diff --git a/src/cell.h b/src/cell.h
index 5e3b07f298d3a5f6de2c69a9d76aaacc59f33332..19bb11a7b9b4c49bcc4c04dc33019d5391749221 100644
--- a/src/cell.h
+++ b/src/cell.h
@@ -29,7 +29,12 @@ struct space;
 
 /* Some constants. */
 #define cell_sid_dt 13
-#define cell_max_tag (1 << 16)
+
+/* Max tag size set to 2^29 to take into account some MPI implementations 
+ * that use 2^31 as the upper bound on MPI tags and the fact that 
+ * cell_next_tag is multiplied by 2 when passed to an MPI function. 
+ * The maximum was lowered by a further factor of 2 to be on the safe side.*/
+#define cell_max_tag (1 << 29)
 
 /* Global variables. */
 extern int cell_next_tag;
diff --git a/theory/paper_pasc/Figures/Hierarchy3.pdf b/theory/paper_pasc/Figures/Hierarchy3.pdf
new file mode 100644
index 0000000000000000000000000000000000000000..235cd289b1dbda5ac509e46f5432bdaa7d636724
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diff --git a/theory/paper_pasc/Figures/Hierarchy3.svg b/theory/paper_pasc/Figures/Hierarchy3.svg
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diff --git a/theory/paper_pasc/acmcopyright.sty b/theory/paper_pasc/acmcopyright.sty
new file mode 100644
index 0000000000000000000000000000000000000000..e8de127a37213e171817b5eed65106ae4f6646b9
--- /dev/null
+++ b/theory/paper_pasc/acmcopyright.sty
@@ -0,0 +1,221 @@
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+   advantage and that copies bear this notice and the full citation on
+   the first page. Copyrights for components of this work owned by
+   others than ACM must be honored. Abstracting with credit is
+   permitted. To copy otherwise, or republish, to post on servers or to
+   redistribute to lists, requires prior specific permission
+   and\hspace*{.5pt}/or  a fee. Request permissions from
+   permissions@acm.org.
+  \or % acmlicensed
+   Permission to make digital or hard copies of all or part of this
+   work for personal or classroom use is granted without fee provided
+   that copies are not made or distributed for profit or commercial
+   advantage and that copies bear this notice and the full citation on
+   the first page. Copyrights for components of this work owned by
+   others than the author(s) must be honored. Abstracting with credit
+   is permitted.  To copy otherwise, or republish, to post on servers
+   or to  redistribute to lists, requires prior specific permission
+   and\hspace*{.5pt}/or  a fee. Request permissions from
+   permissions@acm.org.
+  \or % rightsretained
+   Permission to make digital or hard copies of part or all of this work
+   for personal or classroom use is granted without fee provided that
+   copies are not made or distributed for profit or commercial advantage
+   and that copies bear this notice and the full citation on the first
+   page. Copyrights for third-party components of this work must be
+   honored. For all other uses, contact the
+   owner\hspace*{.5pt}/author(s).
+  \or % usgov
+   This paper is authored by an employee(s) of the United States
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+   by an employee, or contractor of the national government. As such,
+   the Government retains a nonexclusive, royalty-free right to
+   publish or reproduce this article, or to allow others to do so, for
+   Government purposes only. Permission to make digital or hard copies
+   for personal or classroom use is granted. Copies must bear this
+   notice and the full citation on the first page. Copyrights for
+   components of this work owned by others than ACM must be
+   honored. To copy otherwise, distribute, republish, or post,
+   requires prior specific permission and\hspace*{.5pt}/or a
+   fee. Request permissions from permissions@acm.org.
+  \or % cagov
+   This article was authored by employees of the Government of Canada.
+   As such, the Canadian government retains all interest in the
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+   others to do so, provided that clear attribution is given both to
+   the authors and the Canadian government agency employing them.
+   Permission to make digital or hard copies for personal or classroom
+   use is granted. Copies must bear this notice and the full citation
+   on the first page.  Copyrights for components of this work owned by
+   others than the Canadain Government must be honored. To copy
+   otherwise, distribute, republish, or post, requires prior specific
+   permission and\hspace*{.5pt}/or a fee. Request permissions from
+   permissions@acm.org.
