Update README.md

iris/README.md

@@ -2,8 +2,6 @@
 
 Iris is a ray-tracer built alongside KHARMA, using Kokkos and Parthenon.  Currently it is only useful for imaging KHARMA files: it can produce unpolarized and polarized images at radio frequencies comparable to e.g. Event Horizon Telescope observations, and performs within expected variance compared to other polarized ray-tracers in the polarized comparison problems (i.e. the thin disk and sample dump).
 
-However, it is written to be adapted to many other cases, e.g. automatic flux fitting, multiple cameras and frequency bundling, and eventually Monte Carlo spectra.
+However, it is written to be adapted to many other cases, e.g. automatic flux fitting, multiple cameras and frequency bundling, and eventually Monte Carlo spectra and inline imaging as simulations are run.
 
-Iris owes its existence to/uses a lot of code from/shamelessly rips off [ipole](https://github.com/AFD-Illinois/ipole).  A few 
-
-Code from `ipole` is used under the BSD 3-clause license, and Iris is provided with KHARMA under the same license.  I also copied the ipole log/text output format, so anything relying on that for parsing should work fine.
+Iris owes its existence to/uses a lot of code from/shamelessly rips off [ipole](https://github.com/AFD-Illinois/ipole).  Code from `ipole` is used under the BSD 3-clause license, and Iris is provided with KHARMA under the same license.  I also copied the ipole log/text output format, so anything relying on that for parsing should continue to work with iris.