Updated change log

DOI-USGS · Oct 1, 2020 · 6c2036f · 6c2036f
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commit 6c2036f
Showing 1 changed file with 2 additions and 1 deletion.
diff --git a/CHANGELOG.md b/CHANGELOG.md
@@ -35,14 +35,15 @@ update the Unreleased link so that it compares against the latest release tag.
  - Camera models now use the ALE library to interpolate states and orientations. Users will likely see very small changes in sensor ephemerides. These were tested and are within existing interpolation tolerances. [#2370](https://github.com/USGS-Astrogeology/ISIS3/issues/2370)
  - The isis3VarInit script is now just called isisVarInit and allows for more robust paths. [#3945](https://github.com/USGS-Astrogeology/ISIS3/pull/3945)
  - Isis2raw will now output straight to a 32bit file (no stretch) when stretch is set to None and bittype is set to 32bit. [#3878](https://github.com/USGS-Astrogeology/ISIS3/issues/3878)
+ - Findimageoverlaps can now have calculations and writes happen at the same time or sequentially. [#4047](https://github.com/USGS-Astrogeology/ISIS3/pull/4047)
 
 ### Fixed
 
  - Fixed some line scan images using the incorrect state interpolation. [#3928](https://github.com/USGS-Astrogeology/ISIS3/issues/3928)
  - The ISIS library now has the correct version suffix. [#3365](https://github.com/USGS-Astrogeology/ISIS3/issues/3365)
  - Equalizer now reports the correct equation and values used to perform the adjustment. [#3987](https://github.com/USGS-Astrogeology/ISIS3/issues/3987)
  - Map2cam now works correctly when specifying bands for input cubes. [#3856](https://github.com/USGS-Astrogeology/ISIS3/issues/3856)
- 
+
  - mro/hideal2pds app now writes the correct SAMPLE_BIT_MASK values to the output label. [#3978](https://github.com/USGS-Astrogeology/ISIS3/issues/3978)
 
   - For Histograms in ISIS, updated the math for calculating what bin data should be placed in and the min/max values of each bin to be more intuitive. In addition, the output of hist and cnethist were changed to display the min/max values of each bin instead of the middle pixel's DN. [#3882](https://github.com/USGS-Astrogeology/ISIS3/issues/3882)