activity
20202026
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations · 1.5k across the 21 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2026

Study of pulse jitter characteristics of PSR J1744-1134: Towards high precision pulsar timing with InPTA

Jibin Jose, Manoneeta Chakraborty, Neelam Dhanda Batra +15

Variations in the shapes of individual pulses introduce a broadband noise component in pulsar times of arrival beyond what is expected from radiometer noise, referred to as the jit…

astro-ph.HE2026

Profile Reconstruction from Temporally Stable Emission Components for Timing PSR J1713+0747

Shaswata Chowdhury, M. A. Krishnakumar, Sharika Dhakappa +26

The assumption of long-term pulse-profile stability underpins high-precision pulsar timing and forms the basis of pulsar timing array experiments. However, several millisecond puls…

astro-ph.HE2026

The Indian Pulsar Timing Array Data Release 2: III. Search for a Stochastic Gravitational Wave Background

Hemanga Tahbildar, Kunjal Vara, Mayuresh Surnis +28

We present the first independent search for an isotropic stochastic gravitational wave background in the second data release of the Indian Pulsar Timing Array, comprising of 27 mil…

astro-ph.HE2025★ 2 cited

The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget

K. Nobleson, Churchil Dwivedi, Shantanu Desai +33

We present the results of customised single-pulsar noise analysis of 27 millisecond pulsars from the second data release of the Indian Pulsar Timing Array (InPTA-DR2). We model var…

astro-ph.IM2025★ 1 cited

Revisiting wideband pulsar timing measurements

Abhimanyu Susobhanan, Avinash Kumar Paladi, Réka Desmecht +28

In the wideband paradigm of pulsar timing, the time of arrival of a pulsar pulse is measured simultaneously with the corresponding dispersion measure from a frequency-resolved inte…

astro-ph.IM2025★ 6 cited

The Indian Pulsar Timing Array Data Release 2: I. Dataset and Timing Analysis

Prerna Rana, Pratik Tarafdar, Nobleson K +44

The Indian Pulsar Timing Array (InPTA) employs unique features of the upgraded Giant Metrewave Radio Telescope (uGMRT) to monitor dozens of the International Pulsar Timing Array (I…

astro-ph.HE2023★ 4 cited

Low-frequency pulse-jitter measurement with the uGMRT I : PSR J04374715

Tomonosuke Kikunaga, Shinnosuke Hisano, Neelam Dhanda Batra +22

High-precision pulsar timing observations are limited in their accuracy by the jitter noise that appears in the arrival time of pulses. Therefore, it is important to systematically…

astro-ph.IM2023★ 2 cited

Improving DM estimates using low-frequency scattering-broadening estimates

Jaikhomba Singha, Bhal Chandra Joshi, M. A. Krishnakumar +28

A pulsar's pulse profile gets broadened at low frequencies due to dispersion along the line of sight or due to multi-path propagation. The dynamic nature of the interstellar medium…

astro-ph.HE2023

Comparing recent PTA results on the nanohertz stochastic gravitational wave background

The International Pulsar Timing Array Collaboration, G. Agazie, J. Antoniadis +242

The Australian, Chinese, European, Indian, and North American pulsar timing array (PTA) collaborations recently reported, at varying levels, evidence for the presence of a nanohert…

gr-qc2023★ 4 cited

Unveiling a universal relationship between the f(R) parameter and neutron star properties

K. Nobleson, Sarmistha Banik, Tuhin Malik

In recent years, modified gravity theories have gained significant attention as potential replacements for the general theory of relativity. Neutron stars, which are dense compact…

astro-ph.HE2023★ 1k cited

The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

J. Antoniadis, P. Arumugam, S. Arumugam +95

We present the results of the search for an isotropic stochastic gravitational wave background (GWB) at nanohertz frequencies using the second data release of the European Pulsar T…

astro-ph.CO2023★ 111 cited

The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

J. Antoniadis, P. Arumugam, S. Arumugam +111

The European Pulsar Timing Array (EPTA) and Indian Pulsar Timing Array (InPTA) collaborations have measured a low-frequency common signal in the combination of their second and fir…

astro-ph.HE2023★ 76 cited

The second data release from the European Pulsar Timing Array V. Search for continuous gravitational wave signals

J. Antoniadis, P. Arumugam, S. Arumugam +97

We present the results of a search for continuous gravitational wave signals (CGWs) in the second data release (DR2) of the European Pulsar Timing Array (EPTA) collaboration. The m…

astro-ph.IM2023★ 5 cited

Multi-band Extension of the Wideband Timing Technique

Avinash Kumar Paladi, Churchil Dwivedi, Prerna Rana +27

The wideband timing technique enables the high-precision simultaneous estimation of pulsar Times of Arrival (ToAs) and Dispersion Measures (DMs) while effectively modeling frequenc…

astro-ph.HE2023★ 15 cited

Noise analysis of the Indian Pulsar Timing Array data release I

Aman Srivastava, Shantanu Desai, Neel Kolhe +28

The Indian Pulsar Timing Array (InPTA) collaboration has recently made its first official data release (DR1) for a sample of 14 pulsars using 3.5 years of uGMRT observations. We pr…

astro-ph.HE2022★ 24 cited

Nanohertz Gravitational Wave Astronomy during the SKA Era: An InPTA perspective

Bhal Chandra Joshi, Achamveedu Gopakumar, Arul Pandian +34

Decades long monitoring of millisecond pulsars, which exhibit highly stable rotational periods, in pulsar timing array experiments is on the threshold of discovering nanohertz stoc…

astro-ph.IM2022★ 82 cited

The Indian Pulsar Timing Array: First data release

Pratik Tarafdar, Nobleson K., Prerna Rana +35

We present the pulse arrival times and high-precision dispersion measure estimates for 14 millisecond pulsars observed simultaneously in the 300-500 MHz and 1260-1460 MHz frequency…

astro-ph.IM2021★ 19 cited

Low-frequency wideband timing of InPTA pulsars observed with the uGMRT

K Nobleson, Nikita Agarwal, Raghav Girgaonkar +29

High-precision measurements of the pulsar dispersion measure (DM) are possible using telescopes with low-frequency wideband receivers. We present an initial study of the applicatio…

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…

gr-qc2021★ 4 cited

Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity

K Nobleson, Tuhin Malik, Sarmistha Banik

There is a growing interest in investigating modified theories of gravity, primarily, with the aim of explaining the universe's accelerated expansion, which has been confirmed by s…

astro-ph.HE2021★ 23 cited

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.HE2020

Neutron Stars with realistic EoS in f(R) theories of gravity

K Nobleson, Amna Ali, Sarmistha Banik

In this paper, we examine neutron star structure in perturbative gravity models with realistic equation of state. We obtain mass-radius relations in two gravity models of th…

astro-ph.IM2020★ 22 cited

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…