A4 Vertaisarvioitu artikkeli konferenssijulkaisussa

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




Tekijätde Palma F., D'Ammando F., Barnacka A., Hada K., Sahu D.K., Lähteenmäki A., Acciari V.A., Ansoldi S., Antonelli L.A., Arbet Engels A., Artero M., Asano K., Baack D., Babić A., Baquero A., Barres de Almeida U., Barrio J.A., Batković I., Becerra González J., Bednarek W., Bellizzi L., Bernardini E., Bernardos M., Berti A., Besenrieder J., Bhattacharyya W., Bigongiari C., Biland A., Blanch O., Bökenkamp H., Bonnoli G., Bošnjak , Busetto G., Carosi R., Ceribella G., Cerruti M., Chai Y., Chilingarian A., Cikota S., Colak S.M., Colombo E., Contreras J.L., Cortina J., Covino S., D'Amico G., D'Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Delfino M., Delgado J., Delgado Mendez C., Depaoli D., Di Pierro F., Di Venere L., Do Souto Espiñeira E., Dominis Prester D., Donini A., Dorner D., Doro M., Elsaesser D., Fallah Ramazani V., Fattorini A., Fonseca M.V., Font L., Fruck C., Fukami S., Fukazawa Y., García López R.J., Garczarczyk M., Gasparyan S., Gaug M., Giglietto N., Giordano F., Gliwny P., Godinović N., Green J.G., Green D., Hadasch D., Hahn A., Heckmann L., Herrera J., Hoang J., Hrupec D., Hütten M., Inada T., Ishio K., Iwamura Y., Jiménez Martínez I., Jormanainen J., Jouvin L., Karjalainen M., Kerszberg D., Kobayashi Y., Kubo H., Kushida J., Lamastra A., Lelas D., Leone F., Lindfors E., Linhoff L., Lombardi S., Longo F., López-Coto R., López-Moya M., López-Oramas A., Loporchio S., Machado de Oliveira Fraga B., Maggio C., Majumdar P., Makariev M., Mallamaci M., Maneva G., Manganaro M., Mannheim K., Maraschi L., Mariotti M., Martínez M., Mazin D., Menchiari S., Mender S., Mićanović S., Miceli D., Miener T., Miranda J.M., Mirzoyan R., Molina E., Moralejo A., Morcuende D., Moreno V., Moretti E., Nakamori T., Nava L., Neustroev V., Nigro C., Nilsson K., Nishijima K., Noda K., Nozaki S., Ohtani Y., Oka T., Otero-Santos J., Paiano S., Palatiello M., Paneque D., Paoletti R., Paredes J.M., Pavletić L., Peñil P., Persic M., Pihet M., Prada Moroni P.G., Prandini E., Priyadarshi C., Puljak I., Rhode W., Ribó M., Rico J., Righi C., Rugliancich A., Sahakyan N., Saito T., Sakurai S., Satalecka K., Saturni F.G., Schleicher B., Schmidt K., Schweizer T., Sitarek J., Šnidarić I., Sobczynska D., Spolon A., Stamerra A., Strišković J., Strom D., Strzys M., Suda Y., Surić T., Takahashi M., Takeishi R., Tavecchio F., Temnikov P., Terzić T., Teshima M., Tosti L., Truzzi S., Tutone A., Ubach S., van Scherpenberg J., Vanzo G., Vazquez Acosta M., Ventura S., Verguilov V., Vigorito C.F., Vitale V., Vovk I., Will M., Wunderlich C., Yamamoto T., Zarić D.

ToimittajaN/A

Konferenssin vakiintunut nimiInternational Cosmic Ray Conference

KustantajaSissa Medialab Srl

Julkaisuvuosi2022

JournalPOS Proceedings of Science

Kokoomateoksen nimi37th International Cosmic Ray Conference (ICRC2021)

Tietokannassa oleva lehden nimiProceedings of Science

Sarjan nimiPOS Proceedings of Science

Vuosikerta395

Aloitussivu819

ISSN1824-8039

DOIhttps://doi.org/10.22323/1.395.0819

Verkko-osoitehttps://pos.sissa.it/395/819

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/178545593


Tiivistelmä

QSO 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.


Ladattava julkaisu

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Last updated on 2025-27-03 at 21:57