Next: List of Tables
 Up: S.Bhatnagar: Thesis
 Previous: Contents
     Contents 
- Initial radio light curves a Type II-L SNe SN1980k
 - A typical spectral index evolution of a radio loud
Supernovae
 - Typical radio continuum spectrum for Galactic SNRs
 - Radio image of typical Shell-type SNR
 - Radio image of typical plerionic SNR
 - Radio image of typical composite/mixed morphology SNR
 - Radio image of typical barrel-shaped SNR
 - Distribution of known Galactic SNRs as a function Galactic
longitude
 - Schematic diagram showing the effect of the ionosphere
 - Orientation of the XYZ co-ordinate system and its relation to
the Hour angle and declination of the source
 - Geometric relation between the sky plane and the observing
plane
 - Two element interferometer
 - The location of the GMRT antennas
 - The location of the GMRT antennas in the Central Square
 - Full synthesis uv-coverage of the GMRT array
 - Full synthesis uv-coverage of the GMRT Central Square 
 - Schematic diagram of the GMRT receiver
 - Schematic diagram of a single correlator pipeline
 - Antenna phase as a function of declination
 - Antenna phase as a function of HA for Central Square antennas at 327
MHz
 - Antenna phase as a function of HA for arm antennas at 327
MHz
 - Antenna based phases as a function of channel number before
fixed delay calibration
 - Antenna based phases as a function of channel number after
fixed delay calibration
 - Graphical representation of the geometry of the Image
  volume and the Celestial sphere.
 - Graphical illustration to compute the distance between the
tangent plane and a point in the sky at an angle of
.
 - Graphical representation of polyhedron imaging
 - Gray scale image of the field containing G001.4
0.0
 - Gray scale image of the field containing G0003.7
0.0
 - Higher resolution image of field containing G004.2
0.0
 - Gray scale image of the field containing G004.8+6.2
 - Gray scale image of field containing G356.2-1.5
 - Gray scale image of the field containing G356.2+4.5
 - Gray scale image of the field containing G358.0+3.8
 - GMRT 327-MHz image of G001.4
0.0
 - The GMRT 327-MHz image of  G003.8
0.3
 - 327-MHz contours overlayed on the 
m IRAS image of
G003.8
0.3
 - 11 cm image of G003.8
0.3 using 100-m Effelsberg
telescope
 - GMRT 327-MHz image of the field G004.2
0.0
 - IRAS 
 image of G004.2
0.0
 - GMRT image of G004.8
6.2 at 327 MHz and NVSS image at 1400 MHz.
 - VLA image of G004.8
6.2 at 325 MHz. 
 - The GMRT 327-MHz image of G356.3-1.5
 - The GMRT image of G356.2+4.5 at 327 MHz and NVSS image at
1400 MHz.
 - GMRT image of G358.0+3.8 at 327 MHz and NVSS image at
1400 MHz.
 - GMRT 327-MHz image of  G003.7
0.2
 - GMRT 327-MHz image of G355.9-2.5
 - GMRT 327-MHz image of the Kepler's SNR (G004.5
6.8)
 - Comparison of typical thermal and non-thermal
spectrum
 - G003.6
0.1 at 327 and 1420 MHz
 - G003.6
0.1 at 5-GHz and 60
 - HI absorption profiles against G003.6
0.1
 - Continuum spectra of G003.6
0.1
 - Linear structure in the field of G356.3
1.5
 - Image of the Ultra Compact H II region G004.4
0.1 at 327 and
1420 MHz
 - Spectral index 
 for
G004.417
0.126
 - Extended emission around two HII region at the edge of
G003.7
0.2 field
 - Results of the simulations to test the leaky antsol algorithm
 - Comparison of 
 before and after correction for
polarization leakage
 - Computed complex antenna based polarization leakage
 - The Poincaré sphere
 
 
Sanjay Bhatnagar
2005-07-07