On the highest energy emission from millisecond pulsars

Originalpublikation

Saz Parkinson, P.M.; Belfiore, A.; Fidalgo, D.C.; Clark, C.J.; Kerr, M. et al.: On the highest energy emission from millisecond pulsars. In: Proceedings of Science 2017 (2017), Nr. October.

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Zusammenfassung:
Fermi 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 (MSPs). 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 MSPs. Using three times as much data as in our previous study (1FHL), we report on a systematic analysis of these pulsars to determine the highest energy (pulsed) emission from MSPs and discuss the best possible candidates for follow-up observations with ground-based TeV instruments (H.E.S.S., MAGIC, VERITAS, and the upcoming CTA). © Copyright owned by the author(s).
Lizenzbestimmungen: CC BY-NC-ND 4.0 Unported - https://creativecommons.org/licenses/by-nc-nd/4.0/
Publikationstyp: Article
Publikationsstatus: publishedVersion
Erstveröffentlichung: 2017
Schlagwörter (englisch): Gamma rays, Tellurium compounds, Energy emissions, Follow up, Ground based, Millisecond pulsars, Systematic analysis, Veritas, Pulsars
Fachliche Zuordnung (DDC): 530 | Physik
Kontrollierte Schlagwörter: Konferenzschrift

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