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Summary of Parameters

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?



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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

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