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:
-
3C48 (0137+331) at U-band:
AIPS FITS
file,
image (pdf file),
uv plot (pdf file)
-
3C48 (0137+331) at K-band:
AIPS
FITS file,
image,
uv plot
-
3C48 (0137+331) at Q-band:
AIPS
FITS file,
image,
uv
plot
-
3C138 (0521+166) at U-band:
AIPS
FITS file,
image,
uv plot
-
3C138 (0521+166) at K-band:
AIPS
FITS file,
image,
uv plot
-
3C138 (0521+166) at Q-band:
AIPS
FITS file,
image,
uv
plot
-
3C147 (0542+498) at U-band:
AIPS
FITS file,
image,
uv plot
-
3C147 (0542+498) at K-band:
AIPS
FITS file,
image,
uv plot
-
3C147 (0542+498) at Q-band:
AIPS
FITS file,
image,
uv plot
-
3C286 (1331+305) at U-band:
AIPS
FITS file,
image,
uv plot
-
3C286 (1331+305) at K-band:
AIPS
FITS file,
image,
uv plot
-
3C286 (1331+305) at Q-band:
AIPS
FITS file,
image,
uv
plot
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