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ASCL Code Record

[ascl:2109.012] STAR-MELT: STellar AccrRetion Mapping with Emission Line Tomography

STAR-MELT extracts and identifies emission lines from FITS files by matching to a compiled reference database of lines. Line profiles are fitted and quantified, allowing for calculations of physical properties across each individual observation. Temporal variations in lines can readily be displayed and quantified. STAR-MELT is also useful for different applications of spectral analysis where emission line identification is required. Standard data formats for spectra are automatically compatible, with user-defined custom formats also available. Any reference database (atomic or molecular) can also be used for line identification.

Code site:
https://github.com/justyncw/STAR_MELT
Described in:
https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.3331C
Bibcode:
2021ascl.soft09012C

Views: 129

ascl:2109.012
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