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Search for very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the Magic telescope

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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.accessioned2023-06-20T03:34:40Z
dc.date.available2023-06-20T03:34:40Z
dc.date.issued2010-02-10
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 German BMBF and MPG, the Italian INFN, and the Spanish MICINN is gratefully acknowledged. This work was also supported by ETH Research Grant TH 34/043, by the Polish MNiSzW Grant NN203 390834, and by theYIP of the Helmholtz Gemeinschaft. We thank D.A. Smith and the Nancay Radio Observatory operated by the Paris Observatory (associated with the French CNRS) for the ephemerides of PSR J0218+4232, and also S. M. Ransom (NRAO) for the ephemerides of PSR J0205+6449.
dc.description.abstractThe MAGIC collaboration has searched for high-energy gamma-ray emission of some of the most promising pulsar candidates above an energy threshold of 50 GeV, an energy not reachable up to now by other ground-based instruments. Neither pulsed nor steady gamma-ray emission has been observed at energies of 100 GeV from the classical radio pulsars PSR J0205+6449 and PSR J2229+6114 (and their nebulae 3C58 and Boomerang, respectively) and the millisecond pulsar PSR J0218+4232. Here, we present the flux upper limits for these sources and discuss their implications in the context of current model predictions.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipGerman BMBF
dc.description.sponsorshipGerman MPG
dc.description.sponsorshipItalian INFN
dc.description.sponsorshipSpanish MICINN
dc.description.sponsorshipETH Research Grant
dc.description.sponsorshipPolish MNiSzW
dc.description.sponsorshipYIP of the Helmholtz Gemeinschaft
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22349
dc.identifier.doi10.1088/0004-637X/710/1/828
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1088/0004-637X/710/1/828
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43933
dc.issue.number1
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.final835
dc.page.initial828
dc.publisherIOP Publishing
dc.relation.projectIDTH 34/043
dc.relation.projectIDNN203 390834
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordLarge-Area Telescope
dc.subject.keywordMilliseconf Pulsar
dc.subject.keywordX-Ray
dc.subject.keywordPSR J0218+4232
dc.subject.keywordCrab Pulsar
dc.subject.keywordSource List
dc.subject.keyword3C 58
dc.subject.keywordDiscovery
dc.subject.keywordEgret
dc.subject.keywordRadiation.
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 very high energy gamma-ray emission from pulsar-pulsar wind nebula systems with the Magic telescope
dc.typejournal article
dc.volume.number710
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