000417975 001__ 417975
000417975 005__ 20250717101214.0
000417975 0247_ $$2doi$$a10.1126/science.aat8123
000417975 0247_ $$2INSPIRETeX$$aAjello:2018sxm
000417975 0247_ $$2inspire$$ainspire:1706829
000417975 0247_ $$2ISSN$$a0096-3771
000417975 0247_ $$2ISSN$$a2327-7513
000417975 0247_ $$2arXiv$$aarXiv:1812.01031
000417975 0247_ $$2pmid$$apmid:30498122
000417975 0247_ $$2WOS$$aWOS:000451609000039
000417975 0247_ $$2altmetric$$aaltmetric:51967651
000417975 0247_ $$2datacite_doi$$a10.3204/PUBDB-2019-00103
000417975 0247_ $$2openalex$$aopenalex:W2903566946
000417975 037__ $$aPUBDB-2019-00103
000417975 041__ $$aEnglish
000417975 082__ $$a500
000417975 0881_ $$aarXiv:1812.01031
000417975 088__ $$2arXiv$$aarXiv:1812.01031
000417975 1001_ $$0P:(DE-HGF)0$$aAjello, M.$$b0$$eCorresponding author
000417975 245__ $$aA $\gamma$-ray determination of the Universe's star-formation history
000417975 260__ $$aCambridge, Mass.$$bMoses King$$c2018
000417975 3367_ $$2DRIVER$$aarticle
000417975 3367_ $$2DataCite$$aOutput Types/Journal article
000417975 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000417975 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1548949782_20647
000417975 3367_ $$2BibTeX$$aARTICLE
000417975 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000417975 3367_ $$00$$2EndNote$$aJournal Article
000417975 500__ $$a© The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science
000417975 520__ $$aThe light emitted by all galaxies over the history of the Universe produces the extragalactic background light (EBL) at ultraviolet, optical, and infrared wavelengths. The EBL is a source of opacity for $\gamma$ rays via photon-photon interactions, leaving an imprint in the spectra of distant $\gamma$-ray sources. We measure this attenuation using {739} active galaxies and one gamma-ray burst detected by the {\it Fermi} Large Area Telescope. This allows us to reconstruct the evolution of the EBL and determine the star-formation history of the Universe over 90\% of cosmic time. Our star-formation history is consistent with independent measurements from galaxy surveys, peaking at redshift $z\sim2$. Upper limits of the EBL at the epoch of re-ionization suggest a turnover in the abundance of faint galaxies at $z\sim 6$.
000417975 536__ $$0G:(DE-HGF)POF3-613$$a613 - Matter and Radiation from the Universe (POF3-613)$$cPOF3-613$$fPOF III$$x0
000417975 588__ $$aDataset connected to CrossRef, INSPIRE
000417975 693__ $$0EXP:(DE-H253)Fermi-20170101$$5EXP:(DE-H253)Fermi-20170101$$eThe Fermi Large Area Telescope$$x0
000417975 7001_ $$0P:(DE-HGF)0$$aHelgason, K.$$b1$$eCorresponding author
000417975 7001_ $$0P:(DE-H253)PIP1086596$$aPaliya, V.$$b2$$eCorresponding author
000417975 7001_ $$0P:(DE-HGF)0$$aFinke, J.$$b3$$eCorresponding author
000417975 7001_ $$0INSPIRE-00141394$$aDominguez, A.$$b4
000417975 7001_ $$0P:(DE-HGF)0$$aDesai, A.$$b5$$eCorresponding author
000417975 7001_ $$0P:(DE-H253)PIP1014130$$aAckermann, Markus$$b6
000417975 7001_ $$0P:(DE-H253)PIP1018733$$aBühler, Rolf$$b7
000417975 7001_ $$0P:(DE-H253)PIP1006092$$aFranckowiak, Anna$$b8
000417975 7001_ $$0P:(DE-H253)PIP1028885$$aGallardo Romero, Galo Patricio$$b9
000417975 7001_ $$0P:(DE-HGF)0$$aFermi-LAT Collaboration$$b10$$eCollaboration author
000417975 773__ $$0PERI:(DE-600)2066996-3$$a10.1126/science.aat8123$$gVol. 362, no. 6418, p. 1031 - 1034$$n6418$$p1031 - 1034$$tScience$$v362$$x0036-8075$$y2018
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.pdf$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.pdf$$yRestricted$$zStatID:(DE-HGF)0599
