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The Possibility for The Detection of the Sub-TeV Gamma-Ray Emission from Fermi Blazars
- Source :
- Proceedings of the 12th Asia Pacific Physics Conference (APPC12).
- Publication Year :
- 2014
- Publisher :
- Journal of the Physical Society of Japan, 2014.
-
Abstract
- Measurements of the very high energy(VHE) gamma-ray flux from high-redshift blazars are useful for understanding the cosmological evolution of galaxies, because gamma-ray emission from distant blazars is affected by Extragalactic Background Light(EBL). We searched for the detectable VHE gamma-ray blazars with known redshifts using Fermi archive data and selected three high-redshift sources, PKS 0118-272(z=0.558), PKS0454-234(z=1.003) and PKS 1244-255(z=0.633).
Details
- Database :
- OpenAIRE
- Journal :
- Proceedings of the 12th Asia Pacific Physics Conference (APPC12)
- Accession number :
- edsair.doi...........fd9e0470f22d8061f00bcae84f2262cf
- Full Text :
- https://doi.org/10.7566/jpscp.1.013106