Hostname: page-component-7479d7b7d-c9gpj Total loading time: 0 Render date: 2024-07-10T21:27:02.340Z Has data issue: false hasContentIssue false

High Radio Frequency Studies of Equatorial and Southern AGN

Published online by Cambridge University Press:  25 May 2016

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

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.

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
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