alfa 1.0-ok1 (amd64 binary) in openkylin yangtze

 ALFA measures fluxes in emission line spectra, such as those of planetary
 nebulae and HII regions, using a genetic algorithm to rapidly optimise fits
 to large numbers of lines simultaneously. It can subtract night sky emission
 lines before fitting the nebular lines if necessary. It can read plain text
 files containing 1D spectral data, or FITS files containing 1D, 2D or 3D
 datasets.

Details

Package version:
1.0-ok1
Source:
alfa 1.0-ok1 source package in openKylin
Status:
Deleted
Component:
main
Priority:
Optional

Downloadable files