Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-28T07:45:58.909Z Has data issue: false hasContentIssue false
  • English
  • Français

Connection Between Optical and High Frequency Radio Variability in AGN

Published online by Cambridge University Press:  19 July 2016

M. Tornikoski ,
E. Valtaoja ,
A.G. Smith  and
A.D. Nair
M. Tornikoski
Affiliation:
Metsähovi Radio Research Station, SF-02540 Kylmälä, Finland
E. Valtaoja
Affiliation:
Metsähovi Radio Research Station, SF-02540 Kylmälä, Finland
A.G. Smith
Affiliation:
Astronomy Dept., University of Florida, Gainesville, Fl-32611, USA
A.D. Nair
Affiliation:
Astronomy Dept., University of Florida, Gainesville, Fl-32611, USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have been searching for correlated optical and radio variability in large temporal data sets of 22 extragalactic radio sources. The optical data were obtained with the 76-cm reflector at the Rosemary Hill Observatory in Florida, USA. The radio data were obtained at two different sites: 22, 37 and some of the 90 GHz data at the Metsähovi Radio Research Station, Finland, and 90 and 230 GHz data at the Swedish-ESO Submillimetre Telescope (SEST) on La Silla, Chile. Because the SEST data unfortunately reaches only back to 1988, the 90 and 230 GHz data were complemented by the IRAM data from Steppe et al. (A&AS 75, 1988 and A&AS 96, 1992).

Type
Poster Contributions: Variability
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 411
Copyright
Copyright © Kluwer 1994