+  \or % cagovmixed
+   ACM acknowledges that this contribution was co-authored by an
+   affiliate of the national government of Canada. As such, the Crown
+   in Right of Canada retains an equal interest in the copyright.
+   Reprints must include clear attribution to ACM and the author's
+   government agency affiliation.  Permission to make digital or hard
+   copies for personal or classroom use is granted.  Copies must bear
+   this notice and the full citation on the first page. Copyrights for
+   components of this work owned by others than ACM must be honored.
+   To copy otherwise, distribute, republish, or post, requires prior
+   specific permission and\hspace*{.5pt}/or a fee. Request permissions
+   from permissions@acm.org.
+  \or % licensedusgovmixed
+   Publication rights licensed to ACM. ACM acknowledges that this
+   contribution was authored or co-authored by an employee, contractor
+   or affiliate of the United States government. As such, the
+   Government retains a nonexclusive, royalty-free right to publish or
+   reproduce this article, or to allow others to do so, for Government
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+  \or % licensedcagovmixed
+   Publication rights licensed to ACM. ACM acknowledges that this
+   contribution was authored or co-authored by an employee, contractor
+   or affiliate of the national government of Canada. As such, the
+   Government retains a nonexclusive, royalty-free right to publish or
+   reproduce this article, or to allow others to do so, for Government
+   purposes only.
+  \or % othergov
+   ACM acknowledges that this contribution was authored or co-authored
+   by an employee, contractor or affiliate of a national government. As
+   such, the Government retains a nonexclusive, royalty-free right to
+   publish or reproduce this article, or to allow others to do so, for
+   Government purposes only.
+  \or % licensedothergov
+   Publication rights licensed to ACM. ACM acknowledges that this
+   contribution was authored or co-authored by an employee, contractor
+   or affiliate of a national government. As such, the Government
+   retains a nonexclusive, royalty-free right to publish or reproduce
+   this article, or to allow others to do so, for Government purposes
+   only.
+  \fi}
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diff --git a/theory/paper_pasc/biblio.bib b/theory/paper_pasc/biblio.bib
new file mode 100644
index 0000000000000000000000000000000000000000..c0eead89fdf29d3503b5c2a11582f8b59ec45b8f
--- /dev/null
+++ b/theory/paper_pasc/biblio.bib
@@ -0,0 +1,392 @@
+@article{Springel2005,
+   author = {{Springel}, V.},
+    title = "{The cosmological simulation code GADGET-2}",
+  journal = {\mnras},
+   eprint = {astro-ph/0505010},
+ keywords = {methods: numerical, galaxies: interactions, dark matter},
+     year = 2005,
+    month = dec,
+   volume = 364,
+    pages = {1105-1134},
+      doi = {10.1111/j.1365-2966.2005.09655.x},
+   adsurl = {http://adsabs.harvard.edu/abs/2005MNRAS.364.1105S},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Price2012,
+   author = {{Price}, D.~J.},
+   title = "{Smoothed particle hydrodynamics and magnetohydrodynamics}",
+   journal = {Journal of Computational Physics},
+   archivePrefix = "arXiv",
+   eprint = {1012.1885},
+   primaryClass = "astro-ph.IM",
+   year = 2012,
+   month = feb,
+   volume = 231,
+   pages = {759-794},
+   doi = {10.1016/j.jcp.2010.12.011},
+   adsurl = {http://adsabs.harvard.edu/abs/2012JCoPh.231..759P},
+   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
