output
20172026
most citedImproved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

311 citations

Showing astro-ph.IMShow all

7 papers · 1 filter

astro-ph.IM2026

PIE-ADA: Physics-Informed Ensemble with Adaptive Data Augmentation for Photometric Transient Classification

Deba Priyo Guha, Fariya Tabassum

The upcoming Large Synoptic Survey Telescope (LSST) is expected to observe approximately 10 million astronomical transient events per night, creating an urgent need for automated c…

astro-ph.IM2026

JAXtronomy: A JAX port of lenstronomy

Alan Huang, Simon Birrer, Daniel Gilman +4

Gravitational lensing is a phenomenon where light bends around massive objects, resulting in distorted images seen by an observer. Studying gravitationally lensed systems provides…

astro-ph.IM2026

Survey Footprint Explorer: A Browser-Based Interactive Tool for Visualizing and Cross-Matching Astronomical Survey Footprints

S. L. Ahad, R. Brilenkov, J. E. Taylor

We present the Survey Footprint Explorer (v2.5.0), a browser-based interactive tool for visualising and comparing the sky footprints of major astronomical imaging surveys. The tool…

astro-ph.IM2025

RGC: a radio AGN classifier based on deep learning. I. A semi-supervised multiclass model for VLA images

M. S. Hossain, M. S. H. Shahal, K. M. B. Asad +10

Bent radio active galactic nuclei (RAGNs) -- wide-angle tails (WATs) and narrow-angle tails (NATs) -- trace dense environments in galaxy groups and clusters, yet no multiclass clas…

astro-ph.IM2025★ 9 cited

An accurate measurement of the spectral resolution of the JWST Near Infrared Spectrograph

Anowar J. Shajib, Tommaso Treu, Alejandra Melo +4

The spectral resolution () of spectroscopic data is crucial information for accurate kinematic measurements. In this letter, we present a robust measurement of the…

astro-ph.IM2023★ 3 cited

Morphological Classification of Radio Galaxies using Semi-Supervised Group Equivariant CNNs

Mir Sazzat Hossain, Sugandha Roy, K. M. B. Asad +4

Out of the estimated few trillion galaxies, only around a million have been detected through radio frequencies, and only a tiny fraction, approximately a thousand, have been manual…

astro-ph.IM2019★ 62 cited

Primary beam effects of radio astronomy antennas -- II. Modelling the MeerKAT L-band beam

K. M. B. Asad, J. N. Girard, M. de Villers +12

After a decade of design and construction, South Africa's SKA-MID precursor MeerKAT has begun its science operations. To make full use of the widefield capability of the array, it…