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: http://www.eso.org/~chummel/oyster/manual/node93.html
Дата изменения: Tue Apr 28 19:12:50 2015 Дата индексирования: Sun Apr 10 20:24:37 2016 Кодировка: Поисковые слова: annular solar eclipse |
readmodel,file_char
Read a model file.calcmodel
Compute the model data for data sets with non-zero weight.modelchisq()
Function. Return reducedbinarypos([epochof currently loaded data wrt model.
Function. Returnmodelk(componentrelative position for binary model at JD epoch. Use today if no epoch is specified, and use the top hierarchical component if no component is specified. If a component is specified, so must be the epoch. If com=1, compute relative to center of mass, not center of brightness. In the latter case, one can specify lambda (in meters) for the wavelength to use. If abs=1, return individual component positions instead of relative position. In that case, the component index is in the first dimension,
are in the second.
Function. Return velocity semi-amplitude for component. Examples: PRINT,MODELK('A'), PRINT,MODELK('AB').modelpx(component
Function. Return parallax derived from parameters of the specified component. Note that for systems higher than binaries, the results could be inconsistent, indicating an inconsistent set of model parameters.