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THE UNIVERSITY of EDINBURGHDEGREE REGULATIONS & PROGRAMMES OF STUDY 2006/2007
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Astronomical Statistics and X-Ray Astronomy (U01401)? Credit Points : 10 ? SCQF Level : 10 ? Acronym : PHY-4-AstStats Astronomical Statistics: A section on probability and statistics for astronomers introduces the elements of probability theory, the calculus of probabilities and the central limit theorem, going on to consider various uses of statistics, including hypothesis testing, estimation, Bayes' theorem, and the investigation of correlation and regression and the effect of biases in data; the emphasis is on methods that are common in astronomical research, and how to avoid the notorious pitfalls that frequently trap the unwary. Entry Requirements? Pre-requisites : At least 40 credit points accrued in courses of SCQF Level 9 or 10 drawn from Schedule Q. Variants? This course has variants for part year visiting students, as follows
Subject AreasHome subject areaUndergraduate (School of Physics), (School of Physics, Schedule Q) Delivery Information? Normal year taken : 4th year ? Delivery Period : Semester 1 (Blocks 1-2) ? Contact Teaching Time : 2 hour(s) per week for 11 weeks First Class Information
All of the following classes
Summary of Intended Learning Outcomes
Upon successful completion of this course, it is intended that a student will be able to:
Astronomical Statistics 1)Describe the axioms of probability and be able to apply them to problems 2)Derive the Binomial, Poisson and Gaussian distributions and their application in probability 3)Explain the Central Limit Theorem, and show its general importance in probability and statistics 4)Understand how to fit models and estimate parameters using the Least Squares fit and Maximum Likelihood methods 5)Discuss Bayes Theorem and distinguish Baysian and Frequentists approaches to probability and statistics 6)Understand and be able to apply non-parameteric statistics such as the chi-squares, Kolomogorov-Smirnov, and Spearman tests X-Ray Astronomy 1)Understand the radiation processes giving rise to X-ray emission, and describe the astrophysical situations in which these take place 2)Demonstrate an understanding of the thermal emission of galaxy clusters, apply hydrostatic models to these, and discuss the interpretation of the results in a cosmological context 3)Explain the different modes of gas accretion onto black holes, and summarise the differences in their observable properties 4)Review the observational evidence for supermassive black holes, and describe the X-ray properties of active galactic nuclei Assessment Information
Degree Examination, 100%
Exam times
Contact and Further InformationThe Course Secretary should be the first point of contact for all enquiries. Course Secretary Mrs Linda Grieve Course Organiser Prof Alan Heavens School Website : http://www.ph.ed.ac.uk/ College Website : http://www.scieng.ed.ac.uk/ |
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