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Simultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008

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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.accessioned2023-06-20T03:34:36Z
dc.date.available2023-06-20T03:34:36Z
dc.date.issued2010-06
dc.description© ESO 2010. The MAGIC collaboration would like to thank the Instituto de Astrofisica de Canarias for the excellent working condition at the Observatorio del Roque de los Muchachos at La Palma. Major support from Germany's Bundesministerium fur Bildung, Wissenschaft, Forschung und Technologie and Max-Planck-Gesellschaft, Italy's Istituto Nazionale di Fisica Nucleare (INFN) and Istituto Nazionale di Astrofisica (INAF), and Spain's Ministerio de Ciencia e Innovacion is gratefully acknowledged. The work was also supported by Switzerland's ETH Research grant TH34/043, Poland's Ministertwo Nauki i Szkolnictwa Wyzszego grant N N203 390834, and Germany's Young Investigator Program of the Helmholtz Gemeinschaft. This work was also supported by Georgian National Science Foundation grant GNSF/ST07/4-180. EP acknowledges support from the Italian Space Agency through grants ASI-INAF I/023/05/0 and ASI I/088/06/0. N.M. would like to thank to C.W. Danforth for the private communication regarding the newly estimated redshift of the source.
dc.description.abstractThe blazar PG 1553+113 is a well known TeV gamma-ray emitter. In this paper we determine its spectral energy distribution through simultaneous multi-frequency data to study its emission processes. An extensive campaign was carried out between March and April 2008, where optical, X-ray, high-energy (HE) gamma-ray, and very-high-energy (VHE) gamma-ray data were obtained with the KVA, Abastumani, REM, RossiXTE/ASM, AGILE and MAGIC telescopes, respectively. We combine the data to derive the source's spectral energy distribution and interpret its double-peaked shape within the framework of a synchrotron self-Compton model.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipSwitzerland's ETH
dc.description.sponsorshipPoland's Ministertwo Nauki i Szkolnictwa Wyzszego
dc.description.sponsorshipHelmholtz Gemeinschaft
dc.description.sponsorshipGeorgian National Science Foundation
dc.description.sponsorshipItalian Space Agency
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22314
dc.identifier.doi10.1051/0004-6361/200913607
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://dx.doi.org/10.1051/0004-6361/200913607
dc.identifier.relatedurlhttp://www.aanda.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43929
dc.journal.titleAstronomy & Astrophysics
dc.language.isoeng
dc.publisherEDP Sciencies
dc.relation.projectIDTH34/043
dc.relation.projectIDN203 390834
dc.relation.projectIDGNSF/ST07/4-180
dc.relation.projectIDASI-INAF I/023/05/0
dc.relation.projectIDASI I/088/06/0
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordBL-Lacertae Objects
dc.subject.keywordMagic Telescope
dc.subject.keywordVRI Photometry
dc.subject.keywordSky Survey
dc.subject.keywordEmission
dc.subject.keywordEnergy
dc.subject.keywordSpectroscopy
dc.subject.keywordPG-1553+113
dc.subject.keywordAbsorption
dc.subject.keywordSpectra.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleSimultaneous multi-frequency observation of the unknown redshift blazar PG 1553+113 in March-April 2008
dc.typejournal article
dc.volume.number515
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