Multiwavelength variability power spectrum analysis of the blazars 3C 279 and PKS 1510–089 on multiple timescales
Author
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Goyal, Arti
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Soida, Marian
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Stawarz, Lukasz
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Wiita, Paul J.
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Nilsson, Kari
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Jorstad, Svetlana
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Marscher, Alan P.
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Aller, Margo F.
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Aller, Hugh D.
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Lähteenmäki, Anne
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Hovatta, Talvikki
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Zoła, Staszek
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Nalewajko, Krzysztof
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Tornikoski, Merja
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Tammi, Joni
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Hodges, Mark
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Kiehlmann, Sebastian
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Readhead, Anthony C. S.
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Max-Moerbeck Astudillo, Walter Kennerth
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Lindfors, Elina
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Ramazani, Vandad Fallah
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Reichart, D. E.
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Caton, D. B.
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Valverde, Janeth
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Horan, Deirdre
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Ojha, Roopesh
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Van Zyl, Pfesesani
Admission date
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2022-12-20T17:36:30Z
Available date
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2022-12-20T17:36:30Z
Publication date
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2022
Cita de ítem
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The Astrophysical Journal, 927:214 (29pp), 2022
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Identifier
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10.3847/1538-4357/ac4d95
Identifier
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https://repositorio.uchile.cl/handle/2250/189877
Abstract
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We present the results of variability power spectral density (PSD) analysis using multiwavelength radio to GeV gamma-ray light curves covering timescales of decades/years to days/minutes for the blazars 3C 279 and PKS 1510-089. The PSDs are modeled as single power laws, and the best-fit spectral shape is derived using the "power spectral response" method. With more than 10 yr of data obtained with weekly/daily sampling intervals, most of the PSDs cover similar to 2-4 decades in temporal frequency; moreover, in the optical band, the PSDs cover similar to 6 decades for 3C 279 due to the availability of intranight light curves. Our main results are the following: (1) on timescales ranging from decades to days, the synchrotron and the inverse-Compton spectral components, in general, exhibit red-noise (slope similar to 2) and flicker-noise (slope similar to 1) type variability, respectively; (2) the slopes of gamma-ray variability PSDs obtained using a 3 hr integration bin and 3 weeks total duration exhibit a range between similar to 1.4 and similar to 2.0 (mean slope = 1.60 +/- 0.70), consistent within errors with the slope on longer timescales; (3) comparisons of fractional variability indicate more power on timescales <= 100 days at gamma-ray frequencies compared to longer wavelengths, in general (except between the gamma-ray and optical wavelengths for PKS 1510-089); (4) the normalization of intranight optical PSDs for 3C 279 appears to be a simple extrapolation from longer timescales, indicating a continuous (single) process driving the variability at optical wavelengths; and (5) the emission at optical/infrared wavelengths may involve a combination of disk and jet processes for PKS 1510-089.
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Patrocinador
dc.description.sponsorship
Polish National Science Centre (NCN) 2018/29/B/ST9/02298
NCN 2018/29/B/ST9/01793
Polish NSC 2016/22/E/ST9/00061
European Research Council (ERC) 771282
University of Michigan System
National Science Foundation (NSF) AST-0808050
AST-1109911
AST-8021250
AST-8301234
AST8501093
AST-8815678
AST-9120224
AST-9421979
AST9617032
AST-9900723
AST-0307629
AST-0607523
National Aeronautics & Space Administration (NASA) NNX09AU16G
NNX10AP16G
NNX11AO13G
NNX13AP18G
NNX08AW31G
NNX11A043G
NNX14AQ89G
80GSFC21M0002
Caltech
MPIfR
NASA Fermi Guest Investigator grants 80NSSC20K1567
United States Department of Energy (DOE) DE-AC02-76SF00515
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Lenguage
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en
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Publisher
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IOP
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Type of license
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Attribution-NonCommercial-NoDerivs 3.0 United States