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PKS 0537-286, carrying the information of the environment of SMBHs in the early Universe

We present the results of a multifrequency campaign on the high-redshift (z = 3.1) blazar PKS 0537-286. The source was observed at different epochs from 2006 to 2008 with INTEGRAL and Swift, and nearly simultaneously with ground-based near-IR/optical telescopes. The SEDs are compatible with a model based on synchrotron radiation and external inverse Compton scattering. The campaign gives an insight into the physical environment of the blazar.

preprint2009arXivOpen access
E. BottaciniM. AjelloJ. GreinerE. PianA. RauE. PalazziS. CovinG. GhiselliniT. KrühlerA. Küpcü YoldasN. CappellutiP. Afonso
astro-ph.COastro-ph.HE
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E. BottaciniM. AjelloJ. GreinerE. PianA. RauE. PalazziS. CovinG. GhiselliniT. KrühlerA. Küpcü YoldasN. CappellutiP. Afonso

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