VLA images with CLEAN component models attached in CC tables of some primary flux calibrators for use in all (including extended) configurations (1999.2 flux scale), in a format suitable for AIPS. These models are in J2000 coordinates. If your data are in B1950, either change the uv data to J2000 with UVFIX or change the images to B1950 with EPOSWTCH in AIPS. Note that the following models are now distributed with the "TST" version of AIPS as well: The following FITS images of the CLEAN components of the same sources are suitable for use with AIPS++ (i.e., these have not been convolved with a CLEAN beam, and do not have a CC table attached):
Maintained by cchandle@nrao.edu, last updated September 2004