diff --git a/docs/examples/plotting.ipynb b/docs/examples/plotting.ipynb index 84578c3d..cefa08ca 100644 --- a/docs/examples/plotting.ipynb +++ b/docs/examples/plotting.ipynb @@ -66,7 +66,7 @@ "metadata": {}, "source": [ "
\n", - "Note: this example uses the data provided by the xarray.tutorial functions. As such, the units attributes follow the CF conventions, which pint does not understand by default. To still be able to read them we are using the registry provided by cf-xarray.\n", + "Note: this example uses the data provided by the xarray.tutorial functions. As such, the units attributes follow the CF conventions, which astropy does not understand by default. To still be able to read them, registry be aliases can be used. For more information, see cf-xarray.\n", "
" ] }, @@ -110,7 +110,7 @@ "id": "9", "metadata": {}, "source": [ - "Most operations will preserve the units but there are some which will drop them (see the [duck array integration status](https://xarray.pydata.org/en/stable/user-guide/duckarrays.html#missing-features) page). To work around that there are unit-aware versions on the `.pint` accessor. For example, to select data use `.astropy.sel` instead of `.sel`:" + "Most operations will preserve the units but there are some which will drop them (see the [duck array integration status](https://xarray.pydata.org/en/stable/user-guide/duckarrays.html#missing-features) page). To work around that there are unit-aware versions on the `.astropy` accessor. For example, to select data use `.astropy.sel` instead of `.sel`:" ] }, { @@ -145,14 +145,6 @@ "source": [ "monthly_means.astropy.dequantify(format=\"unicode\").plot.imshow(col=\"month\", col_wrap=4)" ] - }, - { - "cell_type": "code", - "execution_count": null, - "id": "13", - "metadata": {}, - "outputs": [], - "source": [] } ], "metadata": {