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High Radio Frequency Studies of Equatorial and Southern AGN

Published online by Cambridge University Press:  25 May 2016

M. Tornikoski  and
E. Valtaoja
M. Tornikoski
Affiliation:
Metsähovi Radio Research Station Metsähovintie 114, FIN–02540 Kylmälä, Finland
E. Valtaoja
Affiliation:
Metsähovi Radio Research Station Metsähovintie 114, FIN–02540 Kylmälä, Finland

Extract

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The Swedish-ESO Submillimetre Telescope (SEST) has been used for the high radio frequency observations of our group's AGN monitoring projects since the end of 1987.

Our SEST results from October 1987 until June 1994 will be published in A&AS (in press); the data will be available electronically. The data set consists of 155 sources with the signal-to-noise -ratio of at least one observation (at 90 or 230 GHz) ≥ 4.

Type
Properties of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 99 - 100
Copyright
Copyright © Kluwer 1996 

References

Tornikoski, M., Valtaoja, E., Teräsranta, H., et al., 1993, AJ , 105, 1680 CrossRefGoogle Scholar
Tornikoski, M., Valtaoja, E., Teräsranta, H., et al., 1994, A&A , 289, 673 Google Scholar