activity
20242026
collaborators

7 papers

astro-ph.HE2026

Probing Merger Shocks in Galaxy Clusters in the SKA Era

Arpan Pal, Ruta Kale, Gabriella Di Gennaro +8

Galaxy cluster mergers represent the most energetic phenomena in the Universe since the Big Bang releasing gravitational potential energy of erg, injecting turbul…

astro-ph.IM2026

VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for QU-Fitting

Arpan Pal, Preshanth Jagannathan

Bayesian QU-fitting is among the most accurate approaches for line-of-sight Faraday inference, but its per-pixel computational cost has made survey-scale application infeasible. QU…

astro-ph.IM2026

Reliability of uGMRT Band-4 Polarimetry: Results from a Quadrature Hybrid Polarizer Bypass Experiment

Arpan Pal, Sanjeet Rai, Ganesh Kumbhar

Polarimetric observations at sub-GHz frequencies offer unique access to the magnetized universe through Faraday rotation and depolarization studies, but achieving reliable polariza…

astro-ph.GA2026

Wiggling Through the ICM: Multi-Resolution Radio Imaging of a Tailed Radio Galaxy in MACS J1354.6+7715

Abdul Gani, Roland Timmerman, Leah K. Morabito +4

Tailed radio galaxies are powerful tracers of interactions between active galactic nuclei (AGN) and the intracluster medium (ICM), providing unique insights into cluster dynamics.…

astro-ph.HE2025

A Linearly Polarized Merger Shock Down to 550 MHz: A uGMRT Study of the Merging Cluster Abell 746

Arpan Pal, Ruta Kale, Reinout J. van Weeren

Radio relics, arc-like polarized sources with highly aligned magnetic fields, are typically found on the outskirts of merging galaxy clusters. The magneto-ionic media responsible f…

astro-ph.HE2025

A Possible Four-Month Periodicity in the Activity of FRB 20240209A

Arpan Pal

Fast Radio Bursts (FRBs) are millisecond-duration radio transients from distant galaxies. While most FRBs are singular events, repeaters emit multiple bursts, with only two-FRB 121…