Illuminating the dark universe with a very high density galaxy redshift survey over a wide area
by Yun Wang, Rachel Bean, Peter Behroozi, Chia-Hsun Chuang, Ian Dell'antonio, Mark Dickinson, Olivier Dore, Daniel Eisenstein, Ryan Foley, Karl Glazebrook, Luigi Guzzo, Christopher Hirata, Shirley Ho, Michael Hudson, Bhuvnesh Jain, Priyamvada Natarajan, Jeff Newman, Alvaro Orsi, Nikhil Padmanabhan, John Peacock, Will Percival, Jason Rhodes, Eduardo Rozo, Lado Samushia, Dan Scolnic, Hee-Jong Seo, David Spergel, Michael Strauss, Risa Wechsler, and David Weinberg
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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