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SPIED-Interactive spiketrum editor

Description:
SPIED allows the user to edit a spiketrum - deleting points and adding new points - in order to control the spectrum obtained by interpolating between the points (e.g. by INTERP or SPIFIT).

Parameters:
SPIKETRUM
The spiketrum to be edited (probably generated either by CSPIKE or by GSPIKE). For more details see HELP FIGARO TECHNIQUES SPIKETRA.
OUTPUT
The name of the resulting edited spiketrum. It may be the same as SPIKETRUM, in which case the result will replace the input in the same file.
COLOUR
The colour for the data to be plotted in. The axes are always plotted in white. The colours allowed are Blue, White, Red, Green, Black, Cyan, Magenta, Yellow. This only works on a colour display, of course. Fitted data will be plotted in the complementary colour
HIGH
The maximum Y value for the plot.
LOW
The minimum Y value for the plot.
XSTART
The maximum X value for the plot.
XEND
The minimum X value for the plot.
ORDER
The order for the polynomial fit.
QUIT
Used to confirm quitting from application.

Source comments:
 S P I E D

 SPIketrum EDitor.  Allows the values of a spiketrum to be
 edited interactively, until the user is satisfied with the
 data that results from interpolating between them.

 Command Parameters -

 SPIKETRUM    (Character) The name of the spiketrum to be
              edited.
 OUTPUT       (Character) The name of the resulting edited
              spiketrum.
 COLOUR       (Character) The colour to be used for the data
              when it is ploted.
 HIGH         (Real) The maximum Y value for the plot.
 LOW          (Real) The minimum Y value for the plot.
 XSTART       (Real) The maximum X value for the plot.
 XEND         (Real) The minimum X value for the plot.
 ORDER        (Integer) The order for the polynomial fit.

 Command keywords -

 QUIT         Used to confirm quitting from application.

 User variables used -    (">" input)

 (>) SOFT     (Character) The device/type of the current soft
              graphics device.

                                    KS / CIT 23rd May 1984


next up previous 79
Next: SPIFIT-Fits a global polynomial to a spiketrum to form a spectrum
Up: Applications in detail
Previous: SPFLUX-Applies a flux calibration spectrum to an observed spectrum

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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