activity
20242026
collaborators

10 papers

math.DG2026

-parabolicity of Riemannian manifolds

Alexander Grigor'yan, Leandro F. Pessoa, Alberto G. Setti

We describe the -parabolicity of a Riemannian manifold in terms of a unified theory of nonlinear -capacities, for the whole range . For example, the \…

astro-ph.IM2026

LeoNet: A Machine Learning Method for Binary Pulsar Classification

Zhaocheng Gong, Jack White, Zeyu Yang +3

Binary pulsars provide valuable laboratories for testing theories of gravity, but orbital Doppler shifts complicate their detection. Fourier-domain acceleration and jerk searches a…

astro-ph.IM2026

MARS: A Lightweight Morphology-Aware RFI Segmentation Network for Mask-Guided Mitigation in Radio Astronomy

Zhaocheng Gong, Jack White, Jayanta Roy +1

Next-generation radio telescopes generate filterbank data at rates that make storing all observations for later offline mitigation impractical. Mitigation must therefore operate in…

astro-ph.IM2025

FIP-TOI: Fast Imaging Pipeline for Pulsar Localisation with a Transient-Oriented Radio Astronomical Imager

X. Li, K. Adamek, O. Bilaniuk +2

Rapid localisation of radio transients requires imaging pipelines that combine low latency, high sensitivity, and accurate transient positioning. Fast Imaging Pipeline (FIP) define…

astro-ph.HE2025

Globular Clusters GMRT Pulsar Search (GCGPS) I: Survey description, discovery and timing of the first pulsar in NGC 6093 (M80)

Jyotirmoy Das, Jayanta Roy, Paulo C. C. Freire +6

This paper describes the new Globular Clusters GMRT Pulsar Search (GCGPS) survey. This survey aims to find MSPs in the globular clusters (GCs) of the Milky Way using uGMRT. The obs…

astro-ph.IM2024

Distribution of the Högbom CLEAN Algorithm Using Tiled Images with Feedback

Daniel Wright, Karel Adámek, Wesley Armour

Data sizes for next generation radio telescopes, such as the Square Kilometre Array (SKA), are far above that of their predecessors. The CLEAN algorithm was originally developed by…

astro-ph.IM2024

Lowering In-Memory Footprint of Antenna Beams via Polynomial Approximation

Ali Taqi, Karel Adámek, Quentin Gueuning +3

With the emergence of new radio telescopes promising larger fields of view at lower observation frequencies (e.g., SKA), addressing direction-dependent effects (DDE) (e.g., directi…

astro-ph.IM2024

Pulscan: Binary pulsar detection using unmatched filters on NVIDIA GPUs

Jack White, Karel Adámek, Jayanta Roy +2

The Fourier Domain Acceleration Search (FDAS) and Fourier Domain Jerk Search (FDJS) are proven matched filtering techniques for detecting binary pulsar signatures in time-domain ra…

astro-ph.IM2024

CLEAN algorithm implementation comparisons between popular software packages

Daniel Wright, Karel Adámek, Wesley Armour

The CLEAN algorithm, first published by Högbom and its later variants such as Multiscale CLEAN (msCLEAN) by Cornwell, has been the most popular tool for deconvolution in radio astr…

astro-ph.HE2024

Toward using GANs in astrophysical Monte-Carlo simulations

Ahab Isaac, Wesley Armour, Karel Adámek

Accurate modelling of spectra produced by X-ray sources requires the use of Monte-Carlo simulations. These simulations need to evaluate physical processes, such as those occurring…