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Useful recipes
a) Low spectral resolution spectra (e.g. line strengths for single
emission lines)
CUR ORD SIG/ERR ITN FIT GAU
LIM SIN CON
b) High spectral resolution spectra (e.g. radial velocity structure of
a single profile)
CUR ORD SIG/ERR ITN FIT GAU
LIM NEW INCH NEX INCH NEX
INCH SEL INCH OPT HARD QUIT
Next: Gauss: Format of data file
Up: Gauss-A Figaro program for interactive Gaussian fitting
Previous: Running the program
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