7–11 Aug 2017
Columbus, Ohio, USA
US/Eastern timezone

Gamma-ray and optical polarimetric monitoring of GeV bright blazars

8 Aug 2017, 16:00
15m
Corinthian Room (The Athenaeum)

Corinthian Room

The Athenaeum

Oral Gamma rays Gamma rays

Speaker

Dr Ryosuke Itoh (Tokyo Institute of technology)

Description

Blazars are thought to possess a relativistic jet that is pointing toward the direction of the Earth and the effect of relativistic beaming enhances its apparent brightness. Although numerous measurements have been performed, the mechanisms behind jet variability, creation, and composition are still debated.

We performed simultaneous gamma-ray and optical photopolarimetry observations
of 45 blazars with Fermi/LAT and Kanata telescope between 2008 July and 2014 December to investigate the mechanisms of variability and search for a basic relation between the several subclasses of blazars. Consequently, we found that a correlation between the gamma-ray and optical flux might be related to gamma-ray luminosity and the maximum polarization degree might be related to gamma-ray luminosity or the ratio of gamma-ray to optical flux. These results imply that low gamma-ray luminosity blazars emit from multiple regions.

Author

Dr Ryosuke Itoh (Tokyo Institute of technology)

Co-authors

Prof. Yasushi Fukazawa (Hiroshima University) Dr Makoto Uemura (Hiroshima University) Dr Yasuyuki Tanaka (Hiroshima University)

Presentation materials