From 6fefbd64388db685424d03cc24fc73f866743384 Mon Sep 17 00:00:00 2001 From: David Turner Date: Thu, 29 Aug 2024 22:28:09 -0400 Subject: [PATCH] Still still trying to make the paper build again Signed-off-by: David Turner --- paper/archive.md | 8 ++++++++ paper/paper.md | 8 -------- 2 files changed, 8 insertions(+), 8 deletions(-) create mode 100644 paper/archive.md diff --git a/paper/archive.md b/paper/archive.md new file mode 100644 index 00000000..69dbecd0 --- /dev/null +++ b/paper/archive.md @@ -0,0 +1,8 @@ +[//]: # (; from in-solar-system objects, to ) +[//]: # (supernovae, to galaxies and galaxy clusters.) + +[//]: # (Any such change will be recorded in the archive history, and processed ) + +[//]: # (observations version controlled, so that the data archive can have a specific version that refers to its exact state ) + +[//]: # (at any given time; this version can be referred to in published work using the data archive.) diff --git a/paper/paper.md b/paper/paper.md index 369c21d1..036ef189 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -63,8 +63,6 @@ no new X-ray missions coming online, during the next decade, archival data will enhanced access to those archives will be vital to the continuation of X-ray astronomy. # Statement of need -[//]: # (; from in-solar-system objects, to ) -[//]: # (supernovae, to galaxies and galaxy clusters.) X-ray observations provide a powerful view of some of the most extreme processes in the Universe, and have had a profound impact on our understanding of many types of astrophysical objects. As such, access to X-ray data should be made as simple as possible, both for X-ray experts and non-specialists whose research benefits from a high-energy @@ -154,14 +152,8 @@ processing it in the same way; this renders making fully processed, and large, X of research unnecessary. This feature in particular can be used to further one of the tenets of open-source science, reproducibility. -[//]: # (Any such change will be recorded in the archive history, and processed ) - -[//]: # (observations version controlled, so that the data archive can have a specific version that refers to its exact state ) - -[//]: # (at any given time; this version can be referred to in published work using the data archive.) # Existing software packages - There are no direct analogues to our module, though we must acknowledge the many pieces of software (and data archives), that greatly helped the development of [Daxa]{.smallcaps}. Data access is made possible primarily by the HEASARC data archive, though the Astroquery [@astroquery] package is also used.