I am working on astrometric
registration of Magellan Megacam images. My first task was to read
the multi-extension FITS files. The image files I have possess 36
extensions, each corresponding to one of Megacam's 36 detectors. The
order of the extensions follows four columns of nine detectors each,
starting at the southwest corner of the mosaic. Thus extension 2 is
for the detector immediately north of extension 1, and so on up
through extension 9, which is the ninth detector of the first column
and hence is at the north edge of the mosaic. Then extension 10 is
for the first detector of the second column, and is immediately to
the east of extension 1. This is a very sensible way of arranging
the detectors and extensions.
One thing that confused me at first is
that although the third and fourth columns have the detectors ordered
exactly as you would expect based on the above, each detector image
in these columns is upside-down relative to the corresponding images
in the first and second columns. One can understand how this might
come about due to spatial constraints on the positioning of readout
electronics.
No comments:
Post a Comment