Analysing Data Recorded with Azimuthal Setups

It is quite obvious that an azimuthal mount causes field rotation, when not used on the North- or the South-pole. For real long exposures (i.e. minutes to hours) this is utterly devastating for every image taken.
Here the abilities and power of CCDs are coming into play. With exposure times of a couple of seconds, field rotation does not play any role for the single frame. As long as the CCD amplifier ensures that the charge in a single pixel is high enough to result in a signal greater than the detection threshold we can integrate over several different frames. Now field rotation will return when not properly taken care of .


IRIS however is capable to compensate for rotation between individual frames during alignment. Lets see what is to be done, on a step by step basis, assuming the raw fits series (after conversion) is called r#.fits (for red), g#.fits (for green) and b#.fits (for blue). Furthermore assume that the data set contains 50 frames.

Have a look at an example analysis done on M52 data. Both results came from the same data set, analysed in different ways.




M52, ETX-70, analysed with K3CCDTools, dark frame subtracted

M52, ETX-70, analysed as described above, no dark frame subtraction





last modified 10.01.05