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diff --git a/physics/LIGO.page b/physics/LIGO.page
index 2e86d5f..b7ba600 100644
--- a/physics/LIGO.page
+++ b/physics/LIGO.page
@@ -1,18 +1,12 @@
---
-format: rst
-categories: physics
toc: no
+title: LIGO: Laser Interferometer Gravitational Observatory
...
-=======================================================================
-LIGO: Laser Interferometer Gravitational Observatory
-=======================================================================
-
.. warning:: This is a rough work in progress!! Likely to be factual errors, poor grammar, etc.
-.. note:: Most of this content is based on a 2002 Caltech course taught by
- Kip Thorn [PH237]_
+.. note: Most of this content is based on a 2002 Caltech course taught by Kip Thorn [PH237]
Noise Sources
~~~~~~~~~~~~~~~~~~~~~~
@@ -53,3 +47,8 @@ This technique requires known, theoretically derived waveforms (within
phase/amplitude). There are other methods when we don't have good guesses
about the waveform we are looking for...
+References
+----------------
+
+[PH237]: **Gravitational Waves** (aka ph237), a course taught by Kip Thorne at Caltech in 2002. See http://elmer.tapir.caltech.edu/ph237/ for notes and lecture videos.
+