The spectral energy distribution of gamma-faint compact radio sources

Details The spectral energy distribution of gamma-faint compact radio sources The spectral energy distribution of gamma-faint compact radio sources

2010-01-10

arxiv.org/abs/1001.1566v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

2009 Fermi Symposium, eConf Proceedings C091122

Scientific paper

MOJAVE is a VLBI program which monitors a statistically complete, radio-selected sample of 135 relativistically beamed, flat-spectrum active galactic nuclei for over more than a decade. In order to understand the high-energy behavior of this radio complete sample, we are performing Swift fill-in observations on the complete MOJAVE-I sample since 2007. The complete study of the spectral energy distribution from radio to X-ray bands on this radio-selected sample will provide us an opportunity to understand the nature of AGN. Here we present the preliminary results of the spectral energy distributions of six gamma-quiet or faint sources from this project: NRAO 140, PKS 0403-13, PKS B0422+004, PKS 0823+033, 3C 309.1, and 3C 380.

Affiliated with

Also associated with

No associations

Rating

The spectral energy distribution of gamma-faint compact radio sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The spectral energy distribution of gamma-faint compact radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectral energy distribution of gamma-faint compact radio sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-718713