Closed tariq-shahbaz closed 2 years ago
Hi Tariq, was this not in fact a problem? (I have an ambition to attempt a more generalised astrometric solution to all hipercam / ultracam etc data, but don't wait up)
Hi Tom
Mmm, yes you could say that. In the end I used "hpackage" package to create the fits files on the individual CCDs (with the bias and flats in the same directory, tar=yes) then then unpacked the tar file.
After plotting the i-band images taken on different nights, I have noticed that the WCS are different. Stars are not in the same position (see chart attached). Shame as I wanted to plot the position of possible brown dwarfs and it would save a lot of hassle if I could just use the HiPERCAM WCS . Not sure how you can do this if you do not have stars in the field you can use for calibration.
Maybe I am doing something silly in python!, but I am seeing Vik next week and hopefully he or Stu can help
Cheers
Tariq
p.s.
AR Sco, found it in my spam! I am still at the IAC.
On Wed, 18 May 2022 at 09:55, Tom @.***> wrote:
Hi Tariq, was this not in fact a problem? (I have an ambition to attempt a more generalised astrometric solution to all hipercam / ultracam etc data, but don't wait up)
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The WCS I apply is really crude -- it just comes straight from the telescope, so absolutely no surprise to hear that the stars "move". The WCS needs to be tweaked from the star positions -- you might know how to do this better than me. My long term aim is to use astrometry.net, but that is long term. The existing method is just a stop gap.
Sometimes hpackage does not add the WCS information to the headers. CCD 1: missing positional data; no WCS added whereas using joinup there seems to be no problem.
It would be used to print out what header items are missing in hpackage.