We present a measurement of the extragalactic background light (EBL) based on a joint likelihood analysis of 32 gamma-ray spectra for 12 blazars in the redshift range z = 0.03–0.944, obtained by the MAGIC telescopes and Fermi-LAT. The EBL is the part of the diffuse extragalactic radiation spanning the ultraviolet, visible, and infrared bands. Major contributors to the EBL are the light emitted by stars through the history of the Universe, and the fraction of it that was absorbed by dust in galaxies and re-emitted at longer wavelengths. The EBL can be studied indirectly through its effect on very high energy photons that are emitted by cosmic sources and absorbed via γγ interactions during their propagation across cosmological distances. We ...
International audienceContext. Cumulative optical and infrared emission from galaxies accumulated ov...
The diffuse Extragalactic Background Light (EBL) contains unique information about the epochs of for...
Abstract: The light emitted by stars and accreting compact objects through the history of the univer...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
The extragalactic background light (EBL) can be probed via the absorption imprint it leaves in the s...
The light emitted by stars and accreting compact objects through the history of the universe is enco...
The direct measurement of the extragalactic background light (EBL) is difficult at optical to infrar...
CNRS/IN2P3, F-91128 Palaiseau, France The imprint of cosmic backgrounds in the gamma ray spectra of ...
International audienceContext. Cumulative optical and infrared emission from galaxies accumulated ov...
The diffuse Extragalactic Background Light (EBL) contains unique information about the epochs of for...
Abstract: The light emitted by stars and accreting compact objects through the history of the univer...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
We present a measurement of the extragalactic background light (EBL) based on a joint likelihood ana...
The extragalactic background light (EBL) can be probed via the absorption imprint it leaves in the s...
The light emitted by stars and accreting compact objects through the history of the universe is enco...
The direct measurement of the extragalactic background light (EBL) is difficult at optical to infrar...
CNRS/IN2P3, F-91128 Palaiseau, France The imprint of cosmic backgrounds in the gamma ray spectra of ...
International audienceContext. Cumulative optical and infrared emission from galaxies accumulated ov...
The diffuse Extragalactic Background Light (EBL) contains unique information about the epochs of for...
Abstract: The light emitted by stars and accreting compact objects through the history of the univer...