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(Eisenstein et al., ApJ, 2005) (Eisenstein et al., ApJ, 2005)

(Eisenstein et al., ApJ, 2005) - PowerPoint Presentation

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(Eisenstein et al., ApJ, 2005) - PPT Presentation

Surveys of large scale structure will probe Dark Energy by measuring the BAO scale vs redshift Planned DESI Euclid WFIRST 2 Hydrogen Intensity Mapping To measure BAO scale there is no need to resolve individual galaxies Map intensity of HI gas using redshifted 21 cm emission alo ID: 185118

lensing cmb ground chime cmb lensing chime ground modes space science 000 detectors frequency based dependence site foregrounds moore

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