@@ -721,6 +721,7 @@ def photom_io(self, tabdata, order=None):
721721 "to surface brightness" )
722722 conversion /= slit .meta .photometry .pixelarea_steradians
723723 else :
724+ conversion_uniform = conversion / slit .meta .photometry .pixelarea_steradians
724725 unit_is_surface_brightness = False
725726 elif isinstance (self .input , datamodels .MultiSpecModel ):
726727 # MultiSpecModel output from extract1d should not require this area conversion?
@@ -735,6 +736,7 @@ def photom_io(self, tabdata, order=None):
735736 "to surface brightness" )
736737 conversion /= self .input .meta .photometry .pixelarea_steradians
737738 else :
739+ conversion_uniform = conversion / self .input .meta .photometry .pixelarea_steradians
738740 unit_is_surface_brightness = False
739741
740742 # Store the conversion factor in the meta data
@@ -795,35 +797,35 @@ def photom_io(self, tabdata, order=None):
795797
796798 # Compute a 2-D grid of conversion factors, as a function of wavelength
797799 if isinstance (self .input , datamodels .MultiSlitModel ):
798-
800+ slit = self . input . slits [ self . slitnum ]
799801 # The NIRSpec fixed-slit primary slit needs special handling if
800802 # it contains a point source
801803 if self .exptype .upper () == 'NRS_FIXEDSLIT' and \
802- self . input . slits [ self . slitnum ] .name == self .input .meta .instrument .fixed_slit and \
803- self . input . slits [ self . slitnum ] .source_type .upper () == 'POINT' :
804+ slit .name == self .input .meta .instrument .fixed_slit and \
805+ slit .source_type .upper () == 'POINT' :
804806
805807 # First, compute 2D array of photom correction values using
806808 # uncorrected wavelengths, which is appropriate for a uniform source
807- scalar_conv = conversion
808- conversion , no_cal = self .create_2d_conversion (self .input .slits [self .slitnum ],
809- self .exptype , scalar_conv ,
809+ conversion_2d_uniform , no_cal = self .create_2d_conversion (slit ,
810+ self .exptype , conversion_uniform ,
810811 waves , relresps , order ,
811812 use_wavecorr = False )
812- slit .photom_uniform = conversion # store the result
813+ slit .photom_uniform = conversion_2d_uniform # store the result
813814
814815 # Now repeat the process using corrected wavelength values,
815816 # which is appropriate for a point source. This is the version of
816817 # the correction that will actually get applied to the data below.
817- conversion , no_cal = self .create_2d_conversion (self . input . slits [ self . slitnum ] ,
818- self .exptype , scalar_conv ,
818+ conversion , no_cal = self .create_2d_conversion (slit ,
819+ self .exptype , conversion ,
819820 waves , relresps , order ,
820821 use_wavecorr = True )
821822 slit .photom_point = conversion # store the result
822823
823824 else :
824- conversion , no_cal = self .create_2d_conversion (self . input . slits [ self . slitnum ] ,
825+ conversion , no_cal = self .create_2d_conversion (slit ,
825826 self .exptype , conversion ,
826827 waves , relresps , order )
828+
827829 elif isinstance (self .input , datamodels .MultiSpecModel ):
828830
829831 # This input does not require a 2d conversion, but a 1d interpolation on the
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