tools:mfit
Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision | ||
|
tools:mfit [2026/08/31 18:53] cjoblin [Installation] |
tools:mfit [2026/08/31 18:54] (current) cjoblin created |
||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | + | ===== cosmicPAHmfit ===== | |
| - | + | **Authors** : Louan de Bentzmann (CNRS, IRAP), Karine Demyk (CNRS, IRAP), Axel Pérignon (CNRS, IRAP), Vincent Marty (CNRS, IRAP), Jean-Michel Glorian (CNRS, IRAP), Christine Joblin (CNRS, IRAP) | |
| - | + | **Licence** : [[https://gitlab.in2p3.fr/ovgso/cosmic-pah/cosmic-pah-mfit/-/blob/1.1/LICENCE|GPLv3]] | |
| - | + | ==== Description ==== | |
| - | + | CosmicPAHmfit is a python fitting tool. It performs a multi-component fit of the selected spectral feature using pseudo-Voigt functions (linear combination of a Gaussian curve and of a Lorentzian curve possibly modified by an asymmetry factor). It has a graphical interface to select the spectral feature of interest as well as the number of components to be included in the fit. For each component, it provides the evolution of the position, width (FWHM) and integrated intensity as a function of temperature. | |
| - | ==== Usage ==== | + | User manual is available through [[https://gitlab.in2p3.fr/ovgso/cosmic-pah/cosmic-pah-mfit/-/wikis/uploads/e15e6afc169937235e6060f1bdc3e518/Manuel_d_utilisation_CosmicPAH-1.pdf|User manuel]] |
| - | + | Full code is available from [[https://gitlab.in2p3.fr/ovgso/cosmic-pah/cosmic-pah-mfit/cosmicPAHmfit/|gitlab]] | |
| - | **Run the following line** | + | ==== Citation ==== |
| - | + | Use the following document to site this application: | |
| - | ``` | + | [[https://gitlab.in2p3.fr/ovgso/cosmic-pah/cosmic-pah-mfit/-/blob/1.1/CITATION.cff|How to cite cosmicPAHmfit]] |
| - | pyenv activate venv; python3 cosmicPAHmfit | + | ==== Installation ==== |
| - | + | It is recommended to use a python virtual environnement. For example by using [[https://github.com/pyenv/pyenv|pyenv]] | |
| - | ``` | + | The python version must be 3.12 or higher. 3.12 to 3.15 are tested and work correctly. |
| - | + | Within the virtual environnement use the following command to install the application: | |
| - | **to exit the pyenv venv you must use:** | + | pip install cosmicPAHmfit |
| - | + | And either one to run the application: | |
| - | ``` | + | python3 -m cosmicPAHmfit |
| - | pyenv deactivate | + | Or |
| - | + | cosmicPAHmfit | |
| - | ``` | + | The installation is detailed in the [[https://gitlab.in2p3.fr/ovgso/cosmic-pah/cosmic-pah-mfit/cosmicPAHmfit/-blob/1.1/README.md|README.md]] |
| - | + | ||
| - | **If (venv) appears in the terminal, the pyenv venv is running. To run the application you can use directly:** | + | |
| - | + | ||
| - | ``` | + | |
| - | python3 cosmicPAHmfit | + | |
| - | + | ||
| - | ``` | + | |
tools/mfit.1788202407.txt.gz · Last modified: 2026/08/31 18:53 by cjoblin
Page Tools
Except where otherwise noted, content on this wiki is licensed under the following license: CC Attribution-Noncommercial-Share Alike 4.0 International
