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- 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 G001.40.0
- Gray scale image of the field containing G0003.70.0
- Higher resolution image of field containing G004.20.0
- 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 G001.40.0
- The GMRT 327-MHz image of G003.80.3
- 327-MHz contours overlayed on the m IRAS image of
G003.80.3
- 11 cm image of G003.80.3 using 100-m Effelsberg
telescope
- GMRT 327-MHz image of the field G004.20.0
- IRAS image of G004.20.0
- GMRT image of G004.86.2 at 327 MHz and NVSS image at 1400 MHz.
- VLA image of G004.86.2 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 G003.70.2
- GMRT 327-MHz image of G355.9-2.5
- GMRT 327-MHz image of the Kepler's SNR (G004.56.8)
- Comparison of typical thermal and non-thermal
spectrum
- G003.60.1 at 327 and 1420 MHz
- G003.60.1 at 5-GHz and 60
- HI absorption profiles against G003.60.1
- Continuum spectra of G003.60.1
- Linear structure in the field of G356.31.5
- Image of the Ultra Compact H II region G004.40.1 at 327 and
1420 MHz
- Spectral index
for
G004.4170.126
- Extended emission around two HII region at the edge of
G003.70.2 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