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- IMage
- (file) Name of image for input. This should be a file
containing continua spectra.
- 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
- OLD (O)
- Correct using previous results
- OUtput
- (file) Name of output file. File to contain
corrected data.
- XStart
- (int) analysis lower limit. The data between the
limits xstart and xend is extracted and the resultant spectrum is used
to locate the lines.
- XEnd
- (int) analysis upper limit. The data between the
limits xstart and xend is extracted and the resultant spectrum is used
to locate the lines.
- XBlock
- (int) Enter averaging width in channels. Each
window is of this width (except perhaps the final one).
- ITeration
- (short) New value of iteration
- LEvel
- (float) Level of edge of tooth
- ORder
- (int) order for polynomial fitting This is for the
continuity correction of the data.
- 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 comb spectrum.
- TOls
- (char) For use in batch only
- KEEP_ITT
- (key) keep iteration files?
- QUick
- (key) Centroid rather than fit Gaussians?
- PRFits
- (key) Print out details of fitting
- PLOtcorr
- (key) Plot correction?
Next: Main Menu
Up: COMB Correction for S-Distortion
Previous: COMB Correction for S-Distortion
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