Fix srctype docs

CHANGES.rst

@@ -1,9 +1,35 @@
 1.10.1 (unreleased)
 ===================
 
-- Remove use of deprecated ``pytest-openfiles`` ``pytest`` plugin. This has been replaced by
+documentation
+-------------
+
+- Corrected information about the application of the ``srctype`` step to WFSS exposures.
+  [#7536]
+
+extract_1d
+----------
+
+- Update to be skipped for NIRSpec fixed slit modes with rateints input as that
+  mode is not allowed. [#7516]
+
+flat_field
+----------
+
+- Updated to allow processing of NIRSpec fixed-slit 3D (rateints) files. [#7516]
+
+other
+-----
+
+- Remove use of deprecated ``pytest-openfiles`` plugin. This has been replaced by
   catching ``ResourceWarning``s. [#7526]
 
+resample_spec
+-------------
+
+- Update ``resample_spec`` to be skipped for NIRSpec fixed slit MultiSlitModel
+  rateints input as that mode is not allowed. [#7516]
+
 
 1.10.0 (2023-04-03)
 ===================
@@ -32,7 +58,7 @@ calwebb_detector1
 cube_build
 ----------
 
--  Windows: MSVC: Allocate ``wave_slice_dq`` array using ``mem_alloc_dq()`` [#7491]
+- Windows: MSVC: Allocate ``wave_slice_dq`` array using ``mem_alloc_dq()`` [#7491]
 
 - Memory improvements, do not allow MIRI and 'internal_cal', allow user to set suffix. [#7521]
 
@@ -66,9 +92,6 @@ extract_1d
 
 - Edit surface brightness unit strings for parsing by ``astropy.units`` [#7511]
 
-- Update to be skipped for NIRSpec fixed slit modes with rateints input as that
-  mode is not allowed. [#7516]
-
 jump
 ----
 
@@ -150,9 +173,6 @@ resample
 
 - Carry through good bits correctly for the variance array [#7515]
 
-- Update ``resample_spec`` to be skipped for NIRSpec fixed slit MultiSlitModel
-  rateints input as that mode is not allowed. [#7516]  
-
 residual_fringe
 ---------------
 

docs/jwst/pipeline/calwebb_spec2.rst

@@ -55,7 +55,7 @@ TSO exposures. The instrument mode abbreviations used in the table are as follow
 +----------------------------------------------------------+-----+-----+-----+-----+-----+-----+------+------+--------+-----+
 | :ref:`extract_2d <extract_2d_step>`\ :sup:`1`            | |c| | |c| |     |     |     |     |      | |c|  |  |c|   | |c| |
 +----------------------------------------------------------+-----+-----+-----+-----+-----+-----+------+------+--------+-----+
-| :ref:`srctype <srctype_step>`\ :sup:`1`                  | |c| | |c| | |c| | |c| | |c| | |c| |  |c| |      |        | |c| |
+| :ref:`srctype <srctype_step>`\ :sup:`1`                  | |c| | |c| | |c| | |c| | |c| | |c| |  |c| | |c|  |  |c|   | |c| |
 +----------------------------------------------------------+-----+-----+-----+-----+-----+-----+------+------+--------+-----+
 | :ref:`master_background <master_background_step>`        |     | |c| |     |     |     |     |      |      |        |     |
 +----------------------------------------------------------+-----+-----+-----+-----+-----+-----+------+------+--------+-----+
@@ -87,7 +87,7 @@ TSO exposures. The instrument mode abbreviations used in the table are as follow
 :sup:`1`\ The exact order of the :ref:`extract_2d <extract_2d_step>`, :ref:`srctype <srctype_step>`,
 and :ref:`flat_field <flatfield_step>` steps depends on the observing mode.
 For NIRISS and NIRCam WFSS, as well as NIRCam TSO grism exposures, the order is
-flat_field followed by extract_2d (no wavecorr or srctype).
+flat_field, extract_2d, and srctype (no wavecorr).
 For all other modes the order is extract_2d, srctype, wavecorr, and flat_field.
 
 :sup:`2`\ By default the :ref:`residual_fringe <residual_fringe_step>` is skipped in the ``calwebb_spec2`` pipeline. 

docs/jwst/srctype/description.rst

@@ -135,6 +135,6 @@ NIRCam and NIRISS WFSS
 ++++++++++++++++++++++
 It is not possible to specify ahead of time the source types for spectra that
 may show up in a Wide-Field Slitless Spectroscopy exposure. So for these modes
-the ``srctype`` step simply sets the SRCTYPE keyword value to "UNKNOWN" and the
-actual source sizes are derived from the catalog information generated
-from direct images that are obtained as part of a WFSS observation.
+the ``srctype`` step uses the value from the ``is_extended`` column of the
+source catalog generated from the direct imaging taken with WFSS observations
+and uses that to set "POINT" or "EXTENDED" for each extracted source.