A dust library for calculating scattering and extinction properties, from the infrared to X-ray
This is a python library for calculating scattering absorption and scattering efficiencies for astrophysical dust from the infrared to the X-ray. This code can also be used to calculate dust scattering halo images in the X-ray, in both interstellar and intergalactic (cosmological) contexts.
Click here for eblur/dust documentation at ReadTheDocs
The first published version of this code was released with Corrales & Paerels (2015). If you use eblur/dust, please cite this publication.
The DOI for the most recent stable release is http://dx.doi.org/10.5281/zenodo.15991
Lia Corrales (@eblur) - lead developer
@mboquien
@JohannesBuchner
If you need support, please email the lead developer:
lia [at] space [dot] mit [dot] edu