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Conference Paper: On the highest energy emission from millisecond pulsars

TitleOn the highest energy emission from millisecond pulsars
Authors
Saz Parkinson, PMBelfiore, AFidalgo, DCClark, CJKerr, MNieder, L
Issue Date2017
PublisherScuola Internazionale Superiore di Studi Avanzati (S I S S A). The Proceedings' web site is located at http://pos.sissa.it
Citation
7th International Fermi Symposium (IFS2017), Garmisch-Partenkirchen, Germany, 15–20 October 2017. In PoS - Proceedings of Science, 2017, v. 312 How to Cite?
DOI: http://dx.doi.org/10.22323/1.312.0008
AbstractFermi has detected over 200 pulsars above 100 MeV. In a previous work, using 3 years of LAT data (1FHL catalog) we reported that 28 of these pulsars show emission above 10 GeV; only three of these, however, were millisecond pulsars. The recently-released Third Catalog of Hard Fermi-LAT Sources (3FHL) contains over 1500 sources showing emission above 10 GeV, 17 of which are associated with gamma-ray millisecond pulsars. Using three times as much data as in our previous study (1FHL), we report on a systematic analysis of these 17 pulsars to determine the highest energy (pulsed) emission from millisecond pulsars and discuss the best possible candidates for follow-up observations with ground based TeV instruments (HESS, MAGIC, VERITAS, and the upcoming CTA).
DescriptionSession Pulsars - Pulsars / 117
Persistent Identifierhttp://hdl.handle.net/10722/267679
ISSN
1824-8039
2023 SCImago Journal Rankings: 0.122

 

DC FieldValueLanguage
dc.contributor.authorSaz Parkinson, PM-
dc.contributor.authorBelfiore, A-
dc.contributor.authorFidalgo, DC-
dc.contributor.authorClark, CJ-
dc.contributor.authorKerr, M-
dc.contributor.authorNieder, L-
dc.date.accessioned2019-02-27T07:40:36Z-
dc.date.available2019-02-27T07:40:36Z-
dc.date.issued2017-
dc.identifier.citation7th International Fermi Symposium (IFS2017), Garmisch-Partenkirchen, Germany, 15–20 October 2017. In PoS - Proceedings of Science, 2017, v. 312-
dc.identifier.issn1824-8039-
dc.identifier.urihttp://hdl.handle.net/10722/267679-
dc.descriptionSession Pulsars - Pulsars / 117-
dc.description.abstractFermi has detected over 200 pulsars above 100 MeV. In a previous work, using 3 years of LAT data (1FHL catalog) we reported that 28 of these pulsars show emission above 10 GeV; only three of these, however, were millisecond pulsars. The recently-released Third Catalog of Hard Fermi-LAT Sources (3FHL) contains over 1500 sources showing emission above 10 GeV, 17 of which are associated with gamma-ray millisecond pulsars. Using three times as much data as in our previous study (1FHL), we report on a systematic analysis of these 17 pulsars to determine the highest energy (pulsed) emission from millisecond pulsars and discuss the best possible candidates for follow-up observations with ground based TeV instruments (HESS, MAGIC, VERITAS, and the upcoming CTA).-
dc.languageeng-
dc.publisherScuola Internazionale Superiore di Studi Avanzati (S I S S A). The Proceedings' web site is located at http://pos.sissa.it-
dc.relation.ispartofPoS - Proceedings of Science-
dc.relation.ispartof7th International Fermi Symposium (IFS2017)-
dc.titleOn the highest energy emission from millisecond pulsars-
dc.typeConference_Paper-
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hk-
dc.identifier.authoritySaz Parkinson, PM=rp01803-
dc.description.naturelink_to_OA_fulltext-
dc.identifier.doi10.22323/1.312.0008-
dc.identifier.scopuseid_2-s2.0-85041084099-
dc.identifier.hkuros290514-
dc.identifier.volume312-
dc.publisher.placeItaly-
dc.identifier.issnl1824-8039-

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