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Interested in a simple fitting code that models OIII, Hbeta, NII, Halpha and SII emission lines in an IFS data cube? You are at the right place. The python code here provides a very basic fitting routine that does a simple Gaussian fit to these optical emission lines in an IFS data cube. The code has been adapted specifically for MUSE.
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darshankakkad/ifuviz
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Interested in a simple fitting code that models OIII, Hbeta, NII, Halpha and SII emission lines in an IFS data cube? You are at the right place. The python code here provides a very basic fitting routine that does a simple Gaussian fit to these optical emission lines in an IFS data cube. The code has been adapted specifically for MUSE.
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