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Illuminating the dark universe with a very high density galaxy redshift survey over a wide area

Published onMay 31, 2019
Illuminating the dark universe with a very high density galaxy redshift survey over a wide area
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Abstract

A very high number density galaxy redshift survey over a wide area (HD GRS Wide) spanning the redshift range of 0.5 < z < 4 using the same tracer, carried out using massively parallel wide field multi-object slit spectroscopy from space, will provide definitive dark energy measurements with minimal observational systematics by design.

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