Name of the Speaker(s): Hidetoshi Kubo
Institution: University of Tokyo
Title of the communication:
X-ray observations of blazars with ASCA
Preliminary abstract:
We have analyzed 15 blazars observed with ASCA since the launch in 1993.
A half of the observations were conducted in the multiwavelength campaigns.
GeV gamma-ray emission has been detected from 9 of them.
The synchrotron process by the relativistic electrons and
the Comptonization of the synchrotron photons are thought to be
the important radiation processes from blazars.
The X-ray band is the "bridge" between the synchrotron and Compton spectrum.
Therefore X-ray observation is crucial to study
the mechanism of emission extending up to GeV or TeV gamma-rays.
In this paper we present the observed properties of blazars in keV regime and
its relation to other wavelength.