Compactness of Weak Radio Sources at High Frequencies

Details Compactness of Weak Radio Sources at High Frequencies Compactness of Weak Radio Sources at High Frequencies

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21012101m&link_type=abstract

American Astronomical Society Meeting 210, #121.01; Bulletin of the American Astronomical Society, Vol. 39, p.328

Other

Scientific paper

We have obtained 8.4 GHz VLBA observations of a 31-GHz complete sample of 100 sources between 10 and 100 mJy. The main goals of these observations are: to determine the angular size, radio spectra and identification for a weak sample of high frequency sources; to find the fraction of sources which have sufficiently compact emission for use as calibrators for VLBI observations; and for design considerations of the proposed DSN Array. We find that a majority of the sources have most of their emission in a compact ə mas radio core, and that most of the other sources have steep radio spectra. The source list was provided from GBT observations to remove discrete sources in the CBI fields.

Affiliated with

Also associated with

No associations

Rating

Compactness of Weak Radio Sources at High Frequencies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Compactness of Weak Radio Sources at High Frequencies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Compactness of Weak Radio Sources at High Frequencies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1028159