610 MHz $--$ Results

In the Chapter 3, we had discussed the procedure for data reduction using the data analysis package AIPS. Using the same package AIPS, we here present the results of our observation at 610 MHz, i.e., the radio images, plots of amplitude as a function of $uv$-distance for a few sources.

The detailed information of these results is summarized in the table A.1 in appendix A. The table includes, (i) the flux density of the source, both, the peak and the integrated. (ii) the best angular resolution, (iii) deconvolved size of the major axis of the source, and (iv) the information of the additional sources, called secondary sources, within the field-of-view. When a secondary source is present in the field-of-view, we also give it's, (a) flux density, (b) distance from the target source, and (c) its position angle.

The same table also gives the information of the number of other detectable secondary sources within the field-of-view. If there are no other strong sources (sources having flux density greater than $\approx$ 5% of the flux density of the source) within the field-of-view, apart from the target source at the phase center, a syntax '$-$' have been put in order to indicate the absence of the secondary sources.