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20152021
most citedEvidence for profile changes in PSR J1713+0747 using the uGMRT

35 citations · 147 across the 7 of their papers we have counts for

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astro-ph.HE202135 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.HE201919 cited

Observed glitches in 8 young pulsars

Avishek Basu, Bhal Chandra Joshi, M. A. Krishnakumar +5

The abrupt change in the pulse period of a pulsar is called a pulsar glitch. In this paper, we present eleven pulsar glitches detected using the Ooty Radio Telescope (ORT) and the…

astro-ph.HE201919 cited

Multi-frequency scatter broadening evolution of pulsars - II. Scatter broadening of nearby pulsars

M. A. Krishnakumar, Yogesh Maan, Bhal Chandra Joshi +1

We present multi-frequency scatter broadening evolution of 29 pulsars observed with the LOw Frequency ARray (LOFAR) and Long Wavelength Array (LWA). We conducted new observations u…

astro-ph.HE2018

Follow-up Timing of Three GMRT Pulsars

Mayuresh P. Surnis, Bhal Chandra Joshi, Maura A. McLaughlin +3

We report on the results of multi-frequency follow-up observations of three pulsars (PSRs J0026+6320, J2208+5500 and J2217+5733) discovered with the Giant Metrewave Radio Telescope…

astro-ph.HE2018

A Search for Pulsars in Steep Spectrum Radio Sources

Yogesh Maan, Cees Bassa, Joeri van Leeuwen +2

We report on a time-domain search for pulsars in 44 steep spectrum radio sources originally identified from recent imaging surveys. The time-domain search was conducted at 327 MHz…