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Contents
- The Electromagnetic Spectrum
- The Radio Telescope.
- The track in the plane traced out by an east-west baseline due to the Earth's
rotation.
- Location of GMRT antennas.
- The block diagram of the receiver system.
- Schematic diagram of a single correlator pipeline.
- Software/Hardware Components of the ONLINE System.
- Distribution of Observed Sources on the Sky Plane.
- 'Flat' -distance plots of the sources at 610 MHz.
- 'Non-Flat' -distance plots of the sources at 610 MHz.
- 'Non-Flat' -distance plots of the sources at 610 MHz.
- 'Non-Flat' -distance plots of the sources at 610 MHz.
- 'Non-Flat' -distance plots of the sources at 610 MHz.
- Images of the Point Sources at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- Images of the sources with non-flat plots at 610 MHz.
- -distance plots of the sources at 235 MHz.
- -distance plots of the sources at 235 MHz.
- -distance plots of the sources at 235 MHz.
- -distance plots of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Images of the sources at 235 MHz.
- Emission of Synchrotron Radiation.
- Spectra of the Source 0240-231.
- Schematic of an ideal power spectrum and one with cutoffs at 10 and 1000 MHz.
- Synchrotron spectrum with a break around 150 MHz.
- Spectrum with a turn over due to synchrotron self absorption.
- Flat spectrum source formed by many different self absorbed components.
- Flat spectrum source with low frequency turnover.
- Composite spectrum - a self absorbed component in a steep spectrum source.
- Spectra with two self absorbed components.
- Sources with Class S Spectra.
- Sources with Class P1-A Spectra.
- Sources with Class P1-B Spectra.
- Sources with Class P2 Spectra.
- Sources with Class F1 Spectra.
- Sources with Class F2 Spectra.
- Sources with Class C1 Spectra.
- Sources with Class C2 Spectra.
- Sources with Class U Spectra.
Manisha Jangam
2007-06-19