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Summary of Parameters
- IMage
- (file) Name of image for input. This should be a file
containing an arc spectrum.
- ARC_OPTS
- (char) Enter arc fit option:
- NEW (N)
- set up a new wavelength calibration
- REPEAT (R)
- Iterate on previous calibration.
- CLONE (C)
- CLone a previous calibration.
- YStart
- (int) analysis lower limit The data between the
limits ystart and yend is extracted and the resultant spectrum is used
to locate the lines.
- YEnd
- (int) analysis upper limit. The data between the
limits ystart and yend is extracted and the resultant spectrum is used
to locate the lines.
- YBlock
- (int) Enter analysis x-sect width Each window is
of this width (except perhaps the final one).
- ITeration
- (short) New value of iteration
- ORder
- (int) order for polynomial fitting This is for the
continuity correction of the data. Ideally the arc should have been
pre-processed with ARCSDI, so a low order e.g. 2 should be used.
- MAXLines
- (int) Maximum number of lines to allow room for.
This must be greater than or equal to the number of lines fitted, so
room should be allowed in case any more are to be added later.
- CLfile
- (file) Name of image for cloning from. This should
be a file containing an arc spectrum.
- TOls
- (char) For use in batch only
- KEEP_ITT
- (key) keep iteration files
- PRFits
- (key) Print out details of fitting
Next: COMB and ARCSDI-Correction for Geometrical Distortions
Up: ARC2D Wavelength Calibration
Previous: Evaluating the Dispersion Relation
FIGARO A general data reduction system
Starlink User Note 86
Keith Shortridge, Horst Meyerdierks,
Malcolm Currie, Martin Clayton, Jon Lockley,
Anne Charles, Clive Davenhall,
Mark Taylor, Tim Ash, Tim Wilkins, Dave Axon,
John Palmer, Anthony Holloway and
Vito Graffagnino
2004 February 17
E-mail:starlink@jiscmail.ac.uk
Copyright © 2013 Science and Technology Facilities Council