This Web page will assist in setting fields in AIPS task IMAGR in the neighborhood of a specified position. This will help deal with confusing sources when it is not possible or desirable to image the full primary beam of the antenna. The procedure is to use the NVSS (NRAO/VLA Sky Survey) survey to select sources in the area of interest and then to produce an AIPS "RUN" file that sets the extra fields containing the confusing sources. The returned file can be either used directly as an AIPS RUN file by stripping the html wrapper or using the cut and paste facility of your window manager to enter the commands directly into AIPS.
The NVSS radio survey uses the NRAO Very Large Array telescope and covers the sky north of a declination of -40 degrees at a frequency of 1.4 GHz, a resolution of 45" and a limiting peak source brightness of about 2.5 mJy/beam. This survey is complete. For detailed general instructions click here or for more about a form entry click on its label.
For details on the probability of the chance coincidence of an NVSS source within a given radius of an arbitrary position look here.
In publications using NVSS results please reference Condon, et al. 1998, AJ, 115, 1693; a preprint of this paper which describes the design and techniques of the NVSS is available here. The contents of the NVSS source catalog is described here. For very extensive searches or listing of large amounts of the catalog it may be best to obtain your own copy of the catalog (from krithika:/astro/catalogues/NVSS/CATALOG/ and it about 150 MByte) and the browsing software (from krithika:/astro/catalogues/NVSS/CATALOG/ for Unix users). For the latest information and detailed descriptions of the NVSS survey see its home page. Entire 4 x 4 degree fields may be obtained as FITS files using image cubes. The NVSS Catalog browser will search the catalog for specified regions and return a list of sources found. A postage stamp server which returns FITS or jpeg files of limited regions from NVSS images is also available.