SED Computation at a Glance

For each source, only the 3 (at most) SEDs with a probability greater than 1% will be considered.

• Select Vizier catalogues overlapping with the XMM catalogue footprint and covering all spectral bands.
• Filter the observations (e.g., LMC/SMC, M31 .. removed).
• Group observations according to the catalogs that cover them.§
• Compute different correlation patterns for each source with the Arches tool. Each pattern is associated with a probability.
• Keep the 3 (at most) most likely correlation patterns.
• Compute the FITS SEDs for each selected pattern.
• Compute the plots from the FITS.
• Deploy the sedfinder API.

This page will be replaced with the XMM2Athena work package report when available.