Python Component Fitting Tool (pycfit)
Python program to replicate many spectral fitting functions of the CFIT system from SolarSoft IDL.
Installation
pip install pycfit
🛠 Important: MacOS 26 (Tahoe)
If running under MacOS Tahoe - pycfit must be run from within an ipython session using the gui qt magic command for the GUI components to work properly.
E.G.
Start ipython with the qt gui magic in place:
$> ipython --gui=qt
or, from within an ipython session:
In [1]: %gui qt
Use
Use interactive fitter to find an initial model based on an averaged spectra
import pycfit
# Retrieve sample data
wavelength, intensity, uncertainty = pycfit.data.get_example_single_spectrum()
# Call the GUI fitter
model = pycfit.cfit_gui(wavelength, intensity, uncertainty=uncertainty)
If you export your model from within the GUI, you can initialize a new pyCFIT instance with it later
from pathlib import Path
fname = Path('path/to/saved/model.py')
model = pycfit.cfit_gui(wavelength, intensity, uncertainty=uncertainty, function=fname)
Use the interactive viewer to fit each point of the raster to the initial model and adjust or mask individual point fittings as needed
# Retrieve a small-patch of sample data
wavelength, intensity, uncertainty, mask = pycfit.data.get_example_grid_spectra()
# Create a Grid fitter, using the previously defined model
myGrid = pycfit.cfit_grid(model, wavelength, intensity,
uncertainty=uncertainty, mask=mask)
# Fit the whole raster
myGrid.fit(maxiter=100) # Astropy fitter keywords like "maxiter" can be passed through
# Inspect and modify the fits at each point
print(myGrid.shape)
myGrid = pycfit.cfit_grid_gui(myGrid)
# Get results
results = myGrid.get_results()
Contacts:
Software Maintenance:
Ayris Narock: ayris.a.narock@nasa.gov
NASA Official:
Therese Kucera: therese.a.kucera@nasa.gov
License
This project is Copyright (c) National Aeronautics and Space Administration and licensed under
the terms of the Apache Software License 2.0 license. This package is based upon
the Openastronomy packaging guide <https://github.com/OpenAstronomy/packaging-guide>_
which is licensed under the BSD 3-clause licence. See the licenses folder for
more information.
Metadata
Release files for pycfit 1.1.0
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
|---|---|---|---|
| pycfit-1.1.0.tar.gz | 1.9 MB | Details |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Reset |
|---|---|---|---|---|
| pycfit-1.1.0-py3-none-any.whl | Python 3 | none | any | Details |
Total release size: 3.9 MB
Release files / pycfit-1.1.0.tar.gz
| Download URL | pycfit-1.1.0.tar.gz |
|---|---|
| Size | 1.9 MB |
| Tags | Source |
|
SHA-256 checksum How to use checksums |
3a0eaa1bc99f18b365ddc44ba0d2e338605175ef2d7b46d336e9a957c976f6f9
|
|
BLAKE2b-256 checksum How to use checksums |
ab16778d49a09b0de54478fa801131c59ab159357bccbb6f92f8917e2b11a8b1
|
| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/7.0.0 CPython/3.12.10
|
Release files / pycfit-1.1.0-py3-none-any.whl
| Download URL | pycfit-1.1.0-py3-none-any.whl |
|---|---|
| Size | 2.0 MB |
| Tags | Python 3 |
|
SHA-256 checksum How to use checksums |
dbb99130f12440c9ff9c493ca069a35ce1dad21e14fec180fb8c496255d6c393
|
|
BLAKE2b-256 checksum How to use checksums |
eb6725ff1a0738b21ee0c4c36459e9d465a6090b6bb93d57c363924ef39b6ab2
|
| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/7.0.0 CPython/3.12.10
|