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  • Ast 305
    Thunch astro ph CO ADS InSpire Radiative Processes Astro 305 MTh 3 00 4 30 AAC 107 The textbook for this course is Rybicki and Lightman Radiative Processes in Astrophysics J Wiley 1979 Please purchase this book from Amazon or your local bookstore Grades will be based on problem sets 50 in class open notes midterm 20 and in class open notes final 30 Problem Sets Problem sets will be

    Original URL path: http://background.uchicago.edu/~whu/Courses/ast305_10.html (2015-06-26)
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  • Ast 307
    ADS InSpire Research Preparation Astro 307 MW 1 30 2 50 TACC 41 This course is designed to prepare you for summer research projects Here is a semi random outline Project Initiation Hashing out idea with advisor Sanity checks and order of magnitude reasoning dimensional analysis Literature search citation trail Try to reproduce known result to test understanding Project Development Keep good notes preferably electronic and collaboration friendly CVS SVN Dropbox Wiki Google Docs Code Keep modular Version control Document as much as possible especially after finishing modular portion Informative variable names even if cumbersome Figures can be rough see presentation but label sufficiently to recall later Project Presentation Figures figures figures Will work in class to perfect technique Minimalist less is more Immediately obvious what main point is Content visually distinguishable in all presentation forms colors line type line width Text legible at journal size and projected for talks never smaller than the journal text Line art in vector format eps pdf Overlay images in raster format png jpeg with vector labels and text Write from the inside out abstract last Don t be afraid to restructure or streamline Construct paper as if giving a talk not as a

    Original URL path: http://background.uchicago.edu/~whu/Courses/ast307_12.html (2015-06-26)
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  • Ast 408
    nbsp Review 02 nbsp Power Animations nbsp Lensing nbsp Power Prehistory nbsp Legacy Material 96 nbsp PhD Thesis 95 Baryon Acoustic Oscillations Cosmic Shear Clusters Transfer Function WMAP Likelihood Reionization PPF for CAMB Halo Mass Conversion Cluster Abundance Cosmology 321 Current Topics 282 Galaxies and Universe 242 Radiative Processes 305 Research Preparation 307 GR Perturbation Theory 408 Advanced CMB 448 University of Chicago Astronomy Department KICP Thunch astro ph CO

    Original URL path: http://background.uchicago.edu/~whu/Courses/ast408_13.html (2015-06-26)
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  • Ast448
    Likelihood Reionization PPF for CAMB Halo Mass Conversion Cluster Abundance Cosmology 321 Current Topics 282 Galaxies and Universe 242 Radiative Processes 305 Research Preparation 307 GR Perturbation Theory 408 Advanced CMB 448 University of Chicago Astronomy Department KICP Thunch astro ph CO ADS InSpire Advanced CMB Astro 448 MW 1 30 2 50 TAAC 41 This course will have be composed of 2 parts The first half will be lecture

    Original URL path: http://background.uchicago.edu/~whu/Courses/ast448_15.html (2015-06-26)
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  • Group
    astro ph CO ADS InSpire Student Projects Dead links from old projects have been removed Graduate Integrated Late ISW Effect and CMB LSS Cross Correlation Alessandro Manzotti Squeezing the CMB Alan Zablocki Studying Extragalactic Point Sourcs with the SPT Monica Mocanu Galileon Cosmology Yin Li Features in DBI Inflation Vinicius Miranda Analytical Reionization Models and CMB Alexander Kaurov Practical lessons in extracting cosmology from the CMB Benedikt Diemer Measurement of

    Original URL path: http://background.uchicago.edu/~whu/Courses/studentprojects.html (2015-06-26)
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  • Group
    Oscillations Cosmic Shear Clusters Transfer Function WMAP Likelihood Reionization PPF for CAMB Halo Mass Conversion Cluster Abundance Cosmology 321 Current Topics 282 Galaxies and Universe 242 Radiative Processes 305 Research Preparation 307 GR Perturbation Theory 408 Advanced CMB 448 University of Chicago Astronomy Department KICP Thunch astro ph CO ADS InSpire Numerical Projects This page is deprecated and will be replaced next time the course is offered External links may

    Original URL path: http://background.uchicago.edu/~whu/Courses/projects.html (2015-06-26)
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  • test.html

    (No additional info available in detailed archive for this subpage)
    Original URL path: /~whu/intermediate/ringing.html (2015-06-26)


  • Inflation
    originated in an inflationary epoch the universe is spatially flat and baryonic dark matter is required We discuss the underlying assumptions of these claims and outline the tests required to ensure they are robust The most critical test the presence of a second feature at the predicted location should soon be available Further in the future secondary anisotropies and polarization should open new windows to the early and low er

    Original URL path: http://background.uchicago.edu/~whu/decadent/decadentpage.html (2015-06-26)
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