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Carolyn Crichton

Publications and source records attributed to Carolyn Crichton.

2 recordsLinked to original sources

Space Sustainability: The Global Commons

Space is no longer a distant, barely reachable frontier of scientific exploration; it has become a critical infrastructure for life on Earth and a rapidly expanding zone of intense commercial activity. Yet this expansion is unfolding in ways that replicate, and amplify, the unsustainable dynamics already driving ecological and social crises on our planet. This chapter explains the concept of space sustainability as a multidimensional challenge; it raises the questions of governance, knowledge, power, justice, and global responsibility. It highlights both the profound benefits derived from space activities and the uneven distribution of costs and risks, from orbital debris and atmospheric impacts to privatization of essential services. We therefore argue that it frames space as a global commons that demands stewardship rather than pure exploitation, cooperation rather than competition, and governance that prioritizes long-term wellbeing rather than laissez-faire approach. Sustainability in space is inseparable from sustainability on Earth. This chapter invites readers, whether they are space administration and industry actors, policymakers, scientists, or simply engaged citizens, to see space not as a limitless frontier, but as a shared domain whose future depends on collective choices made today.

physics.soc-ph↗

The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview

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, $f/0.23$ 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 $0.775 < z < 2.55$ over $\sim$15,000 square degrees of the southern sky. The statistical power of such a survey is sufficient to produce $\sim$7 percent constraints on the dark energy equation of state parameter when combined with measurements from the Planck satellite. Additionally, HIRAX will provide a highly competitive platform for radio transient and HI absorber science while enabling a multitude of cross-correlation studies. In this paper, we describe the science goals of the experiment, overview of the design and status of the sub-components of the telescope system, and describe the expected performance of the initial 256-element array as well as the planned future expansion to the final, 1024-element array.

astro-ph.IM↗