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Initial commit of paper moved from the timing-noise repo

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SHELL = /bin/bash
main = paper_cw_mcmc.pdf
.PHONY : main clean figclean arxiv jones
main : $(main)
git_tag.tex :
./git-tag.sh $@
$(main): *.tex git_tag.tex
pdflatex ${@:.pdf=} && bibtex ${@:.pdf=} && pdflatex ${@:.pdf=} && pdflatex ${@:.pdf=}
clean :
rm -f git_tag.tex $(main:.pdf=){.aux,.bbl,.blg,.log,.out,.pdf,Notes.bib} $(texfigs) $(texonlyfigs)
arxiv :
rm -f $(main)
rm -f git_tag.tex
tar -cvf arxiv_submission.tar *tex *bib bibliography.bib *pdf *.bbl
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primaryClass = "astro-ph.IM",
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author = {{Cutler}, C. and {Gholami}, I. and {Krishnan}, B.},
title = "{Improved stack-slide searches for gravitational-wave pulsars}",
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}
@ARTICLE{prix2009,
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title = "{Targeted search for continuous gravitational waves: Bayesian versus maximum-likelihood statistics}",
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}
@Article{ foreman-mackay2013,
author = {{Foreman-Mackey}, D. and {Hogg}, D.~W. and {Lang}, D. and
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title = "{emcee: The MCMC Hammer}",
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adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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@Article{goggans2004,
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@ARTICLE{wette2013,
author = {{Wette}, K. and {Prix}, R.},
title = "{Flat parameter-space metric for all-sky searches for gravitational-wave pulsars}",
journal = {\prd},
archivePrefix = "arXiv",
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@ARTICLE{wette2015,
author = {{Wette}, K.},
title = "{Parameter-space metric for all-sky semicoherent searches for gravitational-wave pulsars}",
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author = {{Prix}, R.},
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archivePrefix = {arXiv},
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\newcommand{\F}{{\mathcal{F}}}
\newcommand{\A}{\boldsymbol{\mathcal{A}}}
\newcommand{\blambda}{\boldsymbol{\mathbf{\lambda}}}
\newcommand{\blambdaSignal}{\boldsymbol{\mathbf{\lambda}}^{\rm s}}
\newcommand{\Tspan}{T_{\rm span}}
\newcommand{\Tcoh}{T_{\rm coh}}
\newcommand{\tref}{t_{\rm ref}}
\newcommand{\Nseg}{N_{\rm seg}}
\newcommand{\Nsteps}{N_{\rm steps}}
\newcommand{\Ntemps}{N_{\rm temps}}
\newcommand{\Nspindown}{N_{\rm spindowns}}
\renewcommand{\H}{\mathcal{H}}
\newcommand{\Hs}{\H_{\rm s}}
\newcommand{\Hn}{\H_{\rm n}}
\newcommand{\ho}{h_0}
\newcommand{\homax}{\ho^{\rm max}}
\newcommand{\Bsn}{B_{\rm S/N}}
\newcommand{\Pic}{\Pi_{\rm c}}
\newcommand{\mutilde}{\tilde{\mu}}
\newcommand{\Sn}{S_{\rm n}}
\newcommand{\V}{\mathcal{V}}
\newcommand{\Vsky}{\V_{\rm Sky}}
\newcommand{\Vpe}{\V_{\rm PE}}
\newcommand{\smax}{s_{\textrm{max}}}
\newcommand{\fmax}{f_{\textrm{max}}}
Paper/fully_coherent_search_using_MCMC_walkers.png

246 KiB

#!/bin/bash
FILE="$1"
if [ "x$FILE" = x ]; then
echo "usage: $0 <file.tex>" >&2
exit 1
fi
TMPFILE="$FILE.tmp"
gitLOG=`git log -1 --pretty="format:%% generated by $0
\\newcommand{\\commitDATE}{%ai}
\\newcommand{\\commitID}{commitID: %H}
\\newcommand{\\commitIDshort}{commitID: %h}
"`
echo "$gitLOG" > $TMPFILE
diffcmd="git diff -- .";
diff=`$diffcmd`;
if test -n "$diff"; then
echo "\\newcommand{\\commitSTATUS}{UNCLEAN}" >> $TMPFILE
else
echo "\\newcommand{\\commitSTATUS}{CLEAN}" >> $TMPFILE
fi
if cmp -s $TMPFILE $FILE; then
rm -f $TMPFILE
else
mv -f $TMPFILE $FILE
fi
Paper/grided_frequency_search_1D.png

46.9 KiB

This diff is collapsed.
\begin{tabular}{c|cccccc}
Stage & $\Nseg$ & $\Tcoh^{\rm days}$ &$\Nsteps$ & $\V$ & $\Vsky$ & $\Vpe$ \\ \hline
0 & 80 & 1.25 & 100 & 20.0 & 2.0 & 10.0 \\
1 & 40 & 2.5 & 100 & $2{\times}10^{2}$ & 7.0 & 20.0 \\
2 & 20 & 5.0 & 100 & $1{\times}10^{3}$ & 30.0 & 50.0 \\
3 & 10 & 10.0 & 100 & $1{\times}10^{4}$ & $1{\times}10^{2}$ & 90.0 \\
4 & 5 & 20.0 & 100 & $7{\times}10^{4}$ & $4{\times}10^{2}$ & $2{\times}10^{2}$ \\
5 & 1 & 100.0 & 100,100 & $1{\times}10^{6}$ & $1{\times}10^{3}$ & $9{\times}10^{2}$ \\
\end{tabular}
Paper/weak_signal_follow_up_walkers.png

1.32 MiB

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