1999/09/28 by I. W. A. Browne, E. Xanthopoulos, Browne, I. W. A. +5
Earth and Planetary Sciences · Physics and Astronomy · #Adaptive optics and wavefront sensing #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9909459
submitted to "Gravitational Lensing: Recent progress and Future Goals", eds: T.Brainerd and C.Kochanek, ASP Conf Series. 2 pages, 1 figure. LaTex using paspman.tex
arxiv created 1999/09/28 · arxiv updated 2009/12/01
The complex 10-component gravitational lens B1933+503 has been monitored with the VLA during the period February to June 1998. Here we present the results of this A-configuration 8.4 GHz monitoring campaign. The 37 epochs of observations have an average spacing of 3 days. The data have yielded light curves for the four flat-spectrum radio components (components 1, 3, 4 and 6). We find no significant flux density changes in any of the four flat spectrum components.