The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview
Devin Crichton, Moumita Aich, Adam Amara, Kevin Bandura, Bruce A., Bassett, Carlos Bengaly, Pascale Berner, Shruti Bhatporia, Martin Bucher,, Tzu-Ching Chang, H. Cynthia Chiang, Jean-Francois Cliche, Carolyn Crichton,, Romeel Dave, Dirk I. L. de Villiers, Matt A. Dobbs

TL;DR
HIRAX is a radio interferometer array designed for cosmological intensity mapping of neutral hydrogen, aiming to study large-scale structure, dark energy, and transient phenomena with a 256-element setup and future expansion plans.
Contribution
This paper presents the design, status, and expected performance of the HIRAX 256-element array, a novel instrument for cosmological and transient radio science.
Findings
Initial array performance estimates indicate strong potential for large-scale structure mapping.
The experiment can constrain dark energy parameters with about 7% precision.
Future expansion to 1024 elements will enhance scientific capabilities.
Abstract
The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio interferometer array currently in development, with an initial 256-element array to be deployed at the South African Radio Astronomy Observatory (SARAO) Square Kilometer Array (SKA) site in South Africa. Each of the 6m, dishes will be instrumented with dual-polarisation feeds operating over a frequency range of 400-800 MHz. Through intensity mapping of the 21 cm emission line of neutral hydrogen, HIRAX will provide a cosmological survey of the distribution of large-scale structure over the redshift range of over 15,000 square degrees of the southern sky. The statistical power of such a survey is sufficient to produce 7 percent constraints on the dark energy equation of state parameter when combined with measurements from the Planck satellite. Additionally, HIRAX will…
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