Discovery of VHE gamma-ray emission from the BL Lacertae object B3 2247+381 with the MAGIC telescopes
dc.contributor.author | Antoranz Canales, Pedro | |
dc.contributor.author | Barrio Uña, Juan Abel | |
dc.contributor.author | Contreras González, José Luis | |
dc.contributor.author | Fonseca González, María Victoria | |
dc.contributor.author | Miranda Pantoja, José Miguel | |
dc.contributor.author | Scapin, Valeria | |
dc.date.accessioned | 2023-06-20T03:32:41Z | |
dc.date.available | 2023-06-20T03:32:41Z | |
dc.date.issued | 2012-03 | |
dc.description | © ESO 2012. We would like to 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, the Swiss National Fund SNF, and the Spanish MICINN is gratefully acknowledged. This work was also supported by the Marie Curie program, by the CPAN CSD2007-00042 and MultiDark CSD2009-00064 projects of the Spanish Consolider-Ingenio 2010 programme, by grant DO02-353 of the Bulgarian NSF, by grant 127740 of the Academy of Finland, by the YIP of the Helmholtz Gemeinschaft, by the DFG Cluster of Excellence "Origin and Structure of the Universe", and by the Polish MNiSzW Grant N N203 390834. The Fermi-LAT Collaboration acknowledges support from a number of agencies and institutes for both development and the operation of the LAT as well as scientific data analysis. These include NASA and DOE in the United States, CEA/Irfu and IN2P3/CNRS in France, ASI and INFN in Italy, MEXT, KEK, and JAXA in Japan, and the K. A. Wallenberg Foundation, the Swedish Research Council and the National Space Board in Sweden. Additional support from INAF in Italy and CNES in France for science analysis during the operations phase is also gratefully acknowledged. We gratefully acknowledge N. Gehrels for approving this set of ToOs and the entire Swift team, the duty scientists and science planners for the dedicated support, making these observations possible. | |
dc.description.abstract | We study the non-thermal jet emission of the BL Lac object B3 2247+381 during a high optical state. Methods. The MAGIC telescopes observed the source during 13 nights between September 30th and October 30th 2010, collecting a total of 14.2 h of good quality very high energy (VHE) gamma-ray data. Simultaneous multiwavelength data was obtained with X-ray observations by the Swift satellite and optical R-band observations at the KVA-telescope. We also use high energy gamma-ray (HE, 0.1-100GeV) data from the Fermi satellite. Results. The BL Lac object B3 2247+381 (z = 0.119) was detected, for the first time, at VHE gamma-rays at a statistical significance of 5.6 sigma. A soft VHE spectrum with a photon index of -3.2 +/- 0.6 was determined. No significant short term flux variations were found. We model the spectral energy distribution using a one-zone SSC-model, which can successfully describe our data. | |
dc.description.department | Depto. de Estructura de la Materia, Física Térmica y Electrónica | |
dc.description.faculty | Fac. de Ciencias Físicas | |
dc.description.refereed | TRUE | |
dc.description.sponsorship | German MPG | |
dc.description.sponsorship | Swiss National Fund SNF | |
dc.description.sponsorship | Italian INFN | |
dc.description.sponsorship | Spanish MICINN | |
dc.description.sponsorship | Marie Curie program | |
dc.description.sponsorship | CPAN | |
dc.description.sponsorship | MultiDark project of the Spanish Consolider-Ingenio programme | |
dc.description.sponsorship | Bulgarian NSF | |
dc.description.sponsorship | Academy of Finland | |
dc.description.sponsorship | YIP of the Helmholtz Gemeinschaft | |
dc.description.sponsorship | DFG | |
dc.description.sponsorship | Polish MNiSzW | |
dc.description.status | pub | |
dc.eprint.id | https://eprints.ucm.es/id/eprint/21332 | |
dc.identifier.doi | 10.1051/0004-6361/201117967 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.relatedurl | http://arxiv.org/abs/1201.2634 | |
dc.identifier.uri | https://hdl.handle.net/20.500.14352/43812 | |
dc.journal.title | Astronomy & Astrophysics | |
dc.language.iso | eng | |
dc.publisher | EDP Sciencies | |
dc.relation.projectID | CSD2007-00042 | |
dc.relation.projectID | CSD2009-00064 | |
dc.relation.projectID | DO02-353 | |
dc.relation.projectID | 127740 | |
dc.relation.projectID | N N203 390834 | |
dc.rights.accessRights | open access | |
dc.subject.cdu | 537 | |
dc.subject.keyword | Extragalactic Background Light | |
dc.subject.keyword | Large-Area Telescope | |
dc.subject.keyword | Mission | |
dc.subject.keyword | Bepposax | |
dc.subject.keyword | Spectra | |
dc.subject.keyword | Catalog | |
dc.subject.keyword | Blazars | |
dc.subject.keyword | Nuclei | |
dc.subject.keyword | Sample | |
dc.subject.keyword | Quasar. | |
dc.subject.ucm | Electrónica (Física) | |
dc.subject.ucm | Electricidad | |
dc.subject.unesco | 2202.03 Electricidad | |
dc.title | Discovery of VHE gamma-ray emission from the BL Lacertae object B3 2247+381 with the MAGIC telescopes | |
dc.type | journal article | |
dc.volume.number | 539 | |
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