Multiband Observations of the Quasar PKS 2326–502 during Active and Quiescent Gamma-Ray States in 2010–2012
العنوان: | Multiband Observations of the Quasar PKS 2326–502 during Active and Quiescent Gamma-Ray States in 2010–2012 |
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المؤلفون: | Michael Dutka, Roberto Nesci, Justin D. Finke, Joern Wilms, Bryce Carpenter, Jamie Stevens, Neil Gehrels, Eleonora Torresi, Matthias Kadler, Roopesh Ojha, Felicia Krauss, Paola Grandi, Philip G. Edwards, Cornelia Mueller, Filippo D'Ammando |
المساهمون: | ITA, USA, DEU, High Energy Astrophys. & Astropart. Phys (API, FNWI), Dutka Michael S, Carpenter Bryce D, Ojha Roopesh, Finke Justin D, DAmmando F, Kadler Matthia, Edwards Philip G, Stevens Jamie, Torresi Eleonora, Grandi Paola, Nesci Roberto, Krauß Felicia, Müller Cornelia, Wilms Joern, Gehrels Neil |
المصدر: | The Astrophysical Journal, 835, 1-10 Astrophysical Journal, 835(2):182. IOP Publishing Ltd. The Astrophysical Journal, 835, 2, pp. 1-10 The Astrophysical Journal |
سنة النشر: | 2017 |
مصطلحات موضوعية: | Astronomy, Astrophysics::High Energy Astrophysical Phenomena, galaxies: active, FOS: Physical sciences, Electron, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, X-rays: individual (PKS 2326–502), 01 natural sciences, Radio spectrum, law.invention, law, 0103 physical sciences, gamma rays: galaxie, Astrophysics::Solar and Stellar Astrophysics, Blazar, 010303 astronomy & astrophysics, GeneralLiterature_REFERENCE(e.g.,dictionaries,encyclopedias,glossaries), Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Gamma ray, Spectral density, Astronomy and Astrophysics, Quasar, quasars: individual (PKS 2326–502), Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), ultraviolet: galaxie, Spectral energy distribution, radio continuum: galaxie, Astrophysics - High Energy Astrophysical Phenomena, Flare |
الوصف: | Quasi-simultaneous observations of the Flat Spectrum Radio Quasar PKS 2326-502 were carried out in the gamma-ray, X-ray, UV, optical, near-infrared, and radio bands. Thanks to these observations we are able to characterize the spectral energy distribution of the source during two flaring and one quiescent gamma-ray states. These data were used to constrain one-zone leptonic models of the spectral energy distributions of each flare and investigate the physical conditions giving rise to them. While modeling one flare only required changes to the electron spectrum, the other flare needed changes in both the electron spectrum and the size of the emitting region with respect to the quiescent state. These results are consistent with an emerging pattern of two broad classes of flaring states seen in blazars. Comment: 18 pages, 3 figures. Accepted in the Astrophysical Journal |
وصف الملف: | application/pdf; STAMPA |
تدمد: | 0004-637X 0067-0049 0004-6361 1538-3873 1538-3881 |
الوصول الحر: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::048719dc4e3c64cf2cf62aca6874d78fTest https://doi.org/10.3847/1538-4357/835/2/182Test |
حقوق: | OPEN |
رقم الانضمام: | edsair.doi.dedup.....048719dc4e3c64cf2cf62aca6874d78f |
قاعدة البيانات: | OpenAIRE |
تدمد: | 0004637X 00670049 00046361 15383873 15383881 |
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