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10 July 2008ACWI: an experiment to image the Cosmic Web from Antarctica
The Antarctic Cosmic Web Imager (ACWI) is a dedicated 2m-class telescope specifically designed to discover and map
resonance UV line emission from the Intergalactic Medium (IGM) and to explore the low surface brightness universe.
IGM mapping will provide a new measurement of large-scale structure and the distribution of dark matter over a large
and unique range in overdensity. The South Pole provides a location with (1) a target elevation that is constant during
observation hence sees constant airmass (2) the lowest measured extinction of any ground based site (3) a low and
constant ecliptic elevation and hence zodiacal emission away from the target location and (4) long duration nights
yielding stable sky and instrument properties enabling the required accurate sky subtraction. These factors combined
imply a sky background that is the most stable of any ground-based site, a requirement for this particular science case
where the subtraction of sky background, rather than the image quality, must be exquisite. We present the baseline
instrument design that is catered to perform this science case only and is not a general purpose instrument, increasing
robustness and reliability.
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Anna M. Moore, Christopher Martin, Noam C Maitless, Tony Travouillon, "ACWI: an experiment to image the Cosmic Web from Antarctica," Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 70122A (10 July 2008); https://doi.org/10.1117/12.790281