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20192025
most citedEvidence for profile changes in PSR J1713+0747 using the uGMRT

35 citations · 72 across the 6 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2025

A White Paper on The Multi-Messenger Science Landscape in India

Samsuzzaman Afroz, Sanjib Kumar Agarwalla, Dipankar Bhattacharya +35

The multi-messenger science using different observational windows to the Universe such as Gravitational Waves (GWs), Electromagnetic Waves (EMs), Cosmic Rays (CRs), and Neutrinos o…

astro-ph.HE2023★ 27 cited

Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars

Bikram Keshari Pradhan, Dhruv Pathak, Debarati Chatterjee

Gravitational waves (GW) emanating from unstable quasi-normal modes in Neutron Stars (NS) could be accessible with the improved sensitivity of the current GW detectors or with the…

astro-ph.HE2021★ 35 cited

Evidence for profile changes in PSR J1713+0747 using the uGMRT

Jaikhomba Singha, Mayuresh P Surnis, Bhal Chandra Joshi +29

PSR J1713+0747 is one of the most precisely timed pulsars in the international pulsar timing array experiment. This pulsar showed an abrupt profile shape change between April 16, 2…

astro-ph.HE2021

High Precision Measurements of Interstellar Dispersion Measure with the upgraded GMRT

M. A. Krishnakumar, P. K. Manoharan, Bhal Chandra Joshi +19

Pulsar radio emission undergoes dispersion due to the presence of free electrons in the interstellar medium (ISM). The dispersive delay in the arrival time of pulsar signal changes…

astro-ph.HE2019

Correcting the measured values of the rate of change of the spin and orbital periods of rotation powered pulsars

Dhruv Pathak, Manjari Bagchi

For rotation powered pulsars, the rate of change of the spin period is expected to be positive. On the other hand, for a clean binary system (where gravity is the only force acting…