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This process would involve the following steps:
- Check the input file for duplicate points in the x-scale. If there
are any duplicate points for the same detector, then they should be
averaged.
- Specify the new reference x-scale. This could be:
- Equidistant, giving start wavelength, end wavelength and number of
steps or start wavelength, step width and number of steps.
- Consistent with a given resolution, giving start wavelength, end
wavelength and resolution.
- Interpolate the y-values in the input spectrum to the new reference
x-scale using:
- Linear interpolation (flux conserving)
- Cubic spline interpolation
- Polynomial interpolation
N.Trams, ISO Science Operations Team
Using inputs from:
C.Gry, T. Lim, LWS Instrument Dedicated Team
A.Harwood, P.E.Clegg, B.Swinyard, K.King, LWS Instrument Team
S.Lord, S.Unger, IPAC.