Dust Grain Fitter¶
DGFit
is a python package to derive dust grain size and composition
distributions based on fitting observations of interstellar dust.
User Documentation¶
Installation¶
Repository¶
GitHub: DGFit
Quick Start¶
Material needed.
Reporting Issues¶
If you have found a bug in DGFit
please report it by creating a
new issue on the DGFit
GitHub issue tracker.
Please include an example that demonstrates the issue sufficiently so that the developers can reproduce and fix the problem. You may also be asked to provide information about your operating system and a full Python stack trace. The developers will walk you through obtaining a stack trace if it is necessary.
Contributing¶
Like the Astropy project, DGFit
is made both by and for its
users. We accept contributions at all levels, spanning the gamut from fixing a
typo in the documentation to developing a major new feature. We welcome
contributors who will abide by the Python Software Foundation Code of Conduct.
DGFit
follows the same workflow and coding guidelines as
Astropy. The following pages will help you get started with contributing
fixes, code, or documentation (no git or GitHub experience necessary):
For the complete list of contributors please see the DGFit contributors page on Github.
Reference API¶
dgfit.obsdata Module¶
Classes¶
|
ObsData Class |
Class Inheritance Diagram¶
digraph inheritance02045004ea { bgcolor=transparent; rankdir=LR; size="8.0, 12.0"; "ObsData" [URL="api/dgfit.obsdata.ObsData.html#dgfit.obsdata.ObsData",fillcolor=white,fontname="Vera Sans, DejaVu Sans, Liberation Sans, Arial, Helvetica, sans",fontsize=10,height=0.25,shape=box,style="setlinewidth(0.5),filled",target="_top",tooltip="ObsData Class"]; }dgfit.dustgrains Module¶
Classes¶
DustGrains Class |
Class Inheritance Diagram¶
digraph inheritance5f2331fa15 { bgcolor=transparent; rankdir=LR; size="8.0, 12.0"; "DustGrains" [URL="api/dgfit.dustgrains.DustGrains.html#dgfit.dustgrains.DustGrains",fillcolor=white,fontname="Vera Sans, DejaVu Sans, Liberation Sans, Arial, Helvetica, sans",fontsize=10,height=0.25,shape=box,style="setlinewidth(0.5),filled",target="_top",tooltip="DustGrains Class"]; }dgfit.dustmodel Module¶
Classes¶
|
Full dust model including arbitrary size and composition distributions. |
|
Dust model that uses powerlaw size distributions with min/max sizes (MRN). |
|
Dust model that uses the Weingartner & Draine (2001) size distributions. |