High redshift blazars are among the most powerful objects in the Universe. Although they represent a significant fraction of the extragalactic hard X-ray sky, they are not commonly detected in gamma-rays. High redshift (z>2) objects represent <10 per cent of the AGN population observed by Fermi so far, and gamma-ray flaring activity from these sources is even more uncommon. The characterization of the radio-to-gamma-ray properties of high redshift blazars represent a powerful tool for the study of both the energetics of such extreme objects and the Extragalactic Background Light. We present results of a multi-band campaign on TXS 0536+145, which is the highest redshift flaring gamma-ray blazar detected so far. At the peak of the fl...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
We present the gamma-ray data of the extraordinary flaring activity above 100 MeV from the flat spec...
QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. The gravitational l...
High redshift blazars are among the most powerful objects in the Universe. Although they represent ...
High redshift blazars are among the most powerful objects in the Universe. Although they represent a...
We report results of a multiband monitoring campaign of the flat spectrum radio quasar TXS 0536+145 ...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
The detection of high-redshift (z > 3) blazars enables the study of the evolution of the most lum...
The Fermi Gamma-ray Observatory discovered about a thousand extragalactic sources emitting energy fr...
International audienceThe detection of high-redshift ($z\,\gt 3$) blazars enables the study of the e...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
International audienceThe uncharted territory of the high-redshift (z ≳ 3) universe holds the key to...
none2noWe investigate the gamma-ray and X-ray properties of the flat spectrum radio quasar PKS 2149-...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
We present the gamma-ray data of the extraordinary flaring activity above 100 MeV from the flat spec...
QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. The gravitational l...
High redshift blazars are among the most powerful objects in the Universe. Although they represent ...
High redshift blazars are among the most powerful objects in the Universe. Although they represent a...
We report results of a multiband monitoring campaign of the flat spectrum radio quasar TXS 0536+145 ...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
The detection of high-redshift (z > 3) blazars enables the study of the evolution of the most lum...
The Fermi Gamma-ray Observatory discovered about a thousand extragalactic sources emitting energy fr...
International audienceThe detection of high-redshift ($z\,\gt 3$) blazars enables the study of the e...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
International audienceThe uncharted territory of the high-redshift (z ≳ 3) universe holds the key to...
none2noWe investigate the gamma-ray and X-ray properties of the flat spectrum radio quasar PKS 2149-...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
We present the gamma-ray data of the extraordinary flaring activity above 100 MeV from the flat spec...
QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. The gravitational l...