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Small text changes #202

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15 changes: 0 additions & 15 deletions .github/pull_request_template.md

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6 changes: 3 additions & 3 deletions .github/workflows/ci.yml
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Expand Up @@ -21,10 +21,10 @@ jobs:
python-version: '3.10'
toxenv: py310

- name: Python 3.11
- name: Python 3.9
runs-on: ubuntu-latest
python-version: 3.11
toxenv: py311
python-version: 3.9
toxenv: py39

- name: Python 3.12
runs-on: ubuntu-latest
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76 changes: 0 additions & 76 deletions .github/workflows/weekly_cron.yml

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2 changes: 1 addition & 1 deletion README.rst
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@@ -1,7 +1,7 @@
STWCS
-----

.. image:: https://github.com/spacetelescope/stwcs/workflows/CI/badge.svg
.. image:: https://github.com/spacetelescope/stwcs/actions/workflows/weekly_cron.yml/badge.svg
:target: https://github.com/spacetelescope/stwcs/actions
:alt: CI Status

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2 changes: 1 addition & 1 deletion doc/source/fits_convention_tsr/source/sip.rst
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Expand Up @@ -41,7 +41,7 @@ due to velocity aberration observed due to the motion of HST in orbit. The typi
for HST cameras results in a measurable velocity aberration with variations from the center of
the field of view to the edge on the order of 0.1 pixels. More details about this correction can
be found in `Appendix A.3 of the DrizzlePac Handbook
<http://documents.stsci.edu/hst/HST_overview/documents/DrizzlePac/DrizzlePac.cover.html>`_.
<https://hst-docs.stsci.edu/drizzpac>`_.

This scale factor gets computed by
the HST ground systems for start of each exposure and recorded as the VAFACTOR keyword in each
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18 changes: 9 additions & 9 deletions doc/source/hstwcs_ui.rst
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Expand Up @@ -9,9 +9,13 @@ Create an HSTWCS Object
--------------------------
- Create an HSTWCS object using a pyfits HDUList and an extension number

``fobj = pyfits.open('some_file.fits')``
``from astropy.io import fits``

``w = wcsutil.HSTWCS(fobj, 3)``
``from stwcs import wcsutil``

``hdu = fits.open('some_file.fits')``

``w = wcsutil.HSTWCS(hdu, 3)``

- Create an HSTWCS object using a qualified file name.

Expand All @@ -24,10 +28,6 @@ Create an HSTWCS Object
- Create an HSTWCS object from WCS with key 'O'.

``w = wcsutil.HSTWCS('j9irw4b1q_flt.fits', ext=2, wcskey='O')``

- Create a template HSTWCS object for a DEFAULT object.

``w = wcsutil.HSTWCS(instrument='DEFAULT')``

----------------------------------
Coordinate Transformation Examples
Expand All @@ -50,9 +50,9 @@ of the first image pixel is (0,0).

- Apply the entire detector to sky transformation at once:

``outpix = w1.all_pix2world(inpix, 1)``
``outpix = w.all_pix2world(inpix, 1)``

``outpix = w1.all_pix2world(X, Y, 1)``
``outpix = w.all_pix2world(X, Y, 1)``

- The same transformation can be done in separate steps:

Expand All @@ -76,6 +76,6 @@ of the first image pixel is (0,0).
5. Finally the transformation from undistorted to world coordinates is done
by applying the linear WCS.

``wpix = w.wcs_pix2sky(fpix, 1)``
``wpix = w.wcs_pix2world(fpix, 1)``


1 change: 0 additions & 1 deletion stwcs/updatewcs/utils.py
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@@ -1,5 +1,4 @@
import os
import string
from stsci.tools import fileutil

import logging
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2 changes: 1 addition & 1 deletion tox.ini
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@@ -1,5 +1,5 @@
[tox]
envlist= py310, py311, py312, style, dev
envlist= py311, py312, py310, style, dev

[testenv]

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