Observations of the BLAZAR 3C 66A with the MAGIC telescopes in stereoscopic mode
| 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 | López Moya, Marcos | |
| dc.contributor.author | Miranda Pantoja, José Miguel | |
| dc.contributor.author | Nieto Castaño, Daniel | |
| dc.date.accessioned | 2023-06-20T03:34:06Z | |
| dc.date.available | 2023-06-20T03:34:06Z | |
| dc.date.issued | 2011-01-10 | |
| dc.description | © The American Astronomical Society. Supported by INFN Padova, Italy.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, 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 data were obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA's Goddard Space Flight Center. | |
| dc.description.abstract | We report new observations of the intermediate-frequency peaked BL Lacertae object 3C 66A with the MAGIC telescopes. The data sample we use were taken in 2009 December and 2010 January, and comprises 2.3 hr of good quality data in stereoscopic mode. In this period, we find a significant signal from the direction of the blazar 3C 66A. The new MAGIC stereoscopic system is shown to play an essential role for the separation between 3C 66A and the nearby radio galaxy 3C 66B, which is at a distance of only 6'. The derived integral flux above 100 GeV is 8.3% of the Crab Nebula flux and the energy spectrum is reproduced by a power law of photon index 3.64 +/- 0.39(stat) +/- 0.25(sys). Within errors, this is compatible with the one derived by VERITAS in 2009. From the spectra corrected for absorption by the extragalactic background light, we only find small differences between the four models that we applied, and constrain the redshift of the blazar to z < 0.68. | |
| 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 | INFN Padova, Italy | |
| dc.description.sponsorship | German BMBF | |
| dc.description.sponsorship | German MPG | |
| dc.description.sponsorship | Italian INFN | |
| dc.description.sponsorship | Swiss National Fund SNF | |
| dc.description.sponsorship | Spanish MICINN | |
| dc.description.sponsorship | Marie Curie program | |
| dc.description.sponsorship | Spanish Consolider-Ingenio 2010 programme | |
| dc.description.sponsorship | Bulgarian NSF | |
| dc.description.sponsorship | Academy of Finland | |
| dc.description.sponsorship | YIP of the Helmholtz Gemeinschaft | |
| dc.description.sponsorship | DFG Cluster of Excellence "Origin and Structure of the Universe" | |
| dc.description.sponsorship | Polish MNiSzW | |
| dc.description.status | pub | |
| dc.eprint.id | https://eprints.ucm.es/id/eprint/22179 | |
| dc.identifier.doi | 10.1088/0004-637X/726/2/58 | |
| dc.identifier.issn | 0004-637X | |
| dc.identifier.officialurl | http://dx.doi.org/10.1088/0004-637X/726/2/58 | |
| dc.identifier.relatedurl | http://iopscience.iop.org | |
| dc.identifier.relatedurl | http://arxiv.org/abs/1010.0550 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.14352/43901 | |
| dc.issue.number | 2 | |
| dc.journal.title | Astrophysical journal | |
| dc.language.iso | eng | |
| dc.publisher | IOP Publishing | |
| 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.cdu | 539.1 | |
| dc.subject.keyword | BL Lacertae objects | |
| dc.subject.keyword | Extragalactic Background Light | |
| dc.subject.keyword | High-Energy Emission | |
| dc.subject.keyword | Gamma-Ray Emission | |
| dc.subject.keyword | Cherenkov Telescope | |
| dc.subject.keyword | Proton Blazar | |
| dc.subject.keyword | LAC Objects | |
| dc.subject.keyword | TEV Blazars | |
| dc.subject.keyword | X-Ray | |
| dc.subject.keyword | Spectra. | |
| dc.subject.ucm | Electrónica (Física) | |
| dc.subject.ucm | Electricidad | |
| dc.subject.ucm | Física nuclear | |
| dc.subject.unesco | 2202.03 Electricidad | |
| dc.subject.unesco | 2207 Física Atómica y Nuclear | |
| dc.title | Observations of the BLAZAR 3C 66A with the MAGIC telescopes in stereoscopic mode | |
| dc.type | journal article | |
| dc.volume.number | 726 | |
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