Multiwavelength monitoring of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

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dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorSitarek, J.en_US
dc.contributor.authorFallah Ramazani, Vandaden_US
dc.contributor.authorLamastra, A.en_US
dc.contributor.authorManganaro, M.en_US
dc.contributor.authorNilsson, Karien_US
dc.contributor.authorLongo, F.en_US
dc.contributor.authorde Palma, F.en_US
dc.contributor.author, MAGIC Collaborationen_US
dc.contributor.author, Fermi Large Area Telescope Collaborationen_US
dc.contributor.departmentMetsähovi Radio Observatoryen
dc.contributor.departmentDepartment of Electronics and Nanoengineeringen
dc.contributor.groupauthorAnne Lähteenmäki Groupen
dc.contributor.organizationUniversity of Łódźen_US
dc.contributor.organizationNational Institute for Astrophysics (INAF)en_US
dc.contributor.organizationUniversity of Rijekaen_US
dc.contributor.organizationUniversity of Turkuen_US
dc.contributor.organizationUniversity of Triesteen_US
dc.contributor.organizationUniversity of Salentoen_US
dc.contributor.organizationRuhr-Universität Bochumen_US
dc.date.accessioned2023-01-18T09:21:33Z
dc.date.available2023-01-18T09:21:33Z
dc.date.issued2022-03-18en_US
dc.descriptionFunding Information: We acknowledge the support from the agencies and organizations listed here: https://magic.mpp.mpg.de/acknowledgments_ICRC2021 The Fermi-LAT Collaboration acknowledges support for LAT development, operation and data analysis from NASA and DOE (United States), CEA/Irfu and IN2P3/CNRS (France), ASI and INFN (Italy), MEXT, KEK, and JAXA (Japan), and the K.A. Wallenberg Foundation, the Swedish Research Council and the National Space Board (Sweden). Science analysis support in the operations phase from INAF (Italy) and CNES (France) is also gratefully acknowledged. This work performed in part under DOE Contract DE-AC02-76SF00515. Funding Information: We acknowledge the support from the agencies and organizations listed here: https:// magic.mpp.mpg.de/acknowledgments_ICRC2021 The Fermi-LAT Collaboration acknowledges support for LAT development, operation and data analysis from NASA and DOE (United States), CEA/Irfu and IN2P3/CNRS (France), ASI and INFN (Italy), MEXT, KEK, and JAXA (Japan), and the K.A. Wallenberg Foundation, the Swedish Research Council and the National Space Board (Sweden). Science analysis support in the operations phase from INAF (Italy) and CNES (France) is also gratefully acknowledged. This work performed in part under DOE Contract DE-AC02-76SF00515. Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
dc.description.abstractQSO B0218+357 is currently the only gravitationally lensed source from which very-high-energy (VHE, &100GeV) gamma-ray emission has been detected. We report the multiwavelength monitoring observations of this source performed between 2016 and 2020 in radio interferometry, optical, X-ray and gamma-ray bands. During the monitoring individual flares and hints of enhanced states in optical, X-ray and GeV bands have been observed, and the simultaneous data taken by the MAGIC telescopes allow us to search for the VHE gamma-ray emission associated with these events.en
dc.description.versionPeer revieweden
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationSitarek, J, Fallah Ramazani, V, Lamastra, A, Manganaro, M, Nilsson, K, Longo, F, de Palma, F, MAGIC Collaboration & Fermi Large Area Telescope Collaboration 2022, 'Multiwavelength monitoring of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020', POS Proceedings of Science, vol. 395, 819. < https://pos.sissa.it/395/819/pdf >en
dc.identifier.issn1824-8039
dc.identifier.otherPURE UUID: 3dac266c-be05-424c-b63e-02b2a45826eeen_US
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/3dac266c-be05-424c-b63e-02b2a45826eeen_US
dc.identifier.otherPURE LINK: https://pos.sissa.it/395/819/pdf
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/97452185/ICRC2021_819.pdf
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/118834
dc.identifier.urnURN:NBN:fi:aalto-202301181190
dc.language.isoenen
dc.publisherScuola Internazionale Superiore di Studi Avanzati (SISSA)
dc.relation.fundinginfoWe acknowledge the support from the agencies and organizations listed here: https://magic.mpp.mpg.de/acknowledgments_ICRC2021 The Fermi-LAT Collaboration acknowledges support for LAT development, operation and data analysis from NASA and DOE (United States), CEA/Irfu and IN2P3/CNRS (France), ASI and INFN (Italy), MEXT, KEK, and JAXA (Japan), and the K.A. Wallenberg Foundation, the Swedish Research Council and the National Space Board (Sweden). Science analysis support in the operations phase from INAF (Italy) and CNES (France) is also gratefully acknowledged. This work performed in part under DOE Contract DE-AC02-76SF00515. We acknowledge the support from the agencies and organizations listed here: https:// magic.mpp.mpg.de/acknowledgments_ICRC2021 The Fermi-LAT Collaboration acknowledges support for LAT development, operation and data analysis from NASA and DOE (United States), CEA/Irfu and IN2P3/CNRS (France), ASI and INFN (Italy), MEXT, KEK, and JAXA (Japan), and the K.A. Wallenberg Foundation, the Swedish Research Council and the National Space Board (Sweden). Science analysis support in the operations phase from INAF (Italy) and CNES (France) is also gratefully acknowledged. This work performed in part under DOE Contract DE-AC02-76SF00515.
dc.relation.ispartofseriesPOS Proceedings of Scienceen
dc.relation.ispartofseriesVolume 395en
dc.rightsopenAccessen
dc.titleMultiwavelength monitoring of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020en
dc.typeA4 Artikkeli konferenssijulkaisussafi
dc.type.versionpublishedVersion

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