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Cavendish Astrophysics

 
Fig.2: Power spectra at z = 7.7 derived from a 55-day PAPER observation. In both panels, solid cyan depicts upper limits derived from PAPER observations without the removal of off-diagonal covariance terms, and black indicates the final measured power spe
Alt Text: 
Fig.2: Power spectra at z = 7.7 derived from a 55-day PAPER observation. In both panels, solid cyan depicts upper limits derived from PAPER observations without the removal of off-diagonal covariance terms, and black indicates the final measured power spe
Title Text: 
Power Spectrum