Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..12e..47o&link_type=abstract
Long Wavelength Astrophysics, 26th meeting of the IAU, Joint Discussion 12, 21 August 2006, Prague, Czech Republic, JD12, #47
Astronomy and Astrophysics
Astrophysics
Scientific paper
The observed non-thermal spectral index of the radio sources increases with the redshift. Therefore, radio sources at high-redshift can be detected easily at low radio frequencies. We imaged a region with the GMRT at 327 MHz. The achieved rms in the image is ~0.2 mJy/beam. These images have a combination of better sensitivity and better resolution, thereby enabling us to detect many more sources at 327 MHz than reported earlier toward the fainter ends. The source count distribution with limiting sensitivity of 1 mJy will be presented.
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