• An ndf called $<$bolname$>$_map (e.g. h7_map) will be created in the OUT file to hold the coadded data from all the integrations. If the jiggle pattern points fit a 2-d rectangular pattern then these data will be arranged as a 2-d map suitable for plotting as an image. A 2-d parabola will be fitted to the coadded image and the results written in ASCII form to FILE. If an irregular jiggle pattern is used the map will take the form of a 1-D strip.

• Second, an ndf called $<$bolname$>$_peak (e.g. h7_peak) will be created in the OUT file to hold the fitted results to the data for each integration. The results stored are the fit peak, its variance and quality and they are held as a 1-d array suitable for plotting as a graph. The fit results are also written in ASCII form to FILE, as is the coadd of all the individual fits to the data.

ALLBOLS = LOGICAL (Read)

ANALYSIS = CHAR (Read)

FILE = FILENAME (Write)

IN = NDF (Read)

MSG_FILTER = CHAR (Read)

OUT = CHAR (Write)

scuphot o56_lon_ext average o56_lon_pht !

• ALLBOLS must be false for 2 and 3 bolometer photometry unless you know what you are doing.

• SCUPHOT can process JIGGLE/MAP data. The output is the signal for each integration for each bolometer. This is useful for checking sky removal and should not be used for performing on-source photometry on map data! This method can not be used for SCAN/MAP data.