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Article: A gamma-ray determination of the Universe’s star formation history

TitleA gamma-ray determination of the Universe’s star formation history
Authors
Issue Date2018
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2018, v. 362 n. 6418, p. 1031-1035 How to Cite?
AbstractThe 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 measured this attenuation using 739 active galaxies and one gamma-ray burst detected by the Fermi Large Area Telescope. This allowed 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 ~ 2. Upper limits of the EBL at the epoch of reionization suggest a turnover in the abundance of faint galaxies at z ~ 6.
DescriptionP. M. Saz Parkinson is one of the members of The Fermi-LAT Collaboration
Persistent Identifierhttp://hdl.handle.net/10722/266101
ISSN
2023 Impact Factor: 44.7
2023 SCImago Journal Rankings: 11.902
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorThe Fermi-LAT Collaboration-
dc.contributor.authorSaz Parkinson, PM-
dc.date.accessioned2018-12-17T02:16:47Z-
dc.date.available2018-12-17T02:16:47Z-
dc.date.issued2018-
dc.identifier.citationScience, 2018, v. 362 n. 6418, p. 1031-1035-
dc.identifier.issn0036-8075-
dc.identifier.urihttp://hdl.handle.net/10722/266101-
dc.descriptionP. M. Saz Parkinson is one of the members of The Fermi-LAT Collaboration-
dc.description.abstractThe 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 measured this attenuation using 739 active galaxies and one gamma-ray burst detected by the Fermi Large Area Telescope. This allowed 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 ~ 2. Upper limits of the EBL at the epoch of reionization suggest a turnover in the abundance of faint galaxies at z ~ 6.-
dc.languageeng-
dc.publisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org-
dc.relation.ispartofScience-
dc.rightsScience. Copyright © American Association for the Advancement of Science.-
dc.rightsThis is the author’s version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in [Science Journal Title] on [Volume number and date], DOI: [insert DOI number].-
dc.titleA gamma-ray determination of the Universe’s star formation history-
dc.typeArticle-
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hk-
dc.identifier.authoritySaz Parkinson, PM=rp01803-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1126/science.aat8123-
dc.identifier.pmid30498122-
dc.identifier.scopuseid_2-s2.0-85057548351-
dc.identifier.hkuros296462-
dc.identifier.volume362-
dc.identifier.issue6418-
dc.identifier.spage1031-
dc.identifier.epage1035-
dc.identifier.isiWOS:000451609000039-
dc.publisher.placeUnited States-
dc.customcontrol.immutablecsl 181220-
dc.identifier.issnl0036-8075-

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