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Search for VHE gamma-ray emission from the globular cluster M13 with the Magic telescope

dc.contributor.authorAntoranz Canales, Pedro
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorMiranda Pantoja, José Miguel
dc.contributor.authorNieto Castaño, Daniel
dc.date.accessioned2023-06-20T03:35:02Z
dc.date.available2023-06-20T03:35:02Z
dc.date.issued2009-09-01
dc.description© The American Astronomical Society. We thank the Instituto de Astrofisica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The support of the Spanish MICINN and MPG, the Italian INFN and Spanish MICINN is gratefully acknowledged. This work was also supported by ETH Research Grant TH 34/043, by the Polish MNiSzW Grant N N203 390834, and by the YIP of the Helmholtz Gemeinschaft.
dc.description.abstractBased on MAGIC observations from 2007 June to July, we have obtained an integral upper limit to the VHE energy emission of the globular cluster M13 of F (E > 200 GeV) < 5.1 x 10(-12) cm(-2) s(-1), and differential upper limits for E > 140 GeV. Those limits allow us to constrain the population of millisecond pulsars within M13 and to test models for acceleration of leptons inside their magnetospheres and surrounding. We conclude that in M13 either millisecond pulsars are fewer than expected or they accelerate leptons less efficiently than predicted.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipETH Research
dc.description.sponsorshipPolish MNiSzW
dc.description.sponsorshipYIP of the Helmholtz Gemeinschaft
dc.description.sponsorshipSpanish MICINN
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22723
dc.identifier.doi10.1088/0004-637X/702/1/266
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1088/0004-637X/702/1/266
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/0905.2427
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43955
dc.issue.number1
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.final269
dc.page.initial266
dc.publisherIOP Publishing
dc.relation.projectIDTH 34/043
dc.relation.projectIDN N203 390834
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordMillisecond Pulsars
dc.subject.keywordSystems
dc.subject.keywordHess.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleSearch for VHE gamma-ray emission from the globular cluster M13 with the Magic telescope
dc.typejournal article
dc.volume.number702
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relation.isAuthorOfPublication.latestForDiscovery6bc87e5f-9b77-4982-b112-0d4f8aa128d0

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