-

Xdust documentation¶

+

Xdust documentation¶

The xdust library calculates scattering and absorption efficiencies for dust from the infrared to the X-ray. It has special capabilities to calculate dust scattering halo images in the X-ray.

First published version of this code (released with Corrales & Paerels, 2015) http://dx.doi.org/10.5281/zenodo.15991

Source code: github.com/eblur/xdust

-

Support: If you are having issues, please contact liac@umich.edu

+

Support: If you have questions, please contact liac@umich.edu

Features¶

A number of dust grain size distributions and optical constants are @@ -323,34 +326,11 @@

Tutorials¶

    -
  • xdust.grainpop -
    • -
  • xdust.graindist -
    • -
  • xdust.scatteringmodel -
    • -
  • xdust.halos @@ -403,7 +383,7 @@

    Modules¶
      -
    • Xdust documentation
        +
      • Xdust documentation
        • Features
        • Grain Populations
        • X-ray Scattering Halos
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\ No newline at end of file diff --git a/docs/index.rst b/docs/index.rst index c440b8b..459e186 100644 --- a/docs/index.rst +++ b/docs/index.rst @@ -5,7 +5,7 @@ .. _index: -*Xdust* documentation +Xdust documentation ===================== The *xdust* library calculates scattering and absorption efficiencies @@ -17,7 +17,7 @@ http://dx.doi.org/10.5281/zenodo.15991 **Source code:** `github.com/eblur/xdust `_ -**Support:** If you are having issues, please contact liac@umich.edu +**Support:** If you have questions, please contact liac@umich.edu Features -------- @@ -85,10 +85,7 @@ Modules .. toctree:: :maxdepth: 2 - grainpop - graindist - scatmodels - halos + modules/index .. Indices and tables diff --git a/docs/composition.rst b/docs/modules/composition.rst similarity index 90% rename from docs/composition.rst rename to docs/modules/composition.rst index e0c6792..4c883d9 100644 --- a/docs/composition.rst +++ b/docs/modules/composition.rst @@ -1,7 +1,7 @@ .. _composition: -xdust.graindist.composition -=========================== +graindist.composition +===================== The composition library is built on the superclass :ref:`CompositionClass`, which holds the optical constants and material density [g cm^-3] of a grain composition type. @@ -15,7 +15,7 @@ The composition library is built on the superclass :ref:`CompositionClass`, whic .. _CompositionClass: Composition ---------------------------- +----------- .. autoclass:: xdust.graindist.composition.Composition diff --git a/docs/graindist.rst b/docs/modules/graindist.rst similarity index 89% rename from docs/graindist.rst rename to docs/modules/graindist.rst index 65899ba..05a74b4 100644 --- a/docs/graindist.rst +++ b/docs/modules/graindist.rst @@ -1,7 +1,7 @@ .. _graindist: -xdust.graindist -=============== +graindist +========= This module contains: @@ -14,7 +14,7 @@ This is tied together by the :ref:`GrainDistClass` superclass. .. _GrainDistClass: GrainDist ---------------------------- +---------- .. autoclass:: xdust.graindist.GrainDist diff --git a/docs/grainpop.rst b/docs/modules/grainpop.rst similarity index 97% rename from docs/grainpop.rst rename to docs/modules/grainpop.rst index 3a7ad97..0af0b0c 100644 --- a/docs/grainpop.rst +++ b/docs/modules/grainpop.rst @@ -1,7 +1,7 @@ .. _grainpop: -xdust.grainpop -============== +grainpop +======== The :ref:`SingleGrainPop` object is used to model a population of dust grains based on three distinct properties: diff --git a/docs/halos.rst b/docs/modules/halos.rst similarity index 98% rename from docs/halos.rst rename to docs/modules/halos.rst index 92ceae6..355c2d3 100644 --- a/docs/halos.rst +++ b/docs/modules/halos.rst @@ -1,7 +1,7 @@ .. _halos: -xdust.halos -=========== +halos +===== The superclass :ref:`Halo` holds all information and special functions for working with a simulated X-ray dust scattering halo. diff --git a/docs/modules/index.rst b/docs/modules/index.rst new file mode 100644 index 0000000..1fba7df --- /dev/null +++ b/docs/modules/index.rst @@ -0,0 +1,25 @@ +.. xdust documentation master file, created by + sphinx-quickstart on Sunday May 30 2026 + You can adapt this file completely to your liking, but it should at least + contain the root `toctree` directive. + +.. _modules: + +Modules +------- + +.. toctree:: + :maxdepth: 2 + + grainpop + graindist + scatmodels + halos + + +.. Indices and tables + ================== + + * :ref:`genindex` + * :ref:`modindex` + * :ref:`search` diff --git a/docs/scatmodels.rst b/docs/modules/scatmodels.rst similarity index 94% rename from docs/scatmodels.rst rename to docs/modules/scatmodels.rst index cd313aa..2a63b8c 100644 --- a/docs/scatmodels.rst +++ b/docs/modules/scatmodels.rst @@ -1,7 +1,7 @@ .. _scatmodels: -xdust.scatteringmodel -===================== +scatteringmodel +=============== The scattering model library is built on the superclass :ref:`ScatteringModelClass`, which defines the scattering physics model and holds the computational results once the scattering model is calculated. diff --git a/docs/shape.rst b/docs/modules/shape.rst similarity index 92% rename from docs/shape.rst rename to docs/modules/shape.rst index 7a0e6a9..3e4d80d 100644 --- a/docs/shape.rst +++ b/docs/modules/shape.rst @@ -1,7 +1,7 @@ .. _shape: -xdust.graindist.shape -===================== +graindist.shape +=============== The superclass :ref:`ShapeClass` describes the geometric properties of the dust grains. diff --git a/docs/sizedist.rst b/docs/modules/sizedist.rst similarity index 95% rename from docs/sizedist.rst rename to docs/modules/sizedist.rst index 8a398fc..dfc315d 100644 --- a/docs/sizedist.rst +++ b/docs/modules/sizedist.rst @@ -1,7 +1,7 @@ .. _sizedist: -xdust.graindist.sizedist -============================ +graindist.sizedist +================== The size distribution library is built on the superclass :ref:`SizedistClass`, which holds the grain size distribution function and the grain size array.