From 104d062fd29f629c77d272b923d776d5a8b7f1b1 Mon Sep 17 00:00:00 2001 From: Ben Prather Date: Thu, 9 Jan 2025 13:15:31 -0700 Subject: [PATCH] Update README.md --- iris/README.md | 6 ++---- 1 file changed, 2 insertions(+), 4 deletions(-) diff --git a/iris/README.md b/iris/README.md index 13eddcc8..3364b3bb 100644 --- a/iris/README.md +++ b/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.