activity
20082026
most citedHydrogen Epoch of Reionization Array (HERA)

657 citations · 6.8k across the 116 of their papers we have counts for

collaborators

118 papers

quant-ph2026

Architecture and Compilation Co-Design for High-Rate Quantum Product Codes on Neutral Atom Arrays

Adrian Liu, Wan-Hsuan Lin, Daniel Bochen Tan +2

Achieving fault-tolerant quantum computing at a practical scale demands quantum error correction (QEC) codes with high encoding rates. Quantum low-density parity-check (qLDPC) code…

astro-ph.IM2026

Overview of the Canadian Hydrogen Observatory and Radio Transient Detector (CHORD) Project

The CHORD Collaboration, Kevin Bandura, Leonid Belostotski +49

The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD) is a next-generation wideband radio interferometer currently being constructed and commissioned at the Domini…

astro-ph.IM2026

Advancing Astrophysics with the SKA II

Anna Bonaldi, Tyler L. Bourke, Philippa Hartley +45

Advancing Astrophysics with the SKA II (AASKAII), written by our science community, outlines the transformative scientific advances that will be enabled by the SKA telescopes. In t…

astro-ph.IM2026

Machine Learning and the SKA for Cosmic Dawn and the Epoch of Reionization

Anshuman Acharya, Michele Bianco, Daniela Breitman +18

When operational, the SKA will generate unprecedented amounts of data and provide exquisite sensitivity for 21 cm tomography of Cosmic Dawn (CD) and the Epoch of Reionization (EoR)…

astro-ph.CO2026

Overview of 21cm Experiments at high redshift with SKAO

CD Science Working Group, Gianni Bernardi, Daniela Breitman +81

We provide an overview of the eight SKAO Science Book chapters that motivate the Epoch of Reionisation and Cosmic Dawn experiments with SKA-Low. We describe the individual SKA-Low…

astro-ph.CO2026

The of Neutral Hydrogen: Increased CMB Optical Depth at Long Wavelengths

Gilbert Holder, Adrian Liu, Tzu-Ching Chang +1

At wavelengths longer than 21 cm, photons from the long-wavelength tail of the cosmic microwave background (CMB) have a non-zero probability of being absorbed by distant neutral hy…