Conclusions from the image analysis of the VSOP Survey

E. Fomalont; K. Wiik; R. Dodson

REVIEW

Conclusions from the image analysis of the VSOP Survey

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 0901.1493 v1 pith:NROPWC5A submitted 2009-01-12 astro-ph.GA

Conclusions from the image analysis of the VSOP Survey

R. Dodson , E. Fomalont , K. Wiik This is my paper

classification astro-ph.GA

keywords vsopsurveyanalysisconclusionsmissionsourcesactiveastronomy

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

In February 1997, the Japanese radio astronomy satellite HALCA was launched to provide the space-bourne element for the VLBI Space Observatory Programme (VSOP) mission. A significant fraction of the mission time was to be dedicated to the VSOP Survey of bright compact Active Galactic Nuclei (AGN) at 5 GHz, which was lead by ISAS. The VSOP Survey Sources are an unbiased dataset of 294 targets, of which 82% were successfully observed. These are now undergoing statistical analysis to tease out the characteristics of typical AGN sources. We present here the summary of the imaging and conclusions we have reached.

Conclusions from the image analysis of the VSOP Survey

discussion (0)