fixed spectral extraction equivalencyg

spacetelescope · Nov 1, 2024 · dc6fc9c · dc6fc9c
1 parent 8b363ab
commit dc6fc9c
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Showing 2 changed files with 1 addition and 2 deletions.
diff --git a/jdaviz/configs/cubeviz/plugins/spectral_extraction/spectral_extraction.py b/jdaviz/configs/cubeviz/plugins/spectral_extraction/spectral_extraction.py
@@ -567,7 +567,7 @@ def _preview_y_from_extracted(self, extracted):
         # may need flux<>sb equivalencies, as well as spectral_density
         eqv =_eqv_pixar_sr(self.dataset.selected_obj.meta.get('PIXAR_SR', 1.0)) # for conversions between flux <> sb per sr
         eqv += _eqv_flux_to_sb_pixel()  # for conversions between flux <> sb per pix2
-        eqv += u.spectral_density(self.slice_spectral_value * self.slice_display_unit)
+        eqv += u.spectral_density(self.dataset.selected_obj.spectral_axis)
 
         # call this rather than unit.to because this function handles special cases where
         # the solid angle needs to be multiplied out before conversion

diff --git a/jdaviz/configs/imviz/plugins/coords_info/coords_info.py b/jdaviz/configs/imviz/plugins/coords_info/coords_info.py
@@ -637,7 +637,6 @@ def _copy_axes_to_spectral():
                 # or will be generalized for any sb <-> flux
                 if '_pixel_scale_factor' in sp.meta:
                     disp_flux = flux_conversion(sp.flux.value, sp.flux.unit, viewer.state.y_display_unit, spec=sp)  # noqa: E501
-                    #disp_flux = flux_conversion_general(sp.flux.value, sp.flux.unit, )
                 else:
                     disp_flux = sp.flux.to_value(viewer.state.y_display_unit,
                                                  u.spectral_density(sp.spectral_axis))