From 8222fc9d8e2f6249ea6c2b6f5757a49e49cc1218 Mon Sep 17 00:00:00 2001 From: David Turner Date: Fri, 6 Sep 2024 15:50:24 -0400 Subject: [PATCH] Made a wording change to the summary Signed-off-by: David Turner --- paper/paper.md | 6 +++--- 1 file changed, 3 insertions(+), 3 deletions(-) diff --git a/paper/paper.md b/paper/paper.md index 4d940e22..e661fdce 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -58,9 +58,9 @@ preserving low-level control of processing for X-ray experts. It is useful for i observations of a single object of interest, but it excels at creating and managing multi-mission datasets for serendipitous or targeted studies of large samples of X-ray emitting objects. Once relevant observations are identified, the raw data can be downloaded (and optionally processed) through [Daxa]{.smallcaps}, or pre-processed -event lists, images, and exposure maps can be downloaded if they are available. With at least a decade-long `X-ray -desert' on the horizon, archival data will take on even greater importance, and enhanced access to those archives -will be vital to the continuation of X-ray astronomy. +event lists, images, and exposure maps can be downloaded if they are available. With a decade-long `X-ray +desert' potentially on the horizon, archival data will take on even greater importance, and enhanced access to +those archives will be vital to the continuation of X-ray astronomy. # Statement of need X-ray observations provide a powerful view of some of the most extreme processes in the Universe, and have had a