Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/150592
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dc.contributor.authorMAGIC Collaboration-
dc.contributor.authorParedes i Poy, Josep Maria-
dc.contributor.authorRibó Gomis, Marc-
dc.contributor.authorBosch i Ramon, Valentí-
dc.date.accessioned2020-02-18T16:11:35Z-
dc.date.available2020-02-18T16:11:35Z-
dc.date.issued2006-
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2445/150592-
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 γ-ray emission was detected with a significance of 5.5 σ. An integral flux above 200 GeV of (2.3 ± 0.7) × 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 -3.3 ± 0.7 has been determined. No significant flux variation was found.-
dc.format.extent4 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherInstitute of Physics (IOP)-
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1086/508020-
dc.relation.ispartofAstrophysical Journal, 2006, vol. 648, p. 105-108-
dc.relation.urihttps://doi.org/10.1086/508020-
dc.rights(c) American Astronomical Society, 2006-
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationRaigs gamma-
dc.subject.classificationObservacions astronòmiques-
dc.subject.otherGamma rays-
dc.subject.otherAstronomical observations-
dc.titleDiscovery of very high energy gamma-rays from Markarian 180 triggered by an optical outburst-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec546721-
dc.date.updated2020-02-18T16:11:35Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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