2016

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Aghamousa, Amir, Aguilar, Jessica et al.

Understand

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey.

To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data.
We will measure luminous red galaxies up to $z=1.0$.
To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$.

Built on

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“The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12”
A.˜J. Cuesta et al · 2016
Closest in time.
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D. Lang · 2016
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C.˜L. Reichardt, R. de Putter, O. Zahn and Z. Hou · 2041
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Original
M. Sumiyoshi et al · 2064
Closest in time.

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