FIEStool master frames
Whenever new calibration data are taken using the fies-calibs script,
the calibration data are automatically reduced into master frames.
Each set of master frames is stored.
It should always be best to create master frames using calibration
frames that were taken as part of your run. However, you may want to
copy over another set of master frames as a starting point (first guess)
for the reduction with FIEStool. This to limit manual interaction to
a minimum for the order definition and for the wavelength solution.
Recent sets of master frames can be found on our FTP server.
For older sets, please contact staff.
To be able to use these masterframes in your personal FIEStool, you
have to use the same file names and parameters as are used at the NOT.
In the window 'Edit all settings' make sure the file names and
parameters agree, and pay in particular attention to the values
of the following boxes:
Values for the new CCD (CCD15):
Order definition reference | ...../master_orderdef.fits |
Wavelength reference frame | waveref.fits |
Master wavel. ref. frame | ...../master_waveref.fits |
x_start | 101 |
x_end | 2149 |
y_start | 46 |
y_end | 2049 |
Values for the old CCD (CCD13):
Order definition reference | ...../master_orderdef.fits |
Wavelength reference frame | waveref.fits |
Master wavel. ref. frame | ...../master_waveref.fits |
x_start | 51 |
x_end | 2098 |
y_start | 3 |
y_end | 2048 |
|