Preliminary results on 11-months list
A first set of plots with 11-month data is reported below (filled circles=FSRQ, empty=BLL, triangles=other AGN). These plots use only the associations from the EMS v1 with CRATES data, so it is rather heavily biased against weak and/or steep spectrum sources.
Radio luminosity distribution |
Core/total radio flux |
Core/total radio power |
|---|---|---|
|
|
|
Gamma-ray/radio flux (all sources) |
Gamma-ray/radio flux (FSRQ) |
Gamma-ray/radio flux (BLL) |
Gamma-ray index/radio lum. |
|---|---|---|---|
|
|
|
|
Preliminary results on 6-months list
We are now in the process of exploring the subject with the gamma-ray data after 6-months.
An early attempt based on the automatic source association pipeline and the preliminary automatic associations with CRATES did not result in anything meaningful because of an error in the procedure. Results from such attempt that appeared here before June 11th have thus been deleted
In this child page, please find the preliminary results presented at the Como conference on accretion/ejection in AGN (June 2009), based on the 6-months CRATES data: radio luminosity distributions, flux-flux plots, photon index-radio luminosity plot, for the sources with an association probability larger than 90%.