Adaptation of XMM-Newton SAS to GRID and VO architectures via web

Details Adaptation of XMM-Newton SAS to GRID and VO architectures via web Adaptation of XMM-Newton SAS to GRID and VO architectures via web

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asvo.proc..139i&link_type=abstract

Astronomical Spectroscopy and Virtual Observatory, Proceedings of the EURO-VO Workshop, held at the European Space Astronomy Cen

Astronomy and Astrophysics

Astronomy

Scientific paper

The XMM-Newton Scientific Analysis Software (SAS) is a robust software that has allowed users to produce good scientific results since the beginning of the mission. This has been possible given the SAS capability to evolve with the advent of new technologies and adapt to the needs of the scientific community. The prototype of the Remote Interface for Science Analysis (RISA) presented here, is one such example, which provides remote analysis of XMM-Newton data with access to all the existing SAS functionality, while making use of GRID computing technology. This new technology has recently emerged within the astrophysical community to tackle the ever lasting problem of computer power for the reduction of large amounts of data.

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