next up previous index 116
Next: 12:ech_scrunch Scrunch
Up: ECHOMOP TASKS & ECHMENU OPTIONS
Previous: 10:ech_idwave Wavelength Calibrate


11:ech_blaze--Fit and Apply Ripple Correction

This option consists of two steps as follows:

If flux calibration is not being performed it is sometimes desirable to remove the `blaze' function from the extracted spectrum to assist in fitting line profiles etc. during data analysis.

A task is provided for this purpose which operates by fitting curves to the flat-field orders. The curves can be polynomials, splines or simple fits based on local-median values. The fits may be automatically or interactively clipped and the resulting blaze spectrum is normalised such that its median intensity is unity.

The normalised blaze is then divided into the extracted spectrum. It is important to remember that this operation is performed upon the `extracted' spectrum.

After a blaze function has been applied to the extracted order all its values may be reset to unity to ensure that the order(s) cannot be re-flattened in error (TUNE_BLZRSET=YES). If the blaze is to be re-applied then the correct procedure is to first re-extract the order(s) concerned and then re-fit the blaze.

Parameters:

Reduction File Objects:


next up previous index 116
Next: 12:ech_scrunch Scrunch
Up: ECHOMOP TASKS & ECHMENU OPTIONS
Previous: 10:ech_idwave Wavelength Calibrate
ECHOMOP-Echelle Data Reduction Package
Starlink User Note 152
Norman Gray
2003 July 14
E-mail:norman@astro.gla.ac.uk

Copyright © 2003 Council for the Central Laboratory of the Research Councils