Harvard University Department of Astronomy
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Astronomy 193: 
Noise and Data Analysis in Astrophysics

James M. Moran

 

Course Overview

The world today is awash in data, and that data can be massaged a great deal with fast computers.  This course will help you to deal intelligently with data and to assess the work of others.  (Why does the estimated value of the Hubble constant wander beyond its error bars?)  The course is different from most others of this type in that it takes a two-pronged approach to data analysis, whose parts may loosely be called "signal processing" and "parameter estimation."  The first part is most useful in conditioning the data when you don't know exactly what you're looking for, as well as in understanding how your instrument has conditioned the data for you.  The second part is useful for comparing data with models.

The course begins with a thorough discussion of the practical aspects of Fourier transforms, which have many applications to the theory of data filtering and interpolation, and which play an important role in probability theory.  This is followed by an overview of relevant aspects of probability and stochastic processes.  The last two sections of the course are about digital signal processing (e.g., filtering, power spectrum analysis, the effects of sampling, etc.) and parameter estimation (maximum likelihood methods, linear and non-linear least-mean-square analysis with emphasis on accurate error estimation).

 
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Last modified on January 31, 2007