output
19962026
most citedAn Introduction to Convolutional Neural Networks

951 citations

393 papers

astro-ph.GA2026

Determination of kinematic distances of WISE & SMGPS H II regions in the Galactic plane using SEDIGISM cloud association

Moses Langa, Mark Thompson, Andrew Rigby +7

One of the fundamental requirements for studying and understanding Galactic structure and massive star formation is accurate distances to H II regions. However, most distance assig…

cs.HC2026

Digital hybridity and relics in cultural heritage: using corpus linguistics to inform design in emerging technologies from AI to VR

Emma McClaughlin, Glenn McGarry, Alan Chamberlain +2

Hybrid technologies enable the blending of physical and digital elements, creating new ways to experience and interact with the world. Such technologies can transform engagement wi…

physics.space-ph2026★ 1 cited

Turbulent dynamo in the terrestrial magnetosheath

Zoltán Vörös, Owen Wyn Roberts, Yasuhito Narita +10

Dynamo action refers to energy exchange processes through which magnetic fields are generated at the expense of kinetic energy of the plasma flows. Dynamos can generate magnetic fi…

quant-ph2025

Characterizing Fisher information of quantum measurement

Rakesh Saini, Jukka Kiukas, Daniel Burgarth +1

Informationally complete measurements form the foundation of universal quantum state reconstruction, while quantum parameter estimation is based on the local structure of the manif…

astro-ph.SR2025

A multi-viewpoint comparison of the velocity field of coronal propagating disturbances

Nina Stankovic, Huw Morgan, Marilena Mierla +3

Small-scale propagating disturbances (PD) are ubiquitous in the solar corona. Time-Normalised Optical Flow (TNOF) is a method developed for mapping PD velocity fields in time serie…

astro-ph.GA2025★ 1 cited

H II regions and supernova remnants associated with molecular clouds: A pilot study with the SARAO MeerKAT Galactic Plane Survey

Moses O. Langa, Mark A. Thompson, Andrew J. Rigby +5

Massive stars (mass beyond 8 solMass) release vast amounts of energy into the interstellar medium through their stellar winds, photoionising radiation and supernova explosions. The…