activity
20172021
most citedSolving post-Newtonian accurate Kepler Equation

67 citations · 145 across the 4 of their papers we have counts for

collaborators

8 papers

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.HE202143 cited

Explaining temporal variations in the jet position angle of the blazar OJ 287 using its binary black hole central engine model

Lankeswar Dey, Mauri J. Valtonen, A. Gopakumar +5

The bright blazar OJ 287 is the best-known candidate for hosting a supermassive black hole binary system. It inspirals due to the emission of nanohertz gravitational waves (GWs). O…

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.IM2020

pinta: The uGMRT Data Processing Pipeline for the Indian Pulsar Timing Array

Abhimanyu Susobhanan, Yogesh Maan, Bhal Chandra Joshi +20

We introduce pinta, a pipeline for reducing the upgraded Giant Metre-wave Radio Telescope (uGMRT) raw pulsar timing data, developed for the Indian Pulsar Timing Array experiment. W…

gr-qc2020

Pulsar timing array signals induced by black hole binaries in relativistic eccentric orbits

Abhimanyu Susobhanan, Achamveedu Gopakumar, George Hobbs +1

Individual supermassive black hole binaries in non-circular orbits are possible nanohertz gravitational wave sources for the rapidly maturing Pulsar Timing Array experiments. We de…

astro-ph.GA2019

The Unique Blazar OJ 287 and its Massive Binary Black Hole Central Engine

Lankeswar Dey, Achamveedu Gopakumar, Mauri Valtonen +12

The bright blazar OJ 287 is the best-known candidate for hosting a nanohertz gravitational wave (GW) emitting supermassive binary black hole (SMBBH) in the present observable unive…