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- IMage
- (char) Name of image for input, This is the data and should
be a FIGARO format data file.
This should also have a .X axis array which contains the wavelengths of
the lines. For the identification files supplied with the program the
units should be Ångstroms. However, if the user supplies his/her own
files, this need not apply, although some plots may have the wrong
labels.
- ARC_OPTS
- (char) Fit option:
- NEW (N)
- Set up a new analysis
- REPEAT (R)
- Iterate on previous analysis
- CLONE (C)
- CLONE an analysis from another file
- YStart
- (int) Analysis lower limit
- YEnd
- (int) Analysis upper limit
- YBlock
- (int) Analysis cross-section width
- ITeration
- (int) New value of iteration
- MAXLines
- (int) Maximum number of lines to allow room for
- CLfile
- (char) Name of image for CLONING from
- VCorr
- (real) Correction to apply to radial velocities
- TOls
- (char) For use in batch only
- INherit
- (int) Number to control inheritance of previous fits:
- 0
- no inheritance of fits
- 1
- inheritance from next block
- -1
- inheritance from previous block
- DEvice
- (char) Device to use for plotting (greyscale)
- FITRat
- (real) Ratio of widths, heights, or separation, for
double fits
- CAlrat
- (int) Ratio of number of iteration to default
- WHite
- (float) Level to plot as white (greyscale option)
- BLack
- (float) Level to plot as black (greyscale option)
- MAXGauss
- (int) Maximum number of Gaussians that can be fitted
to a profile.
- TStart
- (int) Analysis lower limit
- TEnd
- (int) Analysis upper limit
- TBlock
- (int) Analysis width in T direction
- FIT_MODEL
- (char) Model for fitting
- PLOTLim
- (float) Limits of plot (world coordinates).
This is to allow velocity plots to be forced to all have the same scale,
making comparison easier.
- HArdcopy
- (key) Produce hardcopy plots of fits from cube
- TAble
- (key) Produce table of fits from cube
- PLOT
- (key) Produce plots of rotation curves
- PRInt
- (key) Produce print out of rotation curves
- KEEP_ITT
- (key) Keep iteration files. These files contain
details of the fitting process. If a fit succeeds the file is always
deleted, if it crashed it is always kept, this keyword controls
whether it is deleted if a NAG error occurs.
- FIT
- (key) Perform fitting
- COPY
- (key) Copy previous fits This will repeat all the fits
previously made, which is likely to be of use if data is co-added after
one file has been analysed. Also, when used with CLONE the entire .RES
structure is copied without any change. For the new fits the previous
fits (suitably scaled) are used as first guesses.
- ABsorption
- (key) Allow fitting of absorption lines.
This allows absorption fits to be defined--once defined they can be
fitted whatever the value of this.
- BOunds
- (key) Perform bounded fits to lines (in batch).
This only bounds the widths.
- LAbel
- (key) Put labels on plots.
This is true by default, but it may be preferable if plots are to be
used in a paper to not have labels.
- CONtour
- (key) Produce contour plots
- GRey
- (key) Produce greyscale plots
- LOG
- (key) Use log scale for greyscale and contour plots
- WEIghts
- (key) Use weighted fitting (default is true).
- PRFits
- (key) Print out details of fitting.
This is true by default, but if you wish to avoid large log files set it
to false.
- FULL
- (key) Print out full details of fits in table.
This provides the information in a form which is easier to read into a
FORTRAN program, and includes the information given in PRINT and TABLE.
- CHECK
- (key) This produces an array of line profiles with the fits
superimposed.
The options HARDCOPY, TABLE, PLOT, PRINT, SHAPE and FULL are the same
as for the OUTPUT MENU, except that in batch mode HARDCOPY
will work on all line profiles/blockings which have a successful fit.
CONTOUR and GREYSCALE work on all the lines in batch mode.
Note that the use of TSTART and TEND is with 3-dimensional data files.
At present LONGSLIT only partially supports these, but some of the same
code is used as in FIBDISP.
The keyword PRFITS is true by default but the user may set it to false
to avoid large log files when running in batch.
Next: FIBDISP Analyise 3-d Data (spectral)
Up: LONGSLIT
Previous: Use of Tolerances
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