[MENU BAR] [File] This menu provides the following functions: This option allows to read in data from a file, which are required for fitting a model. For the of the file, please see the manual or the files included in the distribution. Before reading in data for a new binary star, you should use this button to delete data for the current binary, otherwise you would have a mixture of data for different stars in memory. It is not possible to selectively delete only part of the data. Allows you to read in a file defining the geometry of a binary system. For the of the file, please see the manual or the files included in the distribution. that the latter include commands to read data, thus you should use before using this option. This will write the current geometry of the binary system (including spots etc.) to a file for later use. Commands for reading in the data files currently in memory will be included as well. For closing the application. [Output] This menue allows to use the available output options: plots the computed lightcurve. If observational data are available for the selected filter, they will be overplotted. The output filter and the part of the lightcurve plotted can be selected from panel . You need to compute a lightcurve first to use this option. gives you the opportunity to see the binary as a nearby observer would see it. The phase angle and the inclination of the orbital plane can be set interactively. allows you to view a slice through the Roche potential. You can interactively switch between the X-Y plane (the orbital plane) and the X-Z plane (perpendicular to the orbital plane). You can also choose interactively the height above the selected plane. some nifty plots (non-interactive version of and , basically). opens a window with the data on the binary star system, including things like individual masses of the stars, largest radius ({Point Radius}) and smallest radius ({Polar} {Radius}), mean temperatures etc. Basically, this is the header of the output file {NightfallCurve.dat}. shows the profile of an absorption line in the spectrum of the star. You can change the phase interactively. You need to compute the line profile first to use this option.