ASCL Code Record
[ascl:1609.015]
FIT3D: Fitting optical spectra
Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P.; González, J. J.; Rosales-Ortega, F. F.; Cano-Díaz, M.; López-Cobá, C.; Marino, R. A.; Gil de Paz, A.; Mollá, M.; López-Sánchez, A. R.; Ascasibar, Y.; Barrera-Ballesteros, J.
FIT3D fits optical spectra to deblend the underlying stellar population and the ionized gas, and extract physical information from each component. FIT3D is focused on the analysis of Integral Field Spectroscopy data, but is not restricted to it, and is the basis of Pipe3D, a pipeline used in the analysis of datasets like CALIFA, MaNGA, and SAMI. It can run iteratively or in an automatic way to derive the parameters of a large set of spectra.
- Code site:
- https://web.archive.org/web/20200108120557/http://www.astroscu.unam.mx:80/~sfsanchez/FIT3D/index.html
- Described in:
- https://ui.adsabs.harvard.edu/abs/2016RMxAA..52...21S
- Bibcode:
- 2016ascl.soft09015S
Preferred citation method:
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