You can now search the Calibrator Manual around a region of interest.
Flux density measurements of VLA calibrators going back to December 1996 are available in the VLA calibrator flux history database. See what your favorite calibrator has been up to before you plan your next observing run. To properly interpret what you discover read this short document describing current limitations and how to use this utility.
New VLA On-Line Calibrator
Tool (Requires Java). Your one-stop shopping location for finding
information about VLA and VLBA calibrators. This includes plots
of calibrator spectra and light curves, and in some cases
visibility plots and images. This new tool is still under
development so expect some delays and possibly glitches. Please
send comments to caltool@nrao.edu.
We are working towards combining the VLA and VLBA calibrator databases and providing new and better tools to access the joint database. The plan is to design a much-improved calibrator finding tool that will also work for the EVLA and ALMA telescopes. Take a look at our calibrator specifications page. Please send any comments to gtaylor@nrao.edu.
We have begun a VLA polarization monitoring program for ~10 compact calibrators, primarily to enable better calibration of the VLBA. Each source is observed about once a month and reduced semi-automatically. The preliminary results are described in the VLA/VLBA Calibration Page.
Positions for 950 sources were refined on Aug. 28 2001 using the VLBA Calibrator Survey observations as reduced by the NASA Goddard Space Flight Center Geodesy group with the Calc/Solve package. These positions have typical positional errors less than 1 milliarcsec (see Johnston et al 1995, AJ 110, 880; and Beasley et al. in prep). This database is also the primary source of positions for the VLBA correlator. Two sources, J0259+425 and J2307+148 thought to have positions good to less than 50 mas, were discovered to be in error by more than 200 mas.
A tutorial for new users of the 74 and 330 MHz systems at the VLA has been written up by Namir Kassim & Rick Perley. It is available from http://rsd-www.nrl.navy.mil/7213/lazio/tutorial.
The Iridium constellation of satellites has begun transmitting almost continuously at 1622 MHz. This has serious consequences for 1612 MHz OH observations at the VLA, and also for continuum observations near 1622 MHz. For instructions on how to invoke a special set of front end filters to mitigate RFI see this Guide to the 18cm Front End Filters. For more details about the interaction of the VLA with the Iridium see this notice on calibration in the presence of the Iridium constellation for more details.
The flux densities calculated by SETJY for 3C286 using the coefficients determined in 1990 were systematically in error by 0.7 -- 1.7% in AIPS versions up to and including 15JAN96. See the SETJY bug notice for more details. The overall description of the flux density calibration scheme used at the VLA is described in Chapter 2.
Comments? Send them to gtaylor@aoc.nrao.edu
Last Modified on 2003 April 4
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