Fix code style and residual references to SpectralCube

spacetelescope · Sep 14, 2021 · 1cc55d1 · 1cc55d1
1 parent 6aabc15
commit 1cc55d1
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Showing 3 changed files with 2 additions and 3 deletions.
diff --git a/docs/mosviz/plugins.rst b/docs/mosviz/plugins.rst
@@ -69,4 +69,4 @@ The :guilabel:`Remove` button can be used to remove a slit once it has been appl
 In order to plot a slit onto the image viewer, we need WCS information from an image and slit position from a 2D spectrum.
 WCS information is taken from the `meta` attribute of the :class:`~astropy.nddata.CCDData` object representing the data in the
 image viewer. The slit position is calculated using the `S_REGION` header extension value, located in the `meta` attribute of
-the :class:`~spectral_cube.SpectralCube` object that is active in the 2D spectrum viewer.
+the :class:`~specutils.Spectrum1D` object that is active in the 2D spectrum viewer.
diff --git a/jdaviz/configs/mosviz/plugins/parsers.py b/jdaviz/configs/mosviz/plugins/parsers.py
@@ -546,7 +546,7 @@ def mos_niriss_parser(app, data_dir, obs_label=""):
                             sci_hdus.append(i)
                             wav_hdus[i] = ('WAVELENGTH', temp[i].header['EXTVER'])
 
-                # Now get a SpectralCube object for each SCI HDU
+                # Now get a Spectrum1D object for each SCI HDU
                 for sci in sci_hdus:
 
                     if temp[sci].header["SPORDER"] == 1:

diff --git a/jdaviz/configs/mosviz/tests/test_helper.py b/jdaviz/configs/mosviz/tests/test_helper.py
@@ -5,7 +5,6 @@
 from astropy.nddata import CCDData
 from astropy.wcs import WCS
 from jdaviz.configs.mosviz.helper import Mosviz
-from spectral_cube import SpectralCube
 from specutils import Spectrum1D, SpectrumCollection