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docs: fix plot refs
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steven-murray committed Apr 8, 2024
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Expand Up @@ -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

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