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Discovery of very high energy gamma-rays from Markarian 180 triggered by an optical outburst

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.authorLópez Moya, Marcos
dc.contributor.authorMiranda Pantoja, José Miguel
dc.date.accessioned2023-06-20T10:39:28Z
dc.date.available2023-06-20T10:39:28Z
dc.date.issued2006-09-10
dc.description© The American Astronomical Society. We would like to thank the IAC for the excellent working conditions at the ORM in La Palma. The support of the German BMBF and MPG, the Italian INFN, the Spanish CICYT, ETH research grant TH 34/04 3, and the Polish MNiI grant 1P03D01028 is gratefully acknowledged. We also thank H. D. and M. F. Aller, at the University of Michigan Radio Observatory, for providing us with the UMRAO data.
dc.description.abstractThe high-frequency-peaked BL Lacertae object Markarian 180 (Mrk 180) was observed to have an optical outburst in 2006 March, triggering a Target of Opportunity observation with the MAGIC telescope. The source was observed for 12.4 hr, and very high energy gamma-ray emission was detected with a significance of 5.5 sigma. An integral flux above 200 GeV of (2.3 +/- 0.7) x 10(-11) cm(-2) s(-1) was measured, corresponding to 11% of the Crab Nebula flux. A rather soft spectrum with a photon index of has been determined. No significant flux -3.3 x 0.7 variation was found.
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 CICYT
dc.description.sponsorshipETH
dc.description.sponsorshipPolish MNiI
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/23885
dc.identifier.doi10.1086/508020
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1086/508020
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/astro-ph/0606630
dc.identifier.urihttps://hdl.handle.net/20.500.14352/50919
dc.issue.number2 (Par
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.finalL108
dc.page.initialL105
dc.publisherIOP Publishing
dc.relation.projectIDTH 34/04 3
dc.relation.projectID1P03D01028
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordBL Lacertae Objects
dc.subject.keywordExtragalactic Background Light
dc.subject.keywordX-Ray
dc.subject.keywordMagic Telescope
dc.subject.keywordEmission
dc.subject.keywordBlazars
dc.subject.keywordSpectra
dc.subject.keywordConstraints
dc.subject.keywordCatalog
dc.subject.keyword1ES-1959+650.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleDiscovery of very high energy gamma-rays from Markarian 180 triggered by an optical outburst
dc.typejournal article
dc.volume.number648
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