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ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

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336 APPENDIX E. <strong><strong>ISO</strong>CAM</strong> ASTROMETRY: ANGLES AND COORDINATES<br />

E.3.2<br />

From CIA structures to FITS images<br />

The main problem is to know which angle to supply to the fits header routine. It obviously<br />

depends on the type of data.<br />

E.3.2.1<br />

Individual SCDs and the like<br />

This works also for an SAD that would be the average of an SCD, for a reduced beam-switch or<br />

CVF. The only angle that is valid in that case is the ROLL, or α. The obvious way to transfer<br />

the data is to avoid unnecessary rotations during the transfer, thus the Y+ axis will be Axis1<br />

and the Z- axis will be Axis2 (see Figures E.1 and E.5).<br />

The angle that needs to be given to fits header, CROTA2, is then the position angle of<br />

the North axis with respect to the Z- axis. Thus:<br />

θ = 360 ◦ − α<br />

or<br />

CROTA2 = 360 ◦ - ROLL<br />

E.3.2.2<br />

Reconstructed raster images<br />

In that case, the meaningful angle is .RASTER ROTATION, β. The individual images can no<br />

longer be distinguished therefore their ROLL is irrelevant to the raster (it is only coincidentally<br />

meaningful for Y-axis rasters). Here also the simplest way to store the image is to have the M+<br />

axis be Axis1 and the N+ axis be Axis2. Thus, from Figures E.3 and E.5 one has:<br />

θ =90 ◦ − β<br />

or<br />

CROTA2 = 90 ◦ -RASTERROTATION

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