BESTFIT 1.11
Authors/Creators
Description
First public release of BESTFIT Ivano Baronchelli 2018
IDL based SED fitting code for stellar templates V1.1 Ivano Baronchelli 2018 BESTFIT is an IDL based function that can be used to fit photometric data using a collection of template models of stellar spectra. The method used is based on the χ 2 minimization technique. Chosing among a collection of models (internal or supplied by the users), BESTFIT computes the spectral model that better fits the input photometric data. BESTFIT also predicts the expected flux in a users-selected photometric filter (or at a given wavelength). This can be useful in all those cases in which a rough photometrical calibration of the fluxes in a given band is needed or when the user wants to check the photometric calibration in a given band. The parameters and filters files look similar to those used by the hyperz software (Bolzonella+2000). This should make the use easier for people that previously used hyperz.
For installation instructions and manual see the BESTFIT pdf manual included in this folder
Files
Ibaronch/BESTFIT-1.11.zip
Files
(42.3 MB)
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Additional details
Related works
- Is supplement to
- https://github.com/Ibaronch/BESTFIT/tree/1.11 (URL)
References
- Baronchelli, I. et al. (2016)
- Baronchelli, I. et al. (2018)