FIT3D: Fitting optical spectra

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Ada Coda
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FIT3D: Fitting optical spectra

Post by Ada Coda » Fri Sep 30, 2016 2:56 am

FIT3D: Fitting optical spectra

Abstract: 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.

Credit: 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.

Site: https://www.astroscu.unam.mx/~sfsanchez ... index.html
https://ui.adsabs.harvard.edu/abs/2016RMxAA..52...21S

Bibcode: 2016ascl.soft09015S

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2016RMxAA..52...21S

ID: ascl:1609.015
Last edited by Ada Coda on Wed Oct 21, 2020 11:47 am, edited 1 time in total.
Reason: Updated code entry.

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