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.gif?subformat=icon$$xicon$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.jpg?subformat=icon-1440$$xicon-1440$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.jpg?subformat=icon-180$$xicon-180$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.jpg?subformat=icon-640$$xicon-640$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1812.01031.pdf?subformat=pdfa$$xpdfa$$yPublished on 2018-11-30. Available in OpenAccess from 2019-05-30.$$zStatID:(DE-HGF)0510
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.gif?subformat=icon$$xicon$$yRestricted$$zStatID:(DE-HGF)0599
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.jpg?subformat=icon-1440$$xicon-1440$$yRestricted$$zStatID:(DE-HGF)0599
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.jpg?subformat=icon-180$$xicon-180$$yRestricted$$zStatID:(DE-HGF)0599
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.jpg?subformat=icon-640$$xicon-640$$yRestricted$$zStatID:(DE-HGF)0599
000417975 8564_ $$uhttps://bib-pubdb1.desy.de/record/417975/files/1031.full.pdf?subformat=pdfa$$xpdfa$$yRestricted$$zStatID:(DE-HGF)0599
000417975 909CO $$ooai:bib-pubdb1.desy.de:417975$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000417975 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086596$$aExternes Institut$$b2$$kExtern
000417975 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1014130$$aDeutsches Elektronen-Synchrotron$$b6$$kDESY
000417975 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1018733$$aDeutsches Elektronen-Synchrotron$$b7$$kDESY
000417975 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1006092$$aDeutsches Elektronen-Synchrotron$$b8$$kDESY
000417975 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1028885$$aDeutsches Elektronen-Synchrotron$$b9$$kDESY
000417975 9131_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
000417975 9141_ $$y2018
000417975 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000417975 915__ $$0StatID:(DE-HGF)1050$$2StatID$$aDBCoverage$$bBIOSIS Previews
000417975 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search
000417975 915__ $$0StatID:(DE-HGF)1040$$2StatID$$aDBCoverage$$bZoological Record
000417975 915__ $$0StatID:(DE-HGF)0530$$2StatID$$aEmbargoed OpenAccess
000417975 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bSCIENCE : 2017
000417975 915__ $$0StatID:(DE-HGF)1060$$2StatID$$aDBCoverage$$bCurrent Contents - Agriculture, Biology and Environmental Sciences
000417975 915__ $$0StatID:(DE-HGF)1030$$2StatID$$aDBCoverage$$bCurrent Contents - Life Sciences
000417975 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000417975 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000417975 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000417975 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC
000417975 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences
000417975 915__ $$0StatID:(DE-HGF)0310$$2StatID$$aDBCoverage$$bNCBI Molecular Biology Database
000417975 915__ $$0StatID:(DE-HGF)0430$$2StatID$$aNational-Konsortium
000417975 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz
000417975 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000417975 915__ $$0StatID:(DE-HGF)9940$$2StatID$$aIF >= 40$$bSCIENCE : 2017
000417975 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List
000417975 9201_ $$0I:(DE-H253)ZEU-EXP_AT-20120731$$kZEU-EXP/AT$$lAstroteilchenphysik$$x0
000417975 980__ $$ajournal
000417975 980__ $$aVDB
000417975 980__ $$aUNRESTRICTED
000417975 980__ $$areport
000417975 980__ $$aI:(DE-H253)ZEU-EXP_AT-20120731
000417975 9801_ $$aFullTexts