Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-27T04:35:51.567Z Has data issue: false hasContentIssue false
  • English
  • Français

A VSOP Survey Program Pre-launch Continuum Survey

Published online by Cambridge University Press:  12 April 2016

P. G. Edwards  and
E. B. Fomalont
P. G. Edwards
Affiliation:
ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
E. B. Fomalont
Affiliation:
ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229, Japan

Abstract

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 VSOP Survey Program will observe a complete survey of flat-spectrum sources at 5 GHz. In order to determine which of the sample sources are strong and small enough to be detected with VSOP, a pre-launch survey of 377 continuum sources north of δ > −43° was conducted at 5 GHz with the VLBA over 24 hours in June 1996. About 250 of the sources had correlated flux densities ≥ 0.4 Jy between MK–SC and have been included in the VSOP survey sample.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 143 - 144
Copyright
Copyright © Astronomical Society of the Pacific 1998