PSF Homogenization kERnels - pypher
¶
Compute an homogenization kernel between two PSFs
This code is well suited for PSF matching applications in both an astronomical or microscopy context.
It has been developed as part of the ESA Euclid mission and is currently being used for multi-band photometric studies of HST (visible) and Herschel (IR) data.
Features¶
- Warp (rotation + resampling) the PSF images (if necessary),
- Filter images in Fourier space using a regularized Wiener filter,
- Produce a homogenization kernel.
Note: pypher
needs the pixel scale information to be present in the FITS files. If not, use the provided addpixscl
method to add this missing info.
Warning
This code does not
- interpolate NaN values (replaced by 0 instead),
- center PSF images,
- minimize the kernel size.
Quick setup¶
In most cases the code can be installed via
$ pip install pypher
and a kernel can then be produced from two PSFs with a simple command line
$ pypher psf_a.fits psf_b.fits kernel_a_to_b.fits
Other installation procedures are described on the installation page and further command line options here.
User Guide¶
Acknowledging¶
If you make use of any product of this code in a scientific publication, please consider acknowledging the work by citing the following paper
Boucaud *et al.* (2016) “Convolution kernels for multi-wavelength imaging”
Author: | Alexandre Boucaud |
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Email: | alexandre.boucaud [at] ias.u-psud.fr |
Licence: | This work is licensed under a 3-clause BSD license |