+@article{Gingold1977,
+    title={Smoothed particle hydrodynamics-theory and application to non-spherical stars},
+    author={Gingold, Robert A and Monaghan, Joseph J},
+    journal={Monthly notices of the royal astronomical society},
+    volume={181},
+    pages={375--389},
+    year={1977}
+    }
+
+@article{Viccione2008,
+    title={Defining and optimizing algorithms for neighbouring particle identification in SPH fluid simulations},
+    author={Viccione, G and Bovolin, V and Carratelli, E Pugliese},
+    journal={International Journal for Numerical Methods in Fluids},
+    volume={58},
+    number={6},
+    pages={625--638},
+    year={2008},
+    publisher={Wiley Online Library}
+    }
+
+
+@article{Lee1977,
+    title={Worst-case analysis for region and partial region searches in multidimensional binary search trees and balanced quad trees},
+    author={Lee, Der-Tsai and Wong, CK},
+    journal={Acta Informatica},
+    volume={9},
+    number={1},
+    pages={23--29},
+    year={1977},
+    publisher={Springer}
+    }
+
+
+@article{Verlet1967,
+    title = {Computer ``Experiments'' on Classical Fluids. {I}. {T}hermodynamical Properties of {L}ennard-{J}ones Molecules},
+    author = {Verlet, Loup},
+    journal = {Physical Review},
+    volume = {159},
+    number = {1},
+    pages = {98},
+    year = {1967},
+    doi = {10.1103/PhysRev.159.98},
+    publisher = {American Physical Society}
+    }
+
+
+@book{Allen1989,
+    title={Computer simulation of liquids},
+    author={Allen, M.P. and Tildesley, D.J.},
+    volume={18},
+    number={195},
+    year={1989},
+    publisher={Oxford university press}
+    }
+
+@article{Barnes1986,
+  title={A hierarchical O (N log N) force-calculation algorithm},
+  author={Barnes, Josh and Hut, Piet},
+  journal={Nature},
+  year={1986},
+  publisher={Nature Publishing Group}
+}
+
+
+@article{Hernquist1989,
+    title={{TREESPH}-{A} unification of {SPH} with the hierarchical tree method},
+    author={Hernquist, Lars and Katz, Neal},
+    journal={The Astrophysical Journal Supplement Series},
+    volume={70},
+    pages={419--446},
+    year={1989}
+    }
+
+@article{Gonnet2012,
+    author = "Gonnet, Pedro",
+    title = "Pairwise {V}erlet lists: Combining cell lists and {V}erlet lists to improve memory locality and parallelism",
+    journal = "Journal of Computational Chemistry",
+    volume = "33",
+    issue = "1",
+    pages = "76--81",
+    year = "2012"
+    }
+
+@article{Gonnet2013,
+    title={Pseudo-{V}erlet lists: a new, compact neighbour list representation},
+    author={Gonnet, Pedro},
+    journal={Molecular Simulation},
+    volume={39},
+    number={9},
+    pages={721--727},
+    year={2013},
+    publisher={Taylor \& Francis}
+    }
+
+
+@article{Bentley1975,
+    title={Multidimensional binary search trees used for associative searching},
+    author={Bentley, Jon Louis},
+    journal={Communications of the ACM},
+    volume={18},
+    number={9},
+    pages={509--517},
+    year={1975},
+    publisher={ACM}
+    }
+
+@article{Wadsley2004,
+    title={Gasoline: a flexible, parallel implementation of {TreeSPH}},
+    author={Wadsley, JW and Stadel, Joachim and Quinn, Thomas},
+    journal={New Astronomy},
+    volume={9},
+    number={2},
+    pages={137--158},
+    year={2004},
+    publisher={Elsevier}
+    }
+
+@article{Dominguez2011,
+    title={Neighbour lists in smoothed particle hydrodynamics},
+    author={Dom{\'\i}nguez, JM and Crespo, AJC and G{\'o}mez-Gesteira, M and Marongiu, JC},
+    journal={International Journal for Numerical Methods in Fluids},
