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20242026
most citedRevisiting wideband pulsar timing measurements

1 citations · 1 across the 2 of their papers we have counts for

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7 papers

astro-ph.IM20261 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.HE2026

Post-glitch Recovery and the Neutron Star Structure: The Vela Pulsar

Himanshu Grover, Erbil Gügercinoğlu, Bhal Chandra Joshi +4

We present a detailed analysis of the Vela pulsar's rotational behaviour using approximately 100 months of observational data spanning from September 2016 to January 2025, during w…

astro-ph.IM2025

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.IM2024

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.HE2024

The ORT and the uGMRT Pulsar Monitoring Program : Pulsar Timing Irregularities & the Gaussian Process Realization

Himanshu Grover, Bhal Chandra Joshi, Jaikhomba Singha +8

The spin-down law of pulsars is generally perturbed by two types of timing irregularities: glitches and timing noise. Glitches are sudden changes in the rotational frequency of pul…

astro-ph.CO2024

Comparison of CDM and with updated galaxy cluster measurements using Bayesian inference

Kunj Panchal, Shantanu Desai

We use updated gas mass fraction measurements of 44 massive dynamically relaxed galaxy clusters collated in arXiv:2111.09343 to distinguish between the standard CDM model and $…