Resources

Dynamic SEDs of southern blazars (DSSB)

In this paper I generated Fermi/LAT light curves to find time ranges of statistically constant flux using a Bayesian Blocks algorithm. In the time ranges with sufficient data, I created multiwavelength data. These dynamic SEDs were compared.

Some of the data are available at the CDS. More data are available here:

  • Fermi/LAT light curves (ASCII files, 71.7 kiB, zip): 100 MeV – 300 GeV integrated photon flux light curves
  • Multiwavelength data (ASCII files, 80.9 kiB, zip): differential energy flux spectra as a function of frequency in Hz. Frequency bins are given with lower and upper bounds. Please note that fitting was done in detector space, so fit results may vary.
  • Pivot energies (ASCII file, 2.0 kiB): pivot energies of the parabolas fitted to the SEDs, values given in keV, where first value corresponds to low energy parabola, and second value to high energy parabola.

 

AGN unified model
AGN unified model after Urry & Padovani (1995)

Feel free to use this image for non-commerical purposes. A high-res version is available here. Cite as “F. Krauß after Urry & Padovani (1995)” and/or provide the link to this image. Other versions available on request.


cta_worldxcf
Sites of the CTA. Figure not approved by CTA Consortium.

Feel free to use this image for non-commerical purposes. A high-res version is available here.