Update README.md

README.md

@@ -13,18 +13,20 @@ The H-band (1.45−1.85 μm) data were reduced using the standard ESO-SINFONI pi
 
 The galaxy has a highly perturbed morphology, with a prominent arc towards north of the core, which is cospatial with the jet axis (green contours from radio overlay). This suggests its a site of jet-ISM interaction from the expanding radio lobes. 
 
-A quick look at the line profiles over the field of view showed that the broad line emission is limited to the nuclear region-- which were found to be due to kpc-scale outflowing (ionized) gas. The northern arc-like feature only shows narrow line emission and is likely a site of active star formation.  
+A quick look at the line profiles over the field of view showed that the _broad line emission is limited to the nuclear region_-- which were found to be due to kpc-scale outflowing (ionized) gas. The northern arc-like feature only shows narrow line emission and is likely a site of active star formation.  
 
-Thus, _all the analyses are divided spatially into the "NUCLEAR" and "NORTHERN ARC" regions._
+Thus, some of the analyses are divided spatially into the "nuclear" and "northern arc" regions.
 
 ### Codes
 
-- `spaxelwise_Nuclear7x7_NorthernArc.ipynb` |  Script to calculate ...
 - `pipelined_FOV_fitting_&_maps.ipynb` and `pipelined_FOV_fitting_&_maps.py` |  spectrum modelling
 - `3c297_broad&narrow_line_maps.ipynb` |
+- `spaxelwise_Nuclear7x7_NorthernArc.ipynb` |  Script to calculate ...
 - `3c297_overlays.ipynb` |
 - `WHAN_diagnostic_spaxelwise.ipynb` |
 - `telluricOH_fitting.ipynb` |
+- `generate_error_cube.ipynb` |
+
 
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