Gravitational lensing directly measures fluctuations in the gravitational potential along paths to distant objects. Currently, there are no firm examples of radio selected lens systems with image separations >7'', but many with separations <7''. We have made use of the approximately 2500 flat-spectrum radio sources that make up JVAS (the Jodrell Bank VLA Astrometric Survey) (Patnaik et al. 1992 and papers in preparation) to select wide-separation (>6'') gravitational lens candidates. Lensing of flat-spectrum radio sources is relatively easy to recognise since the source structures are point-dominated. In the original JVAS analysis, no attempt was made to look for lenses with separations >6'', so this is a new search. The secondary components will be lensed images or part of the source structure or less probably, simply chance sources nearby.
last modified on Saturday, December 24, 2005 at 10:25:22 PM by helbig@astro.mNuOlStPiAvMa!x.de