collaborators

9 papers

astro-ph.CO2026

The diffraction-lensing interpretation of GW231123 with astrophysical priors

Mark Ho-Yeuk Cheung, Digvijay Wadekar, Matias Zaldarriaga +3

GW231123, if unlensed, is a rare binary black hole merger with high masses and high spins for both progenitors. We show that the signal is better fitted by a lower-mass, lower-spin…

astro-ph.HE2026

Interplanetary scintillation-informed heliospheric modelling for the MeerKAT Pulsar Timing Array 4.5 yr dataset

Saurav Mishra, Daniel J. Reardon, Andrew Zic +9

Heliospheric density variations impart delays on pulse times of arrivals from millisecond pulsars. Improper modelling of these variations may affect gravitational wave detection an…

astro-ph.HE2026

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog

Tousif Islam, Tejaswi Venumadhav, Digvijay Wadekar +6

We provide a comprehensive analysis of GW190711_030756 and GW200114_020818, two of the most significant binary black hole merger candidates in the IAS catalog, with probabilities o…

gr-qc2026

Searching for precessing binary systems with mode-by-mode filtering and marginalization

Zihan Zhou, Digvijay Wadekar, Javier Roulet +8

Nearly all previous binary black hole searches in LIGO--Virgo--KAGRA (LVK) gravitational wave data have assumed that the component spins are aligned with the orbital angular moment…

astro-ph.IM2026

Sample-efficient non-Gaussian noise reduction in gravitational wave data via learnable wavelets

Arush Pimpalkar, Digvijay Wadekar, Mark Ho-Yeuk Cheung +1

We introduce , a wavelet-based neural network architecture to identify and reduce non-Gaussian noise in gravitational wave data. Traditionally, convolutional n…

gr-qc2025

Accuracy of ringdown models calibrated to numerical relativity simulations

Francesco Crescimbeni, Gregorio Carullo, Emanuele Berti +3

The ''ringdown'' stage of gravitational-wave signals from binary black hole mergers, mainly consisting of a superposition of quasinormal modes emitted by the merger remnant, is a k…