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Conference Paper: Fermi-LAT detection of gamma-ray pulsars above 10 GeV

TitleFermi-LAT detection of gamma-ray pulsars above 10 GeV
Authors
Saz Parkinson, PMFermiLat Collaboration
KeywordsFermi Lat
Gamma Rays - Astronomical Observations
Gamma-Ray Telescopes
Pulsars
Issue Date2012
PublisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/
Citation
AIP Conference Proceedings, 2012, v. 1505 n. 1, p. 293-296 How to Cite?
DOI: http://dx.doi.org/10.1063/1.4772255
AbstractThe Large Area Telescope (LAT) on board the Fermi satellite has detected ∼120 pulsars above 100 MeV. While most γ-ray pulsars have spectra that are well modeled by a power law with an exponential cut-off at around a few GeV, some show significant pulsed high-energy (HE, >10 GeV) emission. I present a study of HE emission from LAT γ-ray pulsars and discuss prospects for the detection of pulsations at very high energies (VHE, >100 GeV) with ground-based instruments. © 2012 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/188515
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152
ISI Accession Number ID
WOS:000312503500042
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorSaz Parkinson, PMen_US
dc.contributor.authorFermiLat Collaborationen_US
dc.date.accessioned2013-09-03T04:09:18Z-
dc.date.available2013-09-03T04:09:18Z-
dc.date.issued2012en_US
dc.identifier.citationAIP Conference Proceedings, 2012, v. 1505 n. 1, p. 293-296-
dc.identifier.issn0094-243Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/188515-
dc.description.abstractThe Large Area Telescope (LAT) on board the Fermi satellite has detected ∼120 pulsars above 100 MeV. While most γ-ray pulsars have spectra that are well modeled by a power law with an exponential cut-off at around a few GeV, some show significant pulsed high-energy (HE, >10 GeV) emission. I present a study of HE emission from LAT γ-ray pulsars and discuss prospects for the detection of pulsations at very high energies (VHE, >100 GeV) with ground-based instruments. © 2012 American Institute of Physics.en_US
dc.languageengen_US
dc.publisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/-
dc.relation.ispartofAIP Conference Proceedingsen_US
dc.subjectFermi Laten_US
dc.subjectGamma Rays - Astronomical Observationsen_US
dc.subjectGamma-Ray Telescopesen_US
dc.subjectPulsarsen_US
dc.titleFermi-LAT detection of gamma-ray pulsars above 10 GeVen_US
dc.typeConference_Paperen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1063/1.4772255en_US
dc.identifier.scopuseid_2-s2.0-84873133449en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84873133449&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume1505en_US
dc.identifier.issue1-
dc.identifier.spage293en_US
dc.identifier.epage296en_US
dc.identifier.isiWOS:000312503500042-
dc.publisher.placeUnited Statesen_US
dc.identifier.scopusauthoridSaz Parkinson, PM=8948464400en_US
dc.identifier.scopusauthoridFermiLat Collaboration=55574926300en_US
dc.identifier.issnl0094-243X-

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