A processing technique with fidelity for extended sources.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

A new method is proposed to process extended sources with high fidelity.
The approach is based on analysing the distribution of the observed data
with baseline. This method consists of data calibrating and u-v voids
filling. A map of the supernova remnant HB3 made from actual MSRT data
at 232 MHz is also presented here.

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