A1 Refereed original research article in a scientific journal
Optical Photometric and Radio Monitoring of Gamma-ray Loud Blazars
Authors: Bychkova VS, Kardashev NS, Larionov MG, Volvach AE, Vlasjuk VV, Spiridonova OI, Lachteenmaki A, Tornikoski M, Hovatta T, Nieppola E, Torniainen I, Aller HD, Aller MF
Publisher: INDIAN ACAD SCIENCES
Publication year: 2011
Journal: Journal of Astrophysics and Astronomy
Journal name in source: JOURNAL OF ASTROPHYSICS AND ASTRONOMY
Journal acronym: J ASTROPHYS ASTRON
Volume: 32
Issue: 1-2
First page : 105
Last page: 108
Number of pages: 4
ISSN: 0250-6335
DOI: https://doi.org/10.1007/s12036-011-9015-6
Abstract
The harmonic analysis performed for the light curves of 0716+714 from 2002-2010 in radio and optical wave bands revealed the presence of an apparent periodical component in the flux variations. The period of the radio light curve is nearly 3.6 years, and coincides within the errors with the period of the optical light curve (nearly 3.4 years). The duration of the flares is approximately the same in radio and optical ranges, and it is about 100-150 days.
The harmonic analysis performed for the light curves of 0716+714 from 2002-2010 in radio and optical wave bands revealed the presence of an apparent periodical component in the flux variations. The period of the radio light curve is nearly 3.6 years, and coincides within the errors with the period of the optical light curve (nearly 3.4 years). The duration of the flares is approximately the same in radio and optical ranges, and it is about 100-150 days.
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