A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

Probing the Diffuse Optical-IR Background with TeV Blazars Detected with the MAGIC Telescopes




TekijätElisa Prandini, Alberto Domínguez, Vandad Fallah Ramazani, Tarek Hassan, Daniel Mazin, Abelardo Moralejo, Mireia Nievas Rosillo, Gaia Vanzo, Monica Vazquez Acosta

KustantajaFRONTIERS MEDIA SA

Julkaisuvuosi2017

JournalFrontiers in Astronomy and Space Sciences

Tietokannassa oleva lehden nimiFRONTIERS IN ASTRONOMY AND SPACE SCIENCES

Lehden akronyymiFRONT ASTRON SPACE

Artikkelin numeroUNSP 50

Vuosikerta4

Numero50

Sivujen määrä5

ISSN2296-987X

eISSN2296-987X

DOIhttps://doi.org/10.3389/fspas.2017.00050

Verkko-osoitehttps://www.frontiersin.org/articles/10.3389/fspas.2017.00050/full

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/31738017


Tiivistelmä
Blazars are radio loud quasars whose jet points toward the observer. The observed emission is mostly non-thermal, dominated by the jet emission, and in some cases extends up to the very high energy gamma rays (VHE; E > 100 GeV). To date, more than 60 blazars have been detected at VHE mainly with ground-based imaging atmospheric Cherenkov telescopes (IACTs) such as MAGIC, H.E.S.S., and VERITAS. Energetic photons from a blazar may interact with the diffuse optical and IR background (the extragalactic background light, EBL) leaving an imprint on the blazar energy spectrum. This effect can be used to constrain the EBL, with basic assumptions on the intrinsic energy spectrum. Current generation of IACTs is providing valuable measurements of the EBL density and energy spectrumfromoptical to infrared frequencies. In this contribution, we present the latest results obtained with the data taken with the MAGIC telescopes: using 32 spectra from 12 blazars, the scale factor of the optical density predicted by the EBL model from Dominguez et al. (2011) is constrained to be 0.95 (+0.11, -0.12)(stat) (+0.16, -0.07)(sys), where a value of 1 means the perfect match with the model.

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