+    volume={67},
+    number={12},
+    pages={2026--2042},
+    year={2011},
+    publisher={Wiley Online Library}
+    }
+
+@article{Meagher1982,
+    title={Geometric modeling using octree encoding},
+    author={Meagher, Donald},
+    journal={Computer Graphics and Image Processing},
+    volume={19},
+    number={2},
+    pages={129--147},
+    year={1982},
+    publisher={Elsevier}
+    }
+@article{Carrier1988,
+  title={A fast adaptive multipole algorithm for particle simulations},
+  author={Carrier, J and Greengard, Leslie and Rokhlin, Vladimir},
+  journal={SIAM Journal on Scientific and Statistical Computing},
+  volume={9},
+  number={4},
+  pages={669--686},
+  year={1988},
+  publisher={SIAM}
+}
+
+
+@ARTICLE{Schaye2015,
+   author = {{Schaye}, J. and {Crain}, R.~A. and {Bower}, R.~G. and {Furlong}, M. and 
+	{Schaller}, M. and {Theuns}, T. and {Dalla Vecchia}, C. and 
+	{Frenk}, C.~S. and {McCarthy}, I.~G. and {Helly}, J.~C. and 
+	{Jenkins}, A. and {Rosas-Guevara}, Y.~M. and {White}, S.~D.~M. and 
+	{Baes}, M. and {Booth}, C.~M. and {Camps}, P. and {Navarro}, J.~F. and 
+	{Qu}, Y. and {Rahmati}, A. and {Sawala}, T. and {Thomas}, P.~A. and 
+	{Trayford}, J.},
+    title = "{The EAGLE project: simulating the evolution and assembly of galaxies and their environments}",
+  journal = {\mnras},
+archivePrefix = "arXiv",
+   eprint = {1407.7040},
+ keywords = {methods: numerical, galaxies: evolution, galaxies: formation, cosmology: theory},
+     year = 2015,
+    month = jan,
+   volume = 446,
+    pages = {521-554},
+      doi = {10.1093/mnras/stu2058},
+   adsurl = {http://adsabs.harvard.edu/abs/2015MNRAS.446..521S},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@inproceedings{gonnet2013swift,
+  title={SWIFT: Fast algorithms for multi-resolution SPH on multi-core architectures},
+  author={Gonnet, Pedro and Schaller, Matthieu and Theuns, Tom and Chalk, Aidan BG},
+  booktitle={8th International SPHERIC Workshop},
+  archivePrefix = "arXiv",
+  eprint = {1309.3783},
+  year={2013},
+  organization={Trondheim, Norway}
+}
+
+@inproceedings{theuns2015swift,
+  title={Swift: task-based hydrodynamics and gravity for cosmological simulations},
+  author={Theuns, Tom and Chalk, Aidan and Schaller, Matthieu and Gonnet, Pedro},
+  booktitle={Proceedings of the 3rd International Conference on Exascale Applications and Software},
+  pages={98--102},
+  year={2015},
+  organization={University of Edinburgh}
+}
+
+@article{gonnet2015efficient,
+  title={Efficient and Scalable Algorithms for Smoothed Particle Hydrodynamics on Hybrid Shared/Distributed-Memory Architectures},
+  author={Gonnet, Pedro},
+  journal={SIAM Journal on Scientific Computing},
+  volume={37},
+  number={1},
+  pages={C95--C121},
+  year={2015},
+  publisher={SIAM}
+}
+   
+@article{ref:Dagum1998,
+    title={{OpenMP}: an industry standard {API} for shared-memory programming},
+    author={Dagum, Leonardo and Menon, Ramesh},
+    journal={Computational Science \& Engineering, IEEE},
+    volume={5},
+    number={1},
+    pages={46--55},
+    year={1998},
+    publisher={IEEE}
+    }
+
+@book{ref:Snir1998,
+    title={{MPI}: The Complete Reference (Vol. 1): Volume 1-The {MPI} Core},
+    author={Snir, Marc and Otto, Steve and Huss-Lederman, Steven and Walker, David and Dongarra, Jack},
+    volume={1},
+    year={1998},
+    publisher={MIT press}
+    }
+
+@inproceedings{warren1993parallel,
+  title={A parallel hashed oct-tree n-body algorithm},
+  author={Warren, Michael S and Salmon, John K},
