TSX: TripleSpec eXtraction: Wavelength Solution
- Line identifications:
- Polynomial Formulae:
Polynomial coeffecients.
- Plots of night sky lines:
- Night sky spectra (ASCII tables) (average of 11 x 300s exposures):
- Accuracy of wavelength solution.
The RMS error of the wavelength solution used for all reductions
is about 0.1 to 0.3 pixels or about 0.5 Angstroms. The shift applied
to each individual extraction is generally about 0.2 pixels.
Last modified: 29 May 2014