Work is being carried out by a team ~ 30+ people from the UK, Germany, France, Italy, Spain, Belgium, Japan, USA. The SSC is led by the XMM Newton Survey Scientist, Dr. M.G. Watson (Leicester University).
SSC infrastructures are being set up at many of the collaborating institutions, but the backbone consists of 3 computer systems which host 3 crucial databases:
The OAS is responsible for cross-correlating the serendipitous source lists with an extensive list of existing catalogues (Archive Multiwavelength Database AMW-DB).
MSSL is responsible for the overall coordination of the follow-up and identification programme and for the archival of all the data from this programme (XID-DB)
SSC pipeline processing (the `PPS') starts with the raw data provided by
the XMM Newton Science Operations Centre (SOC). After pipeline processing,
the PPS products are returned to SOC for distribution to the observation
PI and storage for later public access in the XMM science archive. These
products include source lists in the EPIC images, which after cross-correlation
with existing catalogues will feed the target lists for the observing runs
of the XID programme.
modified 10th March 2000
Text based on AXIS proposal by X.Barcons and the SSC consortium.
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