From 561c20dfac90a7841dcb2ca33340b903d564bef0 Mon Sep 17 00:00:00 2001 From: DavidT3 Date: Wed, 2 Feb 2022 09:28:49 +0000 Subject: [PATCH] Made sure Tx and Lx are properly italicised --- paper/paper.md | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/paper/paper.md b/paper/paper.md index defc899d..54059b09 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -161,8 +161,8 @@ publication. The first of these is a hydrostatic and gas mass analysis of the redMaPPeR [@redmappersdss] SDSS selected XCS galaxy cluster sample [@sdssxcs] and well as the ACTDR5 [@actdr5] Sunyaev-Zel'dovich (SZ) selected XCS sample of galaxy clusters. This work also compares commonly measured X-ray properties of clusters -(the X-ray luminosity L$_{\rm{x}}$, and the temperature -T$_{\rm{x}}$) both to results from the existing XCS pipeline and from +(the X-ray luminosity $L_{\rm{x}}$, and the temperature +$T_{\rm{x}}$) both to results from the existing XCS pipeline and from literature, confirming that \texttt{XGA} measurements are consistent with previous work. This process is repeated with \texttt{XGA}'s galaxy cluster gas and hydrostatic mass measurements, again showing they are consistent with previous work. \texttt{XGA}'s ability to stack and combine X-ray surface brightness profiles is currently being used, in