output
19942026

4,205 papers

astro-ph.GA2026

MUSE-ALMA Haloes XV: Cold molecular, ionised, and stellar kinematics of HI-rich galaxies at z 0.5

C. Barfety, N. M. Förster Schreiber, C. Péroux +13

Spatially resolved galaxy kinematics are well studied at z 0 and z > 1, revealing that disks are common out to z , albeit with higher velocity dispersions. z …

astro-ph.GA2026

MUSE-ALMA Haloes XIV: The ALMA Large Programme Data Release

Céline Péroux, Jianhang Chen, Victoria Bollo +10

The interactions between gas and galaxies are of paramount importance to our understanding of structure formation. A fundamental element of such baryon cycle studies is a complete…

cs.CV2026★ 52 cited

Learning from synthetic photorealistic raindrop for single image raindrop removal

Zhixiang Hao, Shaodi You, Yu Li +2

Raindrops adhered to camera lens or windshield are inevitable in rainy scenes and can become an issue for many computer vision systems such as autonomous driving. Because raindrop…

astro-ph.IM2026

A fast, wide-field, and real-time imaging prototype for large aperture arrays

Nithyanandan Thyagarajan, Jishnu Thekkeppattu, David Humphrey

Real-time processing on sub-millisecond timescales is essential for detecting fast astrophysical transients such as fast radio bursts (FRBs) and prompt electromagnetic counterparts…

cs.CR2026

DisCTI: Who Needs to Know Timely? Automated Sector-Aware Cyber Threat Intelligence Dissemination

Fajar Wijitrisnanto, Alsharif Abuadbba, Yansong Gao +1

The timely dissemination of cyber threat intelligence (CTI) is critical for organizations to mount swift and effective incident response. When valid CTI is delivered to the right s…

astro-ph.GA2026

Estimating the local star formation rate density from ASKAP RACS

Sonja Panjkov, O. Ivy Wong., Rachel L. Webster

Understanding the evolution of the cosmic star formation rate density (SFRD) is key to uncovering how the Universe arrived at its present state. This paper presents a novel and eff…