Parameter | Mand | Type | Default | Constraints |
imageset | yes | filename | image.fits | |
Name of EPIC FITS image |
attitudeset | yes | filename | attitude.fits | |
Name of attitude file |
eventset | yes | filename | events.fits | |
Event file, providing bad pixel and exposure extensions |
expimageset | yes | list of filenames | expimage.fits | |
Name(s) of output exposure image(s) |
withdetcoords | no | boolean | false | |
If true, the exposure map will be output in detector coordinates.
In this case, the input image(s) have to be binned in detector coordinates DETX, DETY. |
withvignetting | no | boolean | true | |
If true, the exposure map will include vignetting |
usefastpixelization | no | boolean | true | |
If true, a speed increase
of up to a factor of two is achieved, at the cost of inaccurate exposure
values in border pixels |
attrebin | no | float | 4.0 | [0.0param60.0] |
Positional accuracy of attitude rebinning in
arcseconds. Changes in the attitude less than
attrebin are ignored when rebinning the attitude data. Set attrebin=0.020626481 (i.e., rad) or smaller to ensure that the output sky exposure map matches event lists. |
pimin | no | integer | 2000 | [0param30000] |
Lower PI energy boundaries of exposure images |
pimax | no | integer | 4500 | [0param30000] |
Upper PI energy boundaries of exposure images |
usedlimap | no | boolean | false | |
If true, use discarded line maps provided by epexposure |
Parameter | Mand | Type | Default | Constraints |