diff --git a/docs/cli.rst b/docs/cli.rst
index 1e31118..92162cc 100644
--- a/docs/cli.rst
+++ b/docs/cli.rst
@@ -16,6 +16,7 @@ CLI Reference
    cli/pipeline-publish
    cli/pipeline-refresh
    cli/tile-allsky
+   cli/tile-healpix
    cli/tile-study
    cli/tile-wwtl
    cli/transform-fx3-to-rgb
diff --git a/docs/cli/tile-allsky.rst b/docs/cli/tile-allsky.rst
index 7bf4c11..e370778 100644
--- a/docs/cli/tile-allsky.rst
+++ b/docs/cli/tile-allsky.rst
@@ -105,3 +105,9 @@ because ``fork()``-based multiprocessing is required. MacOS should support this,
 but there is currently (as of Python 3.8) `a bug`_ preventing that.
 
 .. _a bug: https://bugs.python.org/issue33725
+
+
+See Also
+========
+
+- :ref:`cli-tile-healpix`
\ No newline at end of file
diff --git a/docs/cli/tile-healpix.rst b/docs/cli/tile-healpix.rst
new file mode 100644
index 0000000..d28965d
--- /dev/null
+++ b/docs/cli/tile-healpix.rst
@@ -0,0 +1,82 @@
+.. _cli-tile-healpix:
+
+=======================
+``toasty tile-healpix``
+=======================
+
+The ``tile-healpix`` command transforms all-sky FITS images in the HEALPix_
+format into WWT’s FITS TOAST format.
+
+.. _HEALPix: https://healpix.jpl.nasa.gov/
+
+Usage
+=====
+
+.. code-block:: shell
+
+   toasty tile-healpix
+      [--galactic]
+      [--outdir DIR]
+      [--parallelism FACTOR] [-j FACTOR]
+      {FITS-PATH}
+      {TOAST-DEPTH}
+
+The ``FITS-PATH`` argument gives the filename of the input image, which should
+be a single FITS file storing data in the HEALPix_ format.
+
+The ``TOAST-DEPTH`` argument specifies the resolution level of the TOAST
+pixelization that will be generated. A depth of 0 means that the input will be
+sampled onto a single 256×256 tile, a depth of 1 means that the input will be
+sampled onto four tiles for a total resolution of 512×512, and so on. When
+converting from HEALPix, the appropriate TOAST depth can be derived from the
+HEALPix ``N_side`` parameter as approximately::
+
+  depth = log2(N_side) - 6.2
+
+One should typically round up to the next larger integer to err on the side of
+higher resolution, although the best policy will depend on the sampling of the
+input HEALPix map.
+
+The ``--outdir DIR`` option specifies where the output data should be written.
+If unspecified, the data root will be the current directory.
+
+The ``--galactic`` option forces the tiling to assume that the input map is in
+Galactic coordinates, even if the FITS headers do not specify that. This has
+been observed in some data sets in the wild.
+
+The ``--parallelism FACTOR`` argument (or ``-j FACTOR``) specifies the level of
+parallism to use. On operating systems that support parallel processing, the
+default is to use all CPUs. To disable parallel processing, explicitly specify a
+factor of 1.
+
+Notes
+=====
+
+This command requires that the healpy_ Python module is installed.
+
+.. _healpy: https://healpy.readthedocs.io/
+
+This command will create FITS files for the highest-resolution tile layer,
+corresponding to the ``DEPTH`` argument, and emit an ``index_rel.wtml`` file
+containing projection information and template metadata.
+
+The WWT rendering engine can also display datasets in the hierarchical HiPS_
+FITS format, which addresses about the same use case as TOAST. If a HiPS FITS
+dataset already exists, it is probably a wiser choice to use it rather than
+creating a new TOAST pyramid. However, TOAST provides noticeably better
+performance for the initial data display and avoiding positional shifts as the
+user zooms in.
+
+.. _HiPS: https://aladin.unistra.fr/hips/
+
+Currently, parallel processing is only supported on the Linux operating system,
+because ``fork()``-based multiprocessing is required. MacOS should support this,
+but there is currently (as of Python 3.8) `a bug`_ preventing that.
+
+.. _a bug: https://bugs.python.org/issue33725
+
+
+See Also
+========
+
+- :ref:`cli-tile-allsky`
\ No newline at end of file
diff --git a/docs/toasting.rst b/docs/toasting.rst
index b516997..30c0713 100644
--- a/docs/toasting.rst
+++ b/docs/toasting.rst
@@ -35,12 +35,12 @@ workflow in this case is as follows:
    which the curved surface of the sphere is mapped onto a 2D image. For
    full-sphere imagery, only a few choices are ever used: probably the main
    thing to check is whether your image is in equatorial (RA/Dec) or galactic
-   (l/b) coordinates. Consult the :ref:`cli-tile-allsky` documentation for the
-   supported choices. If your image uses an unsupported projection, please `file
-   a request`_ with the developers.
+   (l/b) coordinates. Consult the :ref:`cli-tile-allsky` documentation (or
+   :ref:`cli-tile-healpix`) for the supported choices. If your image uses an
+   unsupported projection, please `file a request`_ with the developers.
 
-4. Determine the *tiling depth* appropriate for your use case. The depth is a number
-   that specifies the highest resolution that your final map will attain.
+4. Determine the *tiling depth* appropriate for your use case. The depth is a
+   number that specifies the highest resolution that your final map will attain.
    Consult the :ref:`cli-tile-allsky` documentation for the quantitative
    definition. The best choice will depend on your individual circumstances. But
    as a general guideline, you should probably choose the depth that yields a
@@ -124,7 +124,7 @@ workflow in this case is as follows:
 
 11. Finally, upload the complete contents of your ``tiled`` subdirectory to your
     web server. In this case, the upload location should be such that the url
-    ``http://myserver.org/datasetname/index.wtml``_ will yield the
+    ``http://myserver.org/datasetname/index.wtml`` will yield the
     ``index.wtml`` file created in the previous step.
 
 .. _file a request: https://github.com/WorldWideTelescope/toasty/issues/