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Abstract

We present GMRT observational results from a project that was designed to identify possible calibrators 235 MHz and 610 MHz, which are important observing frequencies of GMRT. We will present the additional information like the flux density, complexity of the field of view for the sources and also present a few images of individual fields. This information will be useful for observers in GMRT who are trying to identify presented calibrators for their observation.

In the following section, we define and discuss the quality criteria used for identifying calibrators from the list of 150 observed sources. We also group these identified GMRT calibrators at 610 MHz & 235 MHz according to quality as `List1', `List2', etc.



Manisha Jangam 2007-06-19