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Statistical testing (type I and type II errors)Īt the end of this course you will know how to prepare your own astronomical observations with a professional telescope and evaluate the results thereof. Radial velocity modelling for exo-planets Matching of black body models to photometry
Topcat leiden software#
Telescope proposals, technical and scientific justifications.Īstronomical software (review) – ds9, topcat and python The course is defined by two substantial problem sets covering part 1 and part 2, while the observing project provides substantial freedom to the students. The second part focuses on the fitting of models to observational data while the third part which runs parallel throughout the whole course, focuses on the definition and analysis of observations with the 2.5m Isaac Newton Telescope (INT) on La Palma and is carried out in groups of 3-6 students. The first part introduces the students to photometry of stellar sources using both synthetic and aperture photometry with special attention paid to practical error analysis. Each part is introduced in one or more lectures and carried out with the supervision of assistants during practical classes using computers running Linux. The scientific question will be conceived by you working in a group and will teach you how to work as a scientist.
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In the Astronomy Lab and Observing Project you will learn how to prepare and analyse astronomical observations with a professional telescope Modern Astronomical Research and Communication: Finding and reading research articles Description Programmeermethoden NA: basic knowledge of Python Inleiding Astrofysica: coordinate systems, magnitudes, basic stellar properties, HR diagram Praktische Sterrenkunde: basic error analysis, basic photometry & data reduction, 2-parameter linear chi^2 Knowledge of calculus and basic astronomical concepts.