Merge branch 'master' of https://git.overleaf.com/5b9ba87bb3c7df5cc4b…

…b86b8
lsstdarkmatter · Jan 14, 2019 · a9f33d6 · a9f33d6
2 parents b69b128 + 86a1c82
commit a9f33d6
Show file tree

Hide file tree

Showing 2 changed files with 1 addition and 1 deletion.
diff --git a/figures/dmbaryon_pk2.png b/figures/dmbaryon_pk2.png
diff --git a/models/particles.tex b/models/particles.tex
@@ -152,7 +152,7 @@ \subsection{Baryon-Scattering Dark Matter (BSDM) \Contact{Vera}}
 
 \begin{figure}
 \centering
-\includegraphics[width=0.6\columnwidth]{figures/dmbaryon_pk.png}
+\includegraphics[width=0.6\columnwidth]{figures/dmbaryon_pk2.png}.png}
 \caption{Linear matter power spectrum at $z=0$. We show the residuals between the CDM case and the case where there is velocity-independent spin-independent scattering between dark matter and protons. The dark matter particle mass is set to 1 MeV, and all other cosmological parameters are set to their best-fit Planck 2015 values \citep{Ade:2015xua}. Different residual curves display cutoffs at different angular scales, controlled by the magnitude of the interaction cross section. The highest cross section shown corresponds to the current 95\% confidence-level upper limit inferred from analyses of CMB data \citep{Gluscevic:2017ywp,Boddy:2018kfv}.
 \ADW{I think we need a better version of this figure.}
 }