-
Notifications
You must be signed in to change notification settings - Fork 4
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
Showing
4 changed files
with
34 additions
and
2 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -1,9 +1,14 @@ | ||
# regularizepsf | ||
[![codecov](https://codecov.io/gh/punch-mission/regularizepsf/branch/main/graph/badge.svg?token=pn4NTO70I9)](https://codecov.io/gh/punch-mission/regularizepsf) | ||
[![DOI](https://zenodo.org/badge/555583385.svg)](https://zenodo.org/badge/latestdoi/555583385) | ||
[![PyPI version](https://badge.fury.io/py/regularizepsf.svg)](https://badge.fury.io/py/regularizepsf) | ||
|
||
A package for manipulating and correcting various point spread functions. | ||
A package for manipulating and correcting variable point spread functions. | ||
|
||
Below is an example of correcting model data using the package. An initial image of a simplified starfield (a) is synthetically observed with a slowly | ||
varying PSF (b), then regularized with this technique (c). The final image visually matches a direct convolution of | ||
the initial image with the target PSF (d). The panels are gamma-corrected to highlight the periphery of the model PSFs. | ||
![Example result image](model_example.png) | ||
|
||
## Getting started | ||
|
||
|
@@ -17,3 +22,27 @@ See LICENSE for the MIT license | |
|
||
## Need help? | ||
Please contact Marcus Hughes at [[email protected]](mailto:[email protected]). | ||
|
||
## Citation | ||
Please cite the associated paper if you use this technique: | ||
|
||
``` | ||
@misc{https://doi.org/10.48550/arxiv.2212.02594, | ||
doi = {10.48550/ARXIV.2212.02594}, | ||
url = {https://arxiv.org/abs/2212.02594}, | ||
author = {Hughes, J. M. and DeForest, C. E. and Seaton, D. B.}, | ||
keywords = {Instrumentation and Methods for Astrophysics (astro-ph.IM), FOS: Physical sciences, FOS: Physical sciences}, | ||
title = {Coma Off It: Removing Variable Point Spread Functions from Astronomical Images}, | ||
publisher = {arXiv}, | ||
year = {2022}, | ||
copyright = {arXiv.org perpetual, non-exclusive license} | ||
} | ||
``` |
Binary file not shown.
Loading
Sorry, something went wrong. Reload?
Sorry, we cannot display this file.
Sorry, this file is invalid so it cannot be displayed.