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dc.contributor.authorHall, T. A.
dc.contributor.authorBond, I. H.
dc.contributor.authorBradbury, S. M.
dc.contributor.authorBuckley, J. H.
dc.contributor.authorCarson, M. J.
dc.contributor.authorCarter‐Lewis, D. A.
dc.contributor.authorCatanese, M.
dc.contributor.authorDunlea, S.
dc.contributor.authorD’Vali, M.
dc.contributor.authorFegan, D. J.
dc.contributor.authorFegan, S. J.
dc.contributor.authorFinley, J. P.
dc.contributor.authorGaidos, J. A.
dc.contributor.authorGillanders, G. H.
dc.contributor.authorHillas, A. M.
dc.contributor.authorHoran, D.
dc.contributor.authorKertzman, M.
dc.contributor.authorKieda, D.
dc.contributor.authorKildea, J.
dc.contributor.authorKnapp, J.
dc.contributor.authorKrennrich, F.
dc.contributor.authorLang, M. J.
dc.contributor.authorLeBohec, S.
dc.contributor.authorLessard, R.
dc.contributor.authorLloyd‐Evans, J.
dc.contributor.authorMcKernan, B.
dc.contributor.authorMoriarty, P.
dc.contributor.authorMuller, D.
dc.contributor.authorOng, R.
dc.contributor.authorQuinn, J.
dc.contributor.authorReynolds, P. T.
dc.contributor.authorRose, H. J.
dc.contributor.authorSembroski, G. H.
dc.contributor.authorSwordy, S. P.
dc.contributor.authorVassiliev, V. V.
dc.contributor.authorWeekes, T. C.
dc.date.accessioned2018-08-24T08:25:03Z
dc.date.available2018-08-24T08:25:03Z
dc.date.issued2003-02-01
dc.identifier.citationHall, T. A. Bond, I. H.; Bradbury, S. M.; Buckley, J. H.; Carson, M. J.; Carter‐Lewis, D. A.; Catanese, M.; Dunlea, S.; D’Vali, M.; Fegan, D. J.; Fegan, S. J.; Finley, J. P.; Gaidos, J. A.; Gillanders, G. H.; Hillas, A. M.; Horan, D.; Kertzman, M.; Kieda, D.; Kildea, J.; Knapp, J.; Krennrich, F.; Lang, M. J.; LeBohec, S.; Lessard, R.; Lloyd‐Evans, J.; McKernan, B.; Moriarty, P.; Muller, D.; Ong, R.; Quinn, J.; Reynolds, P. T.; Rose, H. J.; Sembroski, G. H.; Swordy, S. P.; Vassiliev, V. V.; Weekes, T. C. (2003). Search for tev emissions from pulsars in binary systems. The Astrophysical Journal 583 (2), 853-860
dc.identifier.issn0004-637X,1538-4357
dc.identifier.urihttp://hdl.handle.net/10379/9264
dc.description.abstractA survey of binary systems containing pulsars was conducted, with the intention of detecting Galactic sources of very high energy gamma-ray emission. Observations were carried out with the Whipple 10 m imaging atmospheric Cerenkov telescope. Standard analysis techniques were applied to these sources to search for steady, unpulsed emission. Periodic tests were also performed to search for emission correlated with both the orbital and spin phases, where appropriate. Analyses indicate that the binaries in this study do not emit detectable levels of very high energy photons within the sensitivity of our instrument. The flux upper limits presented here fail to seriously constrain emission models.
dc.publisherIOP Publishing
dc.relation.ispartofThe Astrophysical Journal
dc.subjectgamma rays : observations
dc.subjectpulsars : general
dc.subjectgamma-ray emission
dc.subjectsource 2cg 135+01
dc.subjectx-ray
dc.subjectmillisecond pulsars
dc.subjectegret catalog
dc.subjectcentaurus x-3
dc.subjectpsr 1957+20
dc.subjectradiation
dc.subjectlsi+61-degrees-303
dc.subjectacceleration
dc.titleSearch for tev emissions from pulsars in binary systems
dc.typeArticle
dc.identifier.doi10.1086/345504
dc.local.publishedsourcehttp://iopscience.iop.org/article/10.1086/345504/pdf
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