GOYAL, A., L. STAWARZ, S. ZOLA, V. MARCHENKO, M. SOIDA, K. NILSSON, S. CIPRINI, A. BARAN, M. OSTROWSKI, P.J. WIITA, A. GOPAL-KRISHNA, A. SIEMIGINOWSKA, M. SOBOLEWSKA, S. JORSTAD, A. MARSCHER, M.F. ALLER, H.D. ALLER, T. HOVATTA, D.B. CATON, D. REICHART, K. MATSUMOTO, K. SADAKANE, K. GAZEAS, M. KIDGER, V. PIIROLA, H. JERMAK, F. ALICAVUS, K.S. BALIYAN, A. BARANSKY, A. BERDYUGIN, P. BLAY, P. BOUMIS, D. BOYD, Y. BUFAN, M.C. TORRENT, F. CAMPOS, J.C. GOMEZ, J. DALESSIO, B. DEBSKI, D. DIMITROV, M. DRÓŻDŻ, H. ER, A. ERDEM, A.E. PEREZ, V.F. RAMAZANI, A.V. FILIPPENKO, E. GAFTON, F. GARCIA, V. GODUNOVA, F.G. PINILLA, M. GOPINATHAN, J.B. HAISLIP, S. HAQUE, J. HARMANEN, R. HUDEC, G. HURST, K.M. IVARSEN, A. JOSHI, M. KAGITANI, N. KARAMAN, R. KARJALAINEN, N. KAUR, D. KOZIEL-WIERZBOWSKA, E. KULIGOWSKA, T. KUNDERA, S. KUROWSKI, A. KVAMMEN, A.P. LACLUYZE, B.C. LEE, A. LIAKOS, J.L. DE HARO, J.P. MOORE, M. MUGRAUER, R.N. NOGUES, A.W. NEELY, W. OGLOZA, S. OKANO, U. PAJDOSZ, J.C. PANDEY, M. PERRI, G. POYNER, J. PROVENCAL, T. PURSIMO, A. RAJ, B. RAJKUMAR, R. REINTHAL, T. REYNOLDS, J. SAARIO, S. SADEGI, T. SAKANOI, J.L.S. GONZALEZ, A. SAMEER, A.O. SIMON, M. SIWAK, T. SCHWEYER, F.C.S. ALFARO, E. SONBAS, J. STROBL, L.O. TAKALO, L.T. ESPASA, J.R. VALDES, V.V. VASYLENKO, F. VERRECCHIA, J.R. WEBB, M. YONEDA, M. ZEJMO, W. ZHENG, Pawel ZIELIŃSKI, Jan JANÍK, V. CHAVUSHYAN, I. MOHAMMED, C.C. CHEUNG a M. GIROLETTI. Stochastic Modeling of Multiwavelength Variability of the Classical BL Lac Object OJ287 on Timescales Ranging from Decades to Hours. Astrophysical Journal. Chicago: University of Chicago Press, 2018, roč. 863, č. 2, s. 1-20. ISSN 0004-637X. Dostupné z: https://dx.doi.org/10.3847/1538-4357/aad2de.
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Základní údaje
Originální název Stochastic Modeling of Multiwavelength Variability of the Classical BL Lac Object OJ287 on Timescales Ranging from Decades to Hours
Autoři GOYAL, A., L. STAWARZ, S. ZOLA (616 Polsko), V. MARCHENKO, M. SOIDA, K. NILSSON, S. CIPRINI, A. BARAN (616 Polsko), M. OSTROWSKI, P.J. WIITA, A. GOPAL-KRISHNA, A. SIEMIGINOWSKA, M. SOBOLEWSKA, S. JORSTAD, A. MARSCHER, M.F. ALLER, H.D. ALLER, T. HOVATTA, D.B. CATON, D. REICHART, K. MATSUMOTO, K. SADAKANE, K. GAZEAS (300 Řecko), M. KIDGER, V. PIIROLA (246 Finsko), H. JERMAK, F. ALICAVUS, K.S. BALIYAN, A. BARANSKY, A. BERDYUGIN, P. BLAY, P. BOUMIS, D. BOYD, Y. BUFAN, M.C. TORRENT, F. CAMPOS, J.C. GOMEZ, J. DALESSIO, B. DEBSKI, D. DIMITROV, M. DRÓŻDŻ (616 Polsko), H. ER, A. ERDEM (792 Turecko), A.E. PEREZ, V.F. RAMAZANI, A.V. FILIPPENKO, E. GAFTON, F. GARCIA, V. GODUNOVA, F.G. PINILLA, M. GOPINATHAN, J.B. HAISLIP, S. HAQUE, J. HARMANEN, R. HUDEC (203 Česká republika), G. HURST, K.M. IVARSEN, A. JOSHI, M. KAGITANI, N. KARAMAN, R. KARJALAINEN, N. KAUR, D. KOZIEL-WIERZBOWSKA (616 Polsko), E. KULIGOWSKA (616 Polsko), T. KUNDERA (616 Polsko), S. KUROWSKI, A. KVAMMEN (616 Polsko), A.P. LACLUYZE, B.C. LEE, A. LIAKOS (300 Řecko), J.L. DE HARO, J.P. MOORE, M. MUGRAUER, R.N. NOGUES, A.W. NEELY, W. OGLOZA (616 Polsko), S. OKANO, U. PAJDOSZ, J.C. PANDEY, M. PERRI, G. POYNER, J. PROVENCAL, T. PURSIMO, A. RAJ, B. RAJKUMAR, R. REINTHAL, T. REYNOLDS, J. SAARIO, S. SADEGI, T. SAKANOI, J.L.S. GONZALEZ, A. SAMEER, A.O. SIMON, M. SIWAK, T. SCHWEYER, F.C.S. ALFARO, E. SONBAS, J. STROBL, L.O. TAKALO, L.T. ESPASA, J.R. VALDES, V.V. VASYLENKO, F. VERRECCHIA, J.R. WEBB, M. YONEDA, M. ZEJMO (616 Polsko), W. ZHENG, Pawel ZIELIŃSKI (616 Polsko), Jan JANÍK (203 Česká republika, garant, domácí), V. CHAVUSHYAN, I. MOHAMMED, C.C. CHEUNG a M. GIROLETTI.
Vydání Astrophysical Journal, Chicago, University of Chicago Press, 2018, 0004-637X.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Spojené státy
Utajení není předmětem státního či obchodního tajemství
WWW URL
Impakt faktor Impact factor: 5.580
Kód RIV RIV/00216224:14310/18:00104124
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.3847/1538-4357/aad2de
UT WoS 000442628400011
Klíčová slova anglicky acceleration of particles; BL Lacertae objects: individual (OJ 287); galaxies: active; magnetic fields; radiation mechanisms: non-thermal
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnil: Mgr. Michal Petr, učo 65024. Změněno: 23. 4. 2024 12:35.
Anotace
We present the results of our power spectral density analysis for the BL Lac object OJ 287, utilizing the Fermi-LAT survey at high-energy.-rays, Swift-XRT in X-rays, several ground-based telescopes and the Kepler satellite in the optical, and radio telescopes at GHz frequencies. The light curves are modeled in terms of continuous-time autoregressive moving average (CARMA) processes. Owing to the inclusion of the Kepler data, we were able to construct for the first time the optical variability power spectrum of a blazar without any gaps across similar to 6 dex in temporal frequencies. Our analysis reveals that the radio power spectra are of a colored-noise type on timescales ranging from tens of years down to months, with no evidence for breaks or other spectral features. The overall optical power spectrum is also consistent with a colored noise on the variability timescales ranging from 117 years down to hours, with no hints of any quasi-periodic oscillations. The X-ray power spectrum resembles the radio and optical power spectra on the analogous timescales ranging from tens of years down to months. Finally, the.-ray power spectrum is noticeably different from the radio, optical, and X-ray power spectra of the source: we have detected a characteristic relaxation timescale in the Fermi-LAT data, corresponding to similar to 150 days, such that on timescales longer than this, the power spectrum is consistent with uncorrelated (white) noise, while on shorter variability timescales there is correlated (colored) noise.
VytisknoutZobrazeno: 24. 7. 2024 18:13