sm fixes

src/Acronyms.bib

@@ -363,7 +363,7 @@
 @acronym{HDL,
   description = {Hardware description language.},
   short = {HDL},
-  long = {Hardware description lanuage}
+  long = {Hardware description language}
 }
 
 @acronym{V4L2,
@@ -373,7 +373,7 @@
 }
 
 @acronym{BSD,
-  description = {Berkeley Software Distribution.},
+description = {Berkeley Software Distribution.},
   short = {BSD},
   long = {Berkeley Software Distribution}
 }

src/Glossary.bib

@@ -333,7 +333,7 @@
 @entry{star-catalogue,
   name = {star catalogue},
   long = {star catalogue},
-  description = {is an \gls{astronomical-catalogue} that lists stars. In astronomy, many stars are referred to simply by catalogue numbers. There are a great many different star catalogue which have been produced for different purposes over the years. Most modern catalogues are available in electronic format and can be freely downloaded from space agencies' data centres. The largest is being compiled from the spacecraft Gaia and thus far has over a billion stars. Completeness and accuracy are described by the faintest limiting magnitude and the accuracy of the positions.%
+  description = {is an \gls{astronomical-catalogue} that lists stars. In astronomy, many stars are referred to simply by catalogue numbers. There are a great many different star catalogues which have been produced for different purposes over the years. Most modern catalogues are available in electronic format and can be freely downloaded from space agencies' data centres. The largest is being compiled from the spacecraft Gaia and thus far has over a billion stars. Completeness and accuracy are described by the faintest limiting magnitude and the accuracy of the positions.%
 			\footnote{\cite{enwiki:Star_catalogue}}
 }
 }

src/Introduction.tex

@@ -63,7 +63,7 @@ The chapters that follow are listed below.
 \end{description}
 \end{mdframed}
 \index{process}\index{hardware}\index{software}
-\index{acquire}\index{solve}\index{detect}\index{identify}\index{upload}
+\index{acquire}\index{detect}\index{identify}\index{upload}
 \index{support}
 
 

src/SNOUG.tex

@@ -220,7 +220,6 @@ leftmargin=1cm,rightmargin=1cm
 \usepackage[nonumberlist,record=hybrid,index,abbreviations,toc,indexcrossrefs,translate=babel,acronym]{glossaries-extra}
 
 \renewcommand{\abbreviationsname}{List of Abbreviations}
-\renewcommand{\acronymname}{List of Acronyms}
 \makeindex
 
 \setabbreviationstyle{long-short}
@@ -248,8 +247,9 @@ leftmargin=1cm,rightmargin=1cm
 }
 
 % OK, ACRONYM shows description, then short.
-% Show short first better.
-% Shows both when long=short, only one needed...
+% Showshort first better.
+% Shows both when desc=long, only one needed...
+% OK, but meh
 \renewcommand*{\glsxtrpostdescacronym}{%
   \space(\glsentrylong{\glscurrententrylabel})%
 }

src/Software.tex

@@ -394,7 +394,7 @@ at present.
 
 \section{GNSS with \texttt{gpsd}}
 \label{sec:software-gnss}
-\index{Galileo}\index{Beidou}
+\index{Galileo}
 
 
 \gls{GNSS} is used for time synchronization and for (somewhat)

src/Solve.tex

@@ -92,7 +92,6 @@ a plate of stars that has been extracted from \texttt{Source Extractor}. XXX
 
 \section{Star Catalogues}
 \label{sec:star-catalogues}
-\index{star-catalogue}
 
 To use a \gls{plate-solver}, you will need \glspl{star-catalogue}. They can get large.
 The \texttt{stvid} application includes a basic \gls{star-catalogue}.

src/Upload.tex

@@ -76,7 +76,7 @@ to the program's author, Cees Bassa:
 \begin{quote}
 With stvid, I typically store 10 seconds worth of video frames, 100 frames at 10 \gls{Hz} frame rate or 250 frames at 25 \gls{Hz} frame rate into a so-called ``four frame''. Here, for each pixel of the initial 100 or 250 frames, the mean, standard deviation, maximum and argmax are stored, each as its own frame. Objects that move will stand out because they will have a high (max - mean) / standard deviation, which allows me to detect trails. Once a trail is detected, the argmax frame tells me the frame number and hence the motion of the trail, and using the timestamps of the individual 100 or 250 frames, I can reconstruct the pixel position as a function of time during the 10 second exposure, using only 4 frames instead of the 100 or 250 individual video frames.
 \end{quote}
-\index{Bassa, Cees}\index{four frame}\index{trail}
+\index{Bassa, Cees}\index{four frame}
 \index{.fits}