collaborators

6 papers

astro-ph.IM2026

Source Finding and Characterisation for SKAO Science

Sabyasachi Pal, Souvik Manik, M Carmen Toribio +8

The advancements in highly sensitive and powerful radio telescopes, including the Square Kilometre Array Observatory (SKAO) and its precursors, MeerKAT, ASKAP, MWA, and HERA, will…

astro-ph.GA2026

Tracing the Origin of Circular-Symmetry Diffuse Radio Sources in the Next-Generation SKAO Era

Sabyasachi Pal, Shobha Kumari, Souvik Manik +2

Circularly symmetric diffuse radio sources represent a recently recognized and rare class of extragalactic synchrotron-emitting structures whose physical origin remains uncertain.…

astro-ph.GA2026

Exploring the Influence of the Jet-environment Interactions on the Observed Asymmetry of Extragalactic Radio Sources with SKAO

Sabyasachi Pal, Souvik Manik, Shobha Kumari +1

Several observational and theoretical studies have suggested that the observed arm-length asymmetries in extragalactic radio sources are primarily driven by interactions between ra…

astro-ph.GA2026

RAD@home discovery of a bow-and-arrow radio galaxy tracing a ~560 kpc bow-shock structure in a multi-halo environment

Ananda Hota, Pratik Dabhade, Shubhrangshu Ghosh +9

We report the RAD@home citizen science discovery of a unique bow-and-arrow-shaped radio galaxy (BAARG; RAD J104501.6+352852, z = 0.159) identified in LoTSS DR2. The source exhibits…

astro-ph.GA2025

Hybrid Morphology Radio Sources from the MeerKAT Absorption Line Survey (MALS): Radio, Mid-infrared and Environmental Characteristics

Souvik Manik, Shobha Kumari, Netai Bhukta +2

Hybrid morphology radio sources (HyMoRSs) are a rare subclass of radio galaxies that display a Fanaroff-Riley type I (FR I) morphology on one side of the central supermassive black…

astro-ph.GA2025

Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations

Shobha Kumari, Sabyasachi Pal, Souvik Manik

We report the discovery of J1218+1813, a circular diffuse radio source detected in the Very Large Array (VLA) FIRST survey at 1400 MHz. The source has an angular diameter of approx…