From 086dfaec82141d92ff24e5413ec1392bc1849ebc Mon Sep 17 00:00:00 2001 From: Steven Murray Date: Mon, 8 Apr 2024 15:11:28 +0200 Subject: [PATCH] docs: fix plot refs --- joss-paper/paper.md | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/joss-paper/paper.md b/joss-paper/paper.md index 7b4eb43..05d6cfa 100644 --- a/joss-paper/paper.md +++ b/joss-paper/paper.md @@ -102,9 +102,9 @@ This figure also demonstrates that the new 21cmSense is capable of producing sensitivity predictions in the cylindrically-averaged 2D power spectrum space, which is helpful for upcoming experiments. -![Sampling of the $(u,v)$-plane for the HERA experiment during a full year of observations.\label{uvsampling}](uv-sampling.png) +![Sampling of the $(u,v)$-plane for the HERA experiment during a full year of observations.\label{uvsampling}](joss-paper/uv-sampling.png) -![Predicted sensitivity of 1000 hours (one year) of HERA observations, as a function of perpendicular and line-of-sight fourier scale. The sensitivity is represented as the signal-to-noise on each $k$-mode, assuming a particular astrophysical model.\label{sense}](2dps.png) +![Predicted sensitivity of 1000 hours (one year) of HERA observations, as a function of perpendicular and line-of-sight fourier scale. The sensitivity is represented as the signal-to-noise on each $k$-mode, assuming a particular astrophysical model.\label{sense}](joss-paper/2dps.png) # Statement of need