Metsähovi Radio Observatory
AGN Research with the Swedish-ESO Submillimeter Telescope (SEST)

The Swedish-ESO Submillimetre Telescope, SEST, is a 15m diameter radio telescope situated at the European Southern Observatory site on Cerro La Silla, at 70.73 deg. W, 29.26 deg. South, 2300 m. The ideal location in the Chilean Andes, together with the high surface accuracy (70 microns rms) and sophisticated receiver equipment makes SEST an optimal telescope for high frequency (90 to 230 GHz) monitoring of southern active galactic nuclei. Flux density measurements of extragalactic radio sources have been made with the SEST telescope by our team from the very beginning of the SEST operation (since 1988). The SEST AGN flux monitoring project is closely connected to our group´s long-term flux density monitoring done at Metsähovi at lower (22 to 37 GHz) radio frequencies (Metsähovi quasar research project) The SEST monitoring project, however, is unique in providing us with large sets of high frequency data and information on otherwise rarely observed southern hemisphere sources.

Main objectives of the high radio frequency monitoring of AGN

	AGN monitoring since 1989, Metsähovi-Turku -collaboration
	Higher radio frequencies: 90 GHz & 230 GHz
	New information about the rarely observed Southern sources
	Information about the high-frequency behaviour of the sources
	Complete flux curves for the equatorial sources
	General source properties: spectra, variability
	Correlating outbursts at various frequency domains (radio-optical-gamma): dense monitoring/long term monitoring
	Testing and developing of shock models for outbursts
	Source classification, unification
	Predicting and interpreting VLBI behaviour

Some of our recent SEST continuum monitoring projects

Multifrequency observations of EGRET -detected gamma ray blazars

This project was initiated at the beginning of the CGRO operation. These observations are very important because for a short time still we will have the valuable opportunity to observe these sources across the electromagnetic spectrum from gamma to the radio frequencies. The project has several goals:

1. To monitor good candidates for our group's CGRO Target-of-opportunity observing proposal at the high radio frequencies.
2. To get detailed multifrequency spectrum of a flaring source in order to further study the emission mechanisms of gamma-rays and the relationsships of the various observing frequencies during a flare.
3. To make follow-up observations at the SEST frequencies of EGRET- detected southern AGN. Most of these sources have not been extensively observed at mm-frequencies, and more detailed studies of the spectra and variability are necessary for more thorough understanding of the nature of various sources.

Long term monitoring of active galactic nuclei

High radio frequency ground support for VSOP observations of AGN

The VSOP space-VLBI satellite was succesfully launched in February 1997. Metsahovi researchers are involved in a very large number of VSOP observing proposals, and most of these projects use also SEST data for ground support.

The VSOP satellite is a new powerful tool for studying the structure and physics of AGN. Ground-based radio observations will be essential for most of these projects, because:

• The monitoring data can be used to relate the observed VLBI features to the events observed in the flux curves during the monitoring, and thus help in understanding the shock formation and the structural changes in the shock component. SEST is one of the few telescopes capable of observing the southern VSOP sources, and its high frequency flux curves are valuable also for the more northern sources.

• Radio monitoring data can be used to determine wether a source is in its flaring or quiescent state, or to select soruces with currently observable interesting events (especially Targets-of-opportunity)

• Flux density information gathered with ground based telescopes is important in constructing spectra for the observed sources.

• Long time series of monitoring data (as we already have for some of our sources observed with the SEST) can be used to determine the variability evolution of the sources.

• High-frequency radio observations can be used to predict outbursts at lower frequencies, because the outbursts often are time delayed.

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SEST publications

See Metsähovi publications

SEST-data from 1989 to June 1994 were published in: Tornikoski et al., Astronomy and Astrophysics Supplement Series 116, 157, 1996 and are available in electronic format at the CDS via anonymous ftp 130.79.128.5

For other data requests contact Dr. Merja Tornikoski.

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For more information write to: Merja.Tornikoskitkk.fi