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Have you ever stopped at a construction project on the way to your of?ce and the day’s astrophysics? Remember the other onlookers – folks just enjoying the sp- tacle, as we all do in following developments away from our areas of active work? We are excited and thrilled when the Hubble Space Telescope discovers an Einstein Cross, when the marvelous pulsars enter our lives, and when computer scientists put a little box on our desk that outperforms yesterday’s giant machines. We are free to make use of such achievements and we respect the imagination and discipline needed to bring them about,…mehr
Have you ever stopped at a construction project on the way to your of?ce and the day’s astrophysics? Remember the other onlookers – folks just enjoying the sp- tacle, as we all do in following developments away from our areas of active work? We are excited and thrilled when the Hubble Space Telescope discovers an Einstein Cross, when the marvelous pulsars enter our lives, and when computer scientists put a little box on our desk that outperforms yesterday’s giant machines. We are free to make use of such achievements and we respect the imagination and discipline needed to bring them about, just as onlookers respect the abilities and planning needed to create a building they may later use. After all, each of us contributes in our own areas as best as we can. In addition to the serious onlookers there will be passersby who take only a casual look at the site. They may use the building later, but have little or no interest in its construction and give no thought to the resources needed tobring it to completion. Upon arriving at work, those persons write astronomy and astrophysics books at various levels, in which they must say something about close binary stars. Usually a page or two will do, and the emphasis is on the MLR (mass, luminosity, radius) data obtained only from binaries.
Prof. Dr. Josef Kallrath ist in der Praxis und Lehre tätig und löst mit Wissenschaftlichem Rechnen praktische Probleme in der Industrie. Schwerpunkt seiner Tätigkeit ist die Mathematische Optimierung zur Unterstützung von Entscheidungsprozessen und die Modellierung physikalischer Systeme. Lehrtätigkeiten übte er an der Universität Heidelberg und derzeitig an der University of Florida in Gainesville/USA aus. Seit 2002 leitet er die Arbeitsgruppe 'raxis der mathematischen Optimierung' der Gesellschaft für Operations Research (GOR).
Inhaltsangabe
I Introduction.- The Database and Methods of Data Acquisition.- II Modeling and Analysis.- A General Approach to Modeling Eclipsing Binaries.- Determination of Eclipsing Binary Parameters.- Advanced Topics and Techniques.- III Light Curve Programs and Software Packages.- Light Curve Models and Software.- TheWilson#x2013;Devinney Program: Extensions and Applications.- Light Curve Software with Graphical User Interface and Visualization.- The Structure of Light Curve Programs and the Outlook for the Future.
Introduction.- The Data Base and Methods of Acquisition.- A General Approach to Modeling Eclipsing Binaries.- Determination of Eclpsing Binary Parameters.- Light Curve Models and Software.- The Wilson-Devinney Program and WD95.- The Structure of Light Curve Programs and the Outlook for the Future.- Appendix A: A Brief Review of Mathematical Optimization.- Appendix B: Estimation of Fitted Parameter Errors: the Details.- Appendix C: Geometry and Coordinate Systems.- Appendix E: Subroutines of the Wilson-Devinney Program.- Appendix F: Graphics Utilities and Visualization.- Appendix G: Glossary of Symbols.- Bibliography.- Subject Index.
I Introduction.- The Database and Methods of Data Acquisition.- II Modeling and Analysis.- A General Approach to Modeling Eclipsing Binaries.- Determination of Eclipsing Binary Parameters.- Advanced Topics and Techniques.- III Light Curve Programs and Software Packages.- Light Curve Models and Software.- TheWilson#x2013;Devinney Program: Extensions and Applications.- Light Curve Software with Graphical User Interface and Visualization.- The Structure of Light Curve Programs and the Outlook for the Future.
Introduction.- The Data Base and Methods of Acquisition.- A General Approach to Modeling Eclipsing Binaries.- Determination of Eclpsing Binary Parameters.- Light Curve Models and Software.- The Wilson-Devinney Program and WD95.- The Structure of Light Curve Programs and the Outlook for the Future.- Appendix A: A Brief Review of Mathematical Optimization.- Appendix B: Estimation of Fitted Parameter Errors: the Details.- Appendix C: Geometry and Coordinate Systems.- Appendix E: Subroutines of the Wilson-Devinney Program.- Appendix F: Graphics Utilities and Visualization.- Appendix G: Glossary of Symbols.- Bibliography.- Subject Index.
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