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19952016
most citedDoppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies

438 citations · 2.5k across the 39 of their papers we have counts for

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astro-ph2009★ 14 cited

Multi-frequency VLBA study of the blazar S5 0716+714 during the active state in 2004: I. Inner jet kinematics

E. A. Rastorgueva, K. Wiik, T. Savolainen +4

We observed the blazar \object{0716+714} with the VLBA during its active state in 2003-2004. In this paper we discuss multi-frequency analysis of the inner jet (first 1 mas) kinema…

astro-ph2008

Studying the continuum spectrum of the parsec scale jets by multi-frequency VLBI measurements

T. Savolainen, K. Wiik, E. Valtaoja +1

Multi-frequency VLBI observations allow studies of the continuum spectrum in the different parts of the parsec scale jets of AGN, providing information on the physical properties o…

astro-ph2008★ 438 cited

Doppler factors, Lorentz factors and viewing angles for quasars, BL Lacertae objects and radio galaxies

T. Hovatta, E. Valtaoja, M. Tornikoski +1

We have calculated variability Doppler boosting factors, Lorentz factors, and viewing angles for a large sample of sources by using total flux density observations at 22 and 37 GHz…

astro-ph2008★ 86 cited

Long-term radio variability of AGN: flare characteristics

T. Hovatta, E. Nieppola, M. Tornikoski +3

We have studied the flare characteristics of 55 AGN at 8 different frequency bands between 4.8 and 230 GHz. Our extensive database enables us to study the various observational pro…

astro-ph2008★ 95 cited

Blazar sequence - an artefact of Doppler boosting

E. Nieppola, E. Valtaoja, M. Tornikoski +2

The blazar sequence is a scenario in which the bolometric luminosity of the blazar governs the appearance of its spectral energy distribution. The most prominent result is the sign…

astro-ph2007★ 2 cited

Magnetic Field Structure in the Parsec Scale Jet of 3C273 from Multifrequency VLBA Observations

T. Savolainen, K. Wiik, E. Valtaoja +1

We present first results from a multifrequency VLBA observations of 3C273 in 2003. The source was observed simultaneously at 5.0, 8.4, 15.3, 22.2, 43.2 and 86.2 GHz, and from this…