next up previous 79
Next: Extinction
Up: Classified list of commands
Previous: Fibre data


Flux calibration

ABCONV -- Convert spectrum from Janskys into AB magnitudes
CALDIV -- Generate calibration spectrum from continuum standard spectra
CFIT -- Generate a spectrum using the cursor
CSET -- Interactively set regions of a spectrum to a constant value
CSPIKE -- Create calibration spiketrum given spiketrum & standard spectrum
FIGSFLUX -- Flux calibrates a FIGS spectrum
FLCONV -- Convert a spectrum in Janskys into one in Ergs/cm**2/s/A
FWCONV -- General unit conversion for spectra
GSPIKE -- Generates a 'spiketrum' from a table of values
INTERP -- Interpolates between the points of a 'spiketrum' -$>$ a spectrum
IRFLUX -- Flux calibrates an IR spectrum using a black-body model
LINTERP -- Linear interpolation between spiketrum points -$>$ spectrum
NCSET -- Set a region of a spectrum to a constant
SFIT -- Fit a polynomial to a spectrum
SPFLUX -- Applies a flux calibration spectrum to an observed spectrum
SPIED -- Interactive spiketrum editor
SPIFIT -- Fits a global polynomial to a spiketrum -$>$ a spectrum



next up previous 79
Next: Extinction
Up: Classified list of commands
Previous: Fibre data

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