Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5 pages, 4 figures, accepted to the ApJ Letters

Scientific paper

We report the observation in the GeV band of the blazar 1ES 0229+200, which over recent years has become one the primary sources used to put constraints on the Extragalactic Background Light (EBL) and Extragalactic Magnetic Field (EGMF). We derive constraints on both the EBL and EGMF from the combined Fermi-HESS data set taking into account the direct and cascade components of the source spectrum. We show that the limit on the EBL depends on the EGMF strength and vice versa. In particular, an EBL density twice as high as that derived by Franceschini et al. (2008) is allowed if the EGMF is strong enough. On the other hand, an EGMF strength as low as 6x10^-18 G is allowed if the EBL density is at the level of the lower bound from the direct source counts. We present the combined EBL and EGMF limits on as an exclusion plot in two dimensional parameter space: EGMF strength vs. EBL density.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light 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 Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fermi/LAT observations of 1ES 0229+200: implications for extragalactic magnetic fields and background light will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-708854

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.