Add to ORKGWe present the results of a new model calculation of the gamma-ray background produced by unresolved blazars, using the second EGRET catalogue and taking account of flaring. These results are compared to the preliminary gamma-ray background spectrum reported recently by the EGRET team. We find that blazars can account for the entire extragalactic gamma-ray background observed by EGRET. In addition, the EGRET spectrum shows some evidence of a signature for the blazar background, in the form of a concavity in the spectrum
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
A study of the statistics of cosmological black-hole jet sources is applied to EGRET blazar data, an...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
The EGRET instrument on the Compton Gamma Ray Observatory (1991-2000) has positively detected high e...
. We present a model for estimating the blazar contribution to the extragalactic fl-ray background (...
The spectral shapes of the contributions of different classes of unresolved gamma-ray emitters can p...
The diffuse extragalactic gamma-ray background (EGRB) above 100 MeV encodes unique information about...
The origin of the extragalactic γ-ray background (EGB) has been debated for some time. The EGB compr...
International audienceThe origin of the extragalactic γ-ray background (EGB) has been debated for so...
We present a calculation of the blazar contribution to the extragalactic diffuse fl-ray background ...
High-energy photons from cosmological emitters suffer attenuation due to pair production interaction...
5 pages, 2 figuresThe spectral shape of the unresolved emission from different classes of gamma-ray ...
We present a comprehensive study for the gamma-ray luminosity function (GLF) of blazars and their co...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
Very high energy gamma-rays from blazars traversing cosmological distances through the metagalactic ...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
A study of the statistics of cosmological black-hole jet sources is applied to EGRET blazar data, an...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
The EGRET instrument on the Compton Gamma Ray Observatory (1991-2000) has positively detected high e...
. We present a model for estimating the blazar contribution to the extragalactic fl-ray background (...
The spectral shapes of the contributions of different classes of unresolved gamma-ray emitters can p...
The diffuse extragalactic gamma-ray background (EGRB) above 100 MeV encodes unique information about...
The origin of the extragalactic γ-ray background (EGB) has been debated for some time. The EGB compr...
International audienceThe origin of the extragalactic γ-ray background (EGB) has been debated for so...
We present a calculation of the blazar contribution to the extragalactic diffuse fl-ray background ...
High-energy photons from cosmological emitters suffer attenuation due to pair production interaction...
5 pages, 2 figuresThe spectral shape of the unresolved emission from different classes of gamma-ray ...
We present a comprehensive study for the gamma-ray luminosity function (GLF) of blazars and their co...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
Very high energy gamma-rays from blazars traversing cosmological distances through the metagalactic ...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
A study of the statistics of cosmological black-hole jet sources is applied to EGRET blazar data, an...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...