Clustering of Galaxies

We will measure the spectrum of the density fluctuations to high precision

even on very large scales

The error in the amplitude of  the fluctuation spectrum

1970 x100

1990 x2

1995 ±0.4

1998 ±0.2

1999 ±0.1

2002 ±0.05

Previous slide

Next slide

Back to first slide

View graphic version