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Pulsar Research with the GMRT: A Status Report

Published online by Cambridge University Press:  12 April 2016

Y. Gupta ,
P. Gothoskar ,
B.C. Joshi ,
M. Vivekanand ,
R. Swain ,
S. Sirothia  and
N.D.R. Bhat
Y. Gupta
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
P. Gothoskar
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
B.C. Joshi
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
M. Vivekanand
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
R. Swain
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
S. Sirothia
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India
N.D.R. Bhat
Affiliation:
National Centre for Radio Astrophysics, TIFR, Pune - 411 007, India

Abstract

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The Giant Metrewave Radio Telescope (GMRT) coming up near Pune, India will be one of the important instruments for pulsar research work at metre wavelengths. Here we describe the capabilities of the GMRT for pulsar work and give the current status of the telescope in this context. Results from recent test observations are also summarised.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 277 - 278
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Swarup, G., Ananthakrishnan, S., Subrahmanya, C.R., Rao, A.P., Kulkarni, V.K., & Kapahi, V.K. 1997, in High Sensitivity Radio Astronomy, ed. Jackson, N. & Davis, R.J. (Cambridge University Press)Google Scholar