained in the catalogue, but it appears more logic.

There are two additional columns at the right of the output table containing the distance to the center in arcmin and the position angle (north by east).


Send comments to Andreas Wicenec <awicenec@eso.org> .
Last update: Apr 10, 1997