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Saving the results

The measurements, as shown in the Spectral fitting results: table can be written out to a text file. Just select the File->Save line fits item and either pick an existing file to overwrite, or enter a new file name. The format of this file is very simple, as shown by the following example (long lines are wrapped for presentation):
# File created by Starlink SPLAT-VO

# Quick results:
# ID Peak Centre Width Equiv Flux Asym	
0 0.5280543 4101.737 9.664325 0 8.636 1.046

# Gaussian results:
# ID Peak PeakErr Centre CentreErr Width WidthErr FWHM FWHMErr	
# Flux FluxErr Rms	
0 0.47457 0.013518 4101.637 0.20611 6.266466 0.2061116 14.7564 0.4853556 
7.454487 0.3243526 0.03108123 

# Lorentzian results:
# ID Peak PeakErr Centre CentreErr Width WidthErr FWHM FWHMErr	
# Flux FluxErr Rms	
0 0.5306862 0.00502416 4101.669 0.05490553 4.108373 0.05540269 11.62023 0.1567025 
9.686626 0.1596041 0.009050248 

# Voigt results:
# ID Peak PeakErr Centre CentreErr Gwidth GwidthErr Lwidth	
# LwidthErr FWHM FWHMErr Flux FluxErr Rms	
0 0.5308469 0.0120453 4101.668 0.05545499 0.6207013 0.7700358 11.48657 0.3663733 
11.68279 0.4136257 9.687501 0.1166889 0.009053993
So each fit type has a section in which the results for each line are shown. Lines are uniquely identified by their ID value.

Accelerator keys



next up previous 104
Next: The filter spectrum window
Up: The spectral line fitting window
Previous: The spectral line fitting window

SPLAT-VO -- A VO-enabled Spectral Analysis Tool
Starlink User Note 243
Peter W. Draper & Mark Taylor
19 December 2008
E-mail:splat@star.rl.ac.uk

Copyright (C) 2001-2005 Council for the Central Laboratory of the Research Councils
Copyright (C) 2006-2007 Particle Physics and Astronomy Research Council
Copyright (C) 2007-2008 Science and Technology Facilities Council