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FORS1 Wavelength Calibration Accuracy
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The determination of the dispersion relation for MOS data is done as
follows: The recipe fors_calib identifies reference lines on MOS arc
lamp exposures, and traces the spectral edges on the associated flat
field exposures. With this information the spectral extraction mask to
be applied in the scientific data reduction is determined. From the
input flat field exposures a normalised flat field frame is also
derived.
The input arc lamp and flat field exposures are assumed to be
obtained quasi-simultaneously, so that they would be described by
exactly the same optical distortions.
Wavelength calibration is performed row by row and produces a 2-D
rebinned science frame. This has the effect of removing the
instrumental line curvature and allows the user to extract her/his
spectra and have them wavelength calibrated without any additional
operation on the frame itself.
The global list
of lines currently used by FORS1 pipeline can be found here.
Due to the high number of possible grism/slit combinations, the
Pipeline currently uses a polynomial with a maximum degree of 5 (for
150I without filters) in the dispersion direction, while a 2nd
order polynomial is adopted in the spatial direction.
Currently (November 2006) the pipeline supports all grisms.
The current version of the Pipeline is known to have some problems with
extreme offsets, that result in arc spectra with few lines.