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authorMohammad Akhlaghi <mohammad@akhlaghi.org>2019-07-08 00:44:50 +0100
committerMohammad Akhlaghi <mohammad@akhlaghi.org>2019-07-08 00:44:50 +0100
commit8ebb7848bf95d07e7162f46387ff4702f685da93 (patch)
tree232581f2666178bf21fa0066939be3a8ff915b8f
parent01ce2ccc075a9660186ca58683db93b1c06bf3e4 (diff)
Introduction for low surface brightness added
To present this talk in the IAU Symposium 355, a slide was added at the start to show the importance.
-rw-r--r--reproducible-paper.tex48
1 files changed, 45 insertions, 3 deletions
diff --git a/reproducible-paper.tex b/reproducible-paper.tex
index a44e352..475b60d 100644
--- a/reproducible-paper.tex
+++ b/reproducible-paper.tex
@@ -12,8 +12,8 @@
(\textcolor{blue}{\href{https://arxiv.org/abs/#1}{arXiv:#1}})}}
%% Set the title
-\title{\LARGE \textbf{BIG} data, \textbf{BIG} responsibility:\\
- \small Template/framework for reproducible scientific projects/papers}
+\title{\LARGE Digging out the low-surface-brightness universe\\
+ \small understanding and constraining the limits of methods used}
%% Set the author
\author{Mohammad Akhlaghi\\\vspace{2mm}\footnotesize Instituto de
@@ -24,7 +24,7 @@
}
%% Set the date and insitutional logos.
-\date{\scriptsize \href{https://eas.unige.ch/EWASS2019/session.jsp?id=SS34}{EWASS 2019, Special Session 34}, June 25th, 2019\\ Lyon, France}
+\date{\scriptsize \href{http://www.iac.es/congreso/iaus355}{IAU Symposium 355, Session 2}, July 8th, 2019\\ Tenerife, Spain}
%% For a wider writing width.
\newcommand\Wider[2][3em]{%
@@ -91,6 +91,48 @@
+ \newcommand{\imgtdir}{/home/mohammad/documents/personal/professional/astronomy/talks/in-prep/images}
+ \begin{frame}{Reproducibility is critically important for low surface brightness astronomy}
+ \small
+ \begin{columns}
+ \column{6cm} Example: Outer surface brighntess of M51 in a
+ \alert{single-exposure} SDSS image, using NoiseChisel.
+
+ \vspace{2mm}
+ \begin{itemize}
+ \setlength\itemsep{3mm}
+ \item Outer wing detected to \alert{$\rm{S/N}=1/20$} or
+ \alert{$30.06$ mag/arcsec$^2$}.
+ \item Deep/orange image from Watkins+2015
+ (\textcolor{blue}{\href{https://arxiv.org/abs/1501.04599}{arXiv:1501.04599}}).
+ \item
+ \textcolor{blue}{\href{https://www.gnu.org/software/gnuastro/manual/html_node/Detecting-large-extended-targets.html}{Complete
+ tutorial}} in manual fully describes how to derive/reproduce
+ this result:
+ \begin{itemize}
+ \item \alert{Run-time} options/configuration.
+ \item Steps \alert{before/after} NoiseChisel.
+ \end{itemize}
+ \item Default settings will \alert{not} give this result.
+ \end{itemize}
+
+ \vspace{2mm}
+ \begin{tcolorbox}[boxsep=0pt,left=1mm,right=1mm,top=1mm,bottom=1mm]
+ Simply reporting in your paper that ``\emph{we used
+ NoiseChisel}'' is \alert{not enough} to reproduce, understand,
+ or verify your result.
+ \end{tcolorbox}
+
+ \column{9cm}
+ \includegraphics[width=0.49\linewidth]{\imgtdir/m51-lf.pdf}
+ \includegraphics[width=0.49\linewidth]{\imgtdir/m51-detection.pdf}
+
+ \includegraphics[width=0.49\linewidth]{\imgtdir/m51-edge.pdf}
+ \includegraphics[width=0.49\linewidth]{\imgtdir/m51-watkins-zoom.png}
+ \end{columns}
+ \end{frame}
+
+
\begin{frame}{Reproducibility crisis in the sciences/astronomy}