Originally reported by: mknoetig (Bitbucket: mknoetig, GitHub: mknoetig)
Hi guys,
I was working on a comparison of MAGIC and FACT data when I wanted to rotate the Theta[x] and Theta[y] coordinates back into the sky coordinates RA/DEC. I have written down a couple of things and will present those in a more comprehensive file. For now I wanted to point out two peculiarities of our system that I had to find first..
This first issue is about the code in SourcePosition.java .There, Fabian defines implicitly a second azimuth, parallel to the one stored in container "AzTracking". This ine os called "AzPointing".
From our discussions, following things about our azimuth got clear:
1.) AzTracking = -180deg -AzPointing
2.) AzTracking should not be used, as it is "uncorrected", in a sense.
Please find attached a plot displaying these issues. Maybe it would be useful, in order to get towards skymaps, to introduce a branch with proper coordinate transformations between all possible coordinate systems ( camera x/y, alt/az, ra/dec, ha/dec, ... ) that work on one consistent definition of the individual systems.
Originally reported by: mknoetig (Bitbucket: mknoetig, GitHub: mknoetig)
Hi guys,
I was working on a comparison of MAGIC and FACT data when I wanted to rotate the Theta[x] and Theta[y] coordinates back into the sky coordinates RA/DEC. I have written down a couple of things and will present those in a more comprehensive file. For now I wanted to point out two peculiarities of our system that I had to find first..
This first issue is about the code in SourcePosition.java .There, Fabian defines implicitly a second azimuth, parallel to the one stored in container "AzTracking". This ine os called "AzPointing".
From our discussions, following things about our azimuth got clear:
1.) AzTracking = -180deg -AzPointing
2.) AzTracking should not be used, as it is "uncorrected", in a sense.
Please find attached a plot displaying these issues. Maybe it would be useful, in order to get towards skymaps, to introduce a branch with proper coordinate transformations between all possible coordinate systems ( camera x/y, alt/az, ra/dec, ha/dec, ... ) that work on one consistent definition of the individual systems.