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Magic gamma-ray telescope observation of the Perseus cluster of galaxies: implications for cosmic rays, dark matter, and NGC 1275

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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.accessioned2023-06-20T03:34:37Z
dc.date.available2023-06-20T03:34:37Z
dc.date.issued2010-02-10
dc.description© The American Astronomical Society. We thank the anonymous referee for valuable comments. We thank Volker Springel for the important work on CR implementation into the GADGET code and comments on the paper. We also thank Yoel Rephaeli for the useful comments on the paper and Eugene Churazov for providing us XMM-Newton X-ray contours. 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 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, by the YIP of the Helmholtz Gemeinschaft, and by grant DO02-353 of the Bulgarian National Science Fund.
dc.description.abstractThe Perseus galaxy cluster was observed by the MAGIC Cherenkov telescope for a total effective time of 24.4 hr during 2008 November and December. The resulting upper limits on the gamma-ray emission above 100 GeV are in the range of 4.6-7.5 x 10(-12) cm(-2) s(-1) for spectral indices from -1.5 to -2.5, thereby constraining the emission produced by cosmic rays, dark matter annihilations, and the central radio galaxy NGC 1275. Results are compatible with cosmological cluster simulations for the cosmic-ray-induced gamma-ray emission, constraining the average cosmic ray-to-thermal pressure to < 4% for the cluster core region (< 8% for the entire cluster).
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.sponsorshipPolish MNiSzW
dc.description.sponsorshipHelmholtz Gemeinschaft
dc.description.sponsorshipBulgarian National Science Fund
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22316
dc.identifier.doi10.1088/0004-637X/710/1/634
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1088/0004-637X/710/1/634
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/0909.3267
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43930
dc.issue.number1
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.final647
dc.page.initial634
dc.publisherIOP Publishing
dc.relation.projectIDTH 34/043
dc.relation.projectIDN N203 390834
dc.relation.projectIDDO02-353
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordActive Galactic Nuclei
dc.subject.keywordParticle Hydrodynamics Simulations
dc.subject.keywordFlux-Limited Sample
dc.subject.keywordHard X-Ray
dc.subject.keywordMagnetic-Fields
dc.subject.keywordRadio Halos
dc.subject.keywordComa Cluster
dc.subject.keywordCosmological Simulations
dc.subject.keywordIntergalactic Medium
dc.subject.keywordHess Observations.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleMagic gamma-ray telescope observation of the Perseus cluster of galaxies: implications for cosmic rays, dark matter, and NGC 1275
dc.typejournal article
dc.volume.number710
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