docs: fix joss plots

rasg-affiliates · Apr 8, 2024 · 1911d1e · 1911d1e
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diff --git a/joss-paper/paper.bib b/joss-paper/paper.bib
@@ -337,3 +337,46 @@ @ARTICLE{jwst
        adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...938L..15C},
       adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
+
+@ARTICLE{Munoz2022,
+       author = {{Mu{\~n}oz}, Julian B. and {Qin}, Yuxiang and {Mesinger}, Andrei and {Murray}, Steven G. and {Greig}, Bradley and {Mason}, Charlotte},
+        title = "{The impact of the first galaxies on cosmic dawn and reionization}",
+      journal = {\mnras},
+     keywords = {galaxies: high-redshift, intergalactic medium, cosmology: theory, dark ages, reionization, first stars, diffuse radiation, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
+         year = 2022,
+        month = apr,
+       volume = {511},
+       number = {3},
+        pages = {3657-3681},
+          doi = {10.1093/mnras/stac185},
+archivePrefix = {arXiv},
+       eprint = {2110.13919},
+ primaryClass = {astro-ph.CO},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.3657M},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
+@article{Murray2020,
+  doi = {10.21105/joss.02582},
+  url = {https://doi.org/10.21105/joss.02582},
+  year = {2020},
+  publisher = {The Open Journal},
+  volume = {5},
+  number = {54},
+  pages = {2582},
+  author = {Steven G. Murray and Bradley Greig and Andrei Mesinger and Julian B. Muñoz and Yuxiang Qin and Jaehong Park and Catherine A. Watkinson},
+  title = {21cmFAST v3: A Python-integrated C code for generating 3D realizations of the cosmic 21cm signal.},
+  journal = {Journal of Open Source Software}
+}
+
+@software{Mesinger2011,
+       author = {{Mesinger}, Andrei and {Furlanetto}, Steven and {Cen}, Renyue},
+        title = "{21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal}",
+ howpublished = {Astrophysics Source Code Library, record ascl:1102.023},
+         year = 2011,
+        month = feb,
+          eid = {ascl:1102.023},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2011ascl.soft02023M},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
diff --git a/joss-paper/paper.md b/joss-paper/paper.md
@@ -97,13 +97,13 @@ An example of the predicted sensitivity of the HERA experiment after a year's ob
 at $z=8.5$ is shown in Figure \ref{sense}, corresponding to the sampling of the $(u,v)$-grid
 shown in Figure \ref{uvsampling}. The sensivity here is a signal-to-noise,
 assuming a signal magnitude computed using a semi-numerical model from the 21cmFAST
-code [@21cmfast], using parameters from [@Munoz22].
+code [@Mesinger2011; @Murray2020], using parameters from [@Munoz22].
 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)
-![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)
+![Sampling of the $(u,v)$-plane for the HERA experiment during a full year of observations.](uv-sampling.png){label="uvsampling"}
+![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.](2dps.png){label="sense"}
 
 # Statement of need