activity
20062008
most citedStatistical analyses of long-term variability of AGN at high radio frequencies

121 citations · 253 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2008★ 1 cited

Long term radio variability of AGN

T. Hovatta, M. Tornikoski, H. J. Lehto +7

A large number of AGN have been monitored for nearly 30 years at 22, 37 and 87 GHz in Metsähovi Radio Observatory. These data were combined with lower frequency 4.8, 8.0 and 14.5 G…

astro-ph2008★ 59 cited

Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006--2007 outburst

C. M. Raiteri, M. Villata, V. M. Larionov +2

The blazar AO 0235+164 was claimed to show a quasi-periodic behaviour in the radio and optical bands. Moreover, an extra emission component contributing to the UV and soft X-ray fl…

astro-ph2007★ 121 cited

Statistical analyses of long-term variability of AGN at high radio frequencies

T. Hovatta, M. Tornikoski, M. Lainela +5

We present a study of variability time scales in a large sample of Active Galactic Nuclei at several frequencies between 4.8 and 230 GHz. We investigate the differences of various…

astro-ph2007★ 43 cited

37 GHz observations of a large sample of BL Lacertae objects

E. Nieppola, M. Tornikoski, A. Lähteenmäki +11

We present 37 GHz data obtained at Metsahovi Radio Observatory in 2001 December - 2005 April for a large sample of BL Lacertae objects. We also report the mean variability indices…

astro-ph2006

IX Russian-Finnish Symposium on Radio Astronomy "Multi-wavelength investigations of solar and stellar activity and active galactic nuclei"

V. E. Abramov-Maximov, T. G. Arshakian, V. M. Bogod +33

The IX Russian-Finnish Symposium on Radio Astronomy was held in Special astrophysical observatory RAS in Nizhnij Arkhyz, Russia on 15-20 October 2006. It was dedicated to the two-s…

astro-ph2006★ 29 cited

Discovery of an Extreme MeV Blazar with the Swift Burst Alert Telescope

Rita M. Sambruna

The Burst Alert Telescope (BAT) onboard Swift detected bright emission from 15--195 keV from the source SWIFT~J0746.3+2548 (J0746 in the following), identified with the optically-f…