This book demonstrates for the first time, using state-of-the-art computer simulations, that the interpretation of future galaxy survey measurements is far more subtle than assumed, and that a major revision to our models of these effects is urgently needed.

This book demonstrates for the first time, using state-of-the-art computer simulations, that the interpretation of future galaxy survey measurements is far more subtle than assumed, and that a major revision to our models of these effects is urgently needed.

This book demonstrates for the first time, using state-of-the-art computer simulations, that the interpretation of future galaxy survey measurements is far more subtle than assumed, and that a major revision to our models of these effects is urgently needed.