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The 72-h WEBT microvariability observation of blazar S5 0716 + 714 in 2009

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dc.contributor.author Bhatta G.
dc.contributor.author Webb J.
dc.contributor.author Hollingsworth H.
dc.contributor.author Dhalla S.
dc.contributor.author Khanuja A.
dc.contributor.author Bachev R.
dc.contributor.author Blinov D.
dc.contributor.author Bottcher M.
dc.contributor.author Bravo Calle O.
dc.contributor.author Calcidese P.
dc.contributor.author Capezzali D.
dc.contributor.author Carosati D.
dc.contributor.author Chigladze R.
dc.contributor.author Collins A.
dc.contributor.author Coloma J.
dc.contributor.author Efimov Y.
dc.contributor.author Gupta A.
dc.contributor.author Hu S.
dc.contributor.author Kurtanidze O.
dc.contributor.author Lamerato A.
dc.contributor.author Larionov V.
dc.contributor.author Lee C.
dc.contributor.author Lindfors E.
dc.contributor.author Murphy B.
dc.contributor.author Nilsson K.
dc.contributor.author Ohlert J.
dc.contributor.author Oksanen A.
dc.contributor.author Pääkkönen P.
dc.contributor.author Pollock J.
dc.contributor.author Rani B.
dc.contributor.author Reinthal R.
dc.contributor.author Rodriguez D.
dc.contributor.author Ros J.
dc.contributor.author Roustazadeh P.
dc.contributor.author Sagar R.
dc.contributor.author Sanchez A.
dc.contributor.author Shastri P.
dc.contributor.author Sillanpää A.
dc.contributor.author Strigachev A.
dc.contributor.author Takalo L.
dc.contributor.author Vennes S.
dc.contributor.author Villata M.
dc.contributor.author Villforth C.
dc.contributor.author Wu J.
dc.contributor.author Zhou X.
dc.date.accessioned 2018-09-18T20:01:45Z
dc.date.available 2018-09-18T20:01:45Z
dc.date.issued 2013
dc.identifier.issn 0004-6361
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/135873
dc.description.abstract Context. The international Whole Earth Blazar Telescope (WEBT) consortium planned and carried out three days of intensive micro-variability observations of S5 0716 + 714 from February 22, 2009 to February 25, 2009. This object was chosen due to its bright apparent magnitude range, its high declination, and its very large duty cycle for micro-variations. Aims. We report here on the long continuous optical micro-variability light curve of 0716+714 obtained during the multi-site observing campaign during which the Blazar showed almost constant variability over a 0.5 mag range. The resulting light curve is presented here for the first time. Observations from participating observatories were corrected for instrumental differences and combined to construct the overall smoothed light curve. Methods. Thirty-six observatories in sixteen countries participated in this continuous monitoring program and twenty of them submitted data for compilation into a continuous light curve. The light curve was analyzed using several techniques including Fourier transform, Wavelet and noise analysis techniques. Those results led us to model the light curve by attributing the variations to a series of synchrotron pulses. Results. We have interpreted the observed microvariations in this extended light curve in terms of a new model consisting of individual stochastic pulses due to cells in a turbulent jet which are energized by a passing shock and cool by means of synchrotron emission. We obtained an excellent fit to the 72-hour light curve with the synchrotron pulse model. © ESO, 2013.
dc.relation.ispartofseries Astronomy and Astrophysics
dc.subject BL Lacertae objects: individual: S5 0716+714
dc.subject Quasars: individual: S5 0716+714
dc.title The 72-h WEBT microvariability observation of blazar S5 0716 + 714 in 2009
dc.type Article
dc.relation.ispartofseries-volume 558
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS00046361-2013-558-SID84885790070


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  • Публикации сотрудников КФУ Scopus [20180]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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