REGISTER/ROMAFOT int_tab reg_tab [wnd_opt] [obj_opt]
This command creates a table with the results of the analysis. However, all the photometric information obtained from the frame as the absolute quantities (magnitudes, colour equations etc.) still have to be derived. In this output table every object occupies one row and the data are stored according the Table .
Table: Romafot Registration Table
The magnitudes MAG1, MAG2 and MAG3 (e.g. U, B and V) are accepted by the commands FIND/ROMAFOT or SELECT/ROMAFOT and are necessary for calibration. In case of program stars (search made with SEARCH/ROMAFOT), these columns are filled with zeros.
The instrumental magnitude MAG_CNV is calculated as , where VOL is the integral over the elementary surface to fit the star, calculated from to . In case of linear data this is expected to differ from the magnitude by a constant.