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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.