+  booktitle={Proceedings of the 1993 ACM/IEEE conference on Supercomputing},
+  pages={12--21},
+  year={1993},
+  organization={ACM}
+}
+
+@article{gonnet2013quicksched,
+   author = {{Gonnet}, P. and {Chalk}, A.~B.~G. and {Schaller}, M.},
+    title = "{QuickSched: Task-based parallelism with dependencies and conflicts}",
+  journal = {ArXiv e-prints},
+archivePrefix = "arXiv",
+   eprint = {1601.05384},
+ primaryClass = "cs.DC",
+ keywords = {Computer Science - Distributed, Parallel, and Cluster Computing},
+     year = 2016,
+    month = jan,
+   adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160105384G},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
+
+
+@book{ref:Blumofe1995,
+	number = {8}, 
+	year = {1995}, 
+	author = {Blumofe, R.D. and Joerg, C.F. and Kuszmaul, B.C. and Leiserson, C.E. and Randall, K.H. and Zhou, Y.}, 
+	volume = {30}, 
+	publisher = {ACM}, 
+	title = {Cilk: An efficient multithreaded runtime system}, 
+    }
+
+@manual{ref:QUARK,
+	month = {April}, 
+	year = {2011}, 
+	author = {YarKhan, A. and Kurzak, J. and Dongarra, J.}, 
+	address = {Electrical Engineering and Computer Science, Innovative Computing Laboratory, University of Tennessee}, 
+	publisher = {University of Tennessee}, 
+	title = {QUARK Users' Guide}, 
+}
+
+@manual{ref:SMPSuperscalar,
+	year = {2008}, 
+	publisher = {Barcelona Supercomputing Center}, 
+	title = {{SMP} {S}uperscalar ({SMPS}s) User's Manual, {B}arcelona Supercomputing Center}, 
+}
+
+@article{ref:Augonnet2011,
+	year = {2011}, 
+	author = {Augonnet, C\'edric and Thibault, Samuel and Namyst, Raymond and Wacrenier, Pierre-Andr\'e}, 
+	journal = {Concurrency and Computation: Practice and Experience, Special Issue: Euro-Par 2009}, 
+	volume = {23}, 
+	pages = {187--198}, 
+	publisher = {John Wiley & Sons, Ltd.}, 
+	doi = {10.1002/cpe.1631}, 
+	url = {http://hal.inria.fr/inria-00550877}, 
+	title = {Star{PU}: A Unified Platform for Task Scheduling on Heterogeneous Multicore Architectures}, 
+}
+
+@article{ref:Duran2009,
+    title={A proposal to extend the {OpenMP} tasking model with dependent tasks},
+    author={Duran, Alejandro and Ferrer, Roger and Ayguad{\'e}, Eduard and Badia, Rosa M and Labarta, Jesus},
+    journal={International Journal of Parallel Programming},
+    volume={37},
+    number={3},
+    pages={292--305},
+    year={2009},
+    publisher={Springer}
+    }
+
+@book{ref:Reinders2007,
+    title={Intel threading building blocks: outfitting {C++} for multi-core processor parallelism},
+    author={Reinders, James},
+    year={2007},
+    publisher={O'Reilly Media, Incorporated}
+    }
+
+@inproceedings{ref:Agullo2009,
+    title={Numerical linear algebra on emerging architectures: The {PLASMA} and {MAGMA} projects},
+    author={Agullo, Emmanuel and Demmel, Jim and Dongarra, Jack and Hadri, Bilel and Kurzak, Jakub and Langou, Julien and Ltaief, Hatem and Luszczek, Piotr and Tomov, Stanimire},
+    booktitle={Journal of Physics: Conference Series},
+    volume={180},
+    number={1},
+    pages={012037},
+    year={2009},
+    organization={IOP Publishing}
+    }
+
+@article{ref:Bangerth2007,
+    author = 	 {W. Bangerth and R. Hartmann and G. Kanschat},
+    title = 	 {{deal.II} -- a General Purpose Object Oriented Finite Element Library},
+    journal = 	 {ACM Trans. Math. Softw.},
+    year = 	 "2007",
+    volume = 	 "33",
+    number = 	 "4",
+    pages = 	 {24/1--24/27}
+    }
+      
+@article{ref:Karypis1998,
+    title={A fast and high quality multilevel scheme for partitioning irregular graphs},
+    author={Karypis, George and Kumar, Vipