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. 2012 Nov 30;338(6111):1190-2.
doi: 10.1126/science.1227160. Epub 2012 Nov 1.

The imprint of the extragalactic background light in the gamma-ray spectra of blazars

M Ackermann  1 M AjelloA AllafortP SchadyL BaldiniJ BalletG BarbielliniD BastieriR BellazziniR D BlandfordE D BloomA W BorglandE BottaciniA BouvierJ BregeonM BrigidaP BruelR BuehlerS BusonG A CaliandroR A CameronP A CaraveoE CavazzutiC CecchiE CharlesR C G ChavesA ChekhtmanC C CheungJ ChiangG ChiaroS CipriniR ClausJ Cohen-TanugiJ ConradS CutiniF D'AmmandoF de PalmaC D DermerS W DigelE do Couto e SilvaA DomínguezP S DrellA Drlica-WagnerC FavuzziS J FeganW B FockeA FranckowiakY FukazawaS FunkP FuscoF GarganoD GasparriniN GehrelsS GermaniN GigliettoF GiordanoM GirolettiT GlanzmanG GodfreyI A GrenierJ E GroveS GuiriecM GustafssonD HadaschM HayashidaE HaysM S JacksonT JoglerJ KataokaJ KnödlsederM KussJ LandeS LarssonL LatronicoF LongoF LoparcoM N LovelletteP LubranoM N MazziottaJ E McEneryJ MehaultP F MichelsonT MizunoC MonteM E MonzaniA MorselliI V MoskalenkoS MurgiaA TramacereE NussJ GreinerM OhnoT OhsugiN OmodeiM OrientiE OrlandoJ F OrmesD PanequeJ S PerkinsM Pesce-RollinsF PironG PivatoT A PorterS RainòR RandoM RazzanoS RazzaqueA ReimerO ReimerL C ReyesS RitzA RauC RomoliM RothM Sánchez-CondeD A SanchezJ D ScargleC SgròE J SiskindG SpandreP SpinelliŁukasz StawarzD J SusonH TakahashiT TanakaJ G ThayerD J ThompsonL TibaldoM TinivellaD F TorresG TostiE TrojaT L UsherJ VandenbrouckeV VasileiouG VianelloV VitaleA P WaiteB L WinerK S WoodM Wood
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The imprint of the extragalactic background light in the gamma-ray spectra of blazars

M Ackermann et al. Science. .

Abstract

The light emitted by stars and accreting compact objects through the history of the universe is encoded in the intensity of the extragalactic background light (EBL). Knowledge of the EBL is important to understand the nature of star formation and galaxy evolution, but direct measurements of the EBL are limited by galactic and other foreground emissions. Here, we report an absorption feature seen in the combined spectra of a sample of gamma-ray blazars out to a redshift of z ∼ 1.6. This feature is caused by attenuation of gamma rays by the EBL at optical to ultraviolet frequencies and allowed us to measure the EBL flux density in this frequency band.

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