2009

Empirical H-alpha emitter count predictions for dark energy surveys

Geach, J. E., Cimatti, A., Percival, W. et al.

Understand

Future galaxy redshift surveys aim to measure cosmological quantities from the galaxy power spectrum.

A prime example is the detection of baryonic acoustic oscillations (BAOs), providing a standard ruler to measure the dark energy equation of state, w(z), to high precision.
The strongest practical limitation for these experiments is how quickly accurate redshifts can be measured for sufficient galaxies to map the large-scale structure.
A promising strategy is to target emission-line (i.e.

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