Galaxy Redshifts: Improved Techniques

Preprint
Publisher Website
Google Scholar
Abstract
This paper analyses the effects of random noise in determining errors and confidence levels for galaxy redshifts obtained by cross-correlation techniques. The main finding is that confidence levels have previously been overestimated, and errors inaccurately calculated in certain applications. New formul\ae\ are presented.

This publication has 0 references indexed in Scilit: