Evidence for a cosmological effect in γ-ray spectra of BL Lacs
arXiv:1303.5923 · doi:10.1051/0004-6361/201220631
Abstract
We update the list of GeV-TeV extragalactic γ-ray sources using the 2-year catalog from the Fermi-LAT and recent results ground-based γ-ray telescopes. Breaks in the spectra between the high energy (100 MeV <E< 300 GeV) and the very high energy (E> 200 GeV) ranges, and their dependence on distance, are discussed in the context of absorption on the extragalactic background light (EBL). We calculate the size of the expected break using a model for the EBL and compare it to the data taking into account systematic uncertainties in the measurements. We develop a novel Bayeasian model to describe this dataset and use it to constrain two simple models for the EBL-induced breaks.
accepted for publication in A&A
References in corpus (7)
- MAGIC discovery of VHE Emission from the FSRQ PKS 1222+21
- The Imprint of The Extragalactic Background Light in the Gamma-Ray Spectra of Blazars
- Measurement of the extragalactic background light imprint on the spectra of the brightest blazars observed with H.E.S.S
- SN 1994W: An Interacting Supernova or Two Interacting Shells?
- Formation of hard VHE gamma-ray spectra of blazars due to internal photon-photon absorption
- Constraining blazar distances with combined Fermi and TeV data: an empirical approach
- Cascading on extragalactic background light
Cited by in corpus (34)
- Physics potential of the International Axion Observatory (IAXO)
- The extragalactic background light, the Hubble constant, and anomalies: conclusions from 20 years of TeV gamma-ray observations
- Diffuse -ray emission from misaligned active galactic nuclei
- Constraints on the Intergalactic Magnetic Field with Gamma-Ray Observations of Blazars
- Measurement of the Extragalactic Background Light using MAGIC and Fermi-LAT gamma-ray observations of blazars up to z = 1
- Active galactic nuclei at gamma-ray energies
- Diffuse -ray emission from unresolved BL Lac objects
- The 2012 flare of PG 1553+113 seen with H.E.S.S. and Fermi-LAT
- Star formation history, dust attenuation and extragalactic background light
- Spectral analysis of Fermi-LAT blazars above 50 GeV
- Gamma-rays from Blazars and the Extragalactic Background Light
- Constraints on axion-like particle properties with very high energy gamma-ray observations of Galactic sources
- F-GAMMA: Multi-frequency radio monitoring of Fermi blazars. The 2.64 to 43 GHz Effelsberg light curves from 2007-2015
- The high-energy -ray emission of AP Librae
- Bethe-Heitler cascades as a plausible origin of hard spectra in distant TeV blazars
- Anisotropy test of the axion-like particle Universe opacity effect: a case for the Cherenkov Telescope Array
- Gamma-ray Cosmology and Tests of Fundamental Physics
- Distinguishing Axion Models with IAXO
- Effect of axion-like particles on the spectrum of the extragalactic gamma-ray background
- Prospects for future very high-energy gamma-ray sky survey: impact of secondary gamma rays
- Estimation of the Extragalactic Background Light using TeV Observations of BL~Lacs
- The host galaxy and Fermi-LAT counterpart of HESS J1943+213
- Expected Signature For the Lorentz Invariance Violation Effects on Absorption
- From Radio to TeV: The surprising Spectral Energy Distribution of AP Librae
- Axion-Like Particle Searches with IACTs
- Model-independent Redshift Estimation of BL Lac Objects through VHE Observations
- Investigating the Origin of Observed Central Dips in Radial Metallicity Profiles
- Search for anomalous features in gamma-ray blazar spectra corrected for the absorption on the extragalactic background light
- Propagation of very-high-energy -rays from distant blazars
- Cherenkov telescope array extragalactic survey discovery potential and the impact of axion-like particles and secondary gamma rays
- GeV-TeV -ray energy spectral break of BL Lac objects
- Dark Matter and Fundamental Physics Searches with IACTs
- The H.E.S.S. extragalactic sky survey with the first decade of observations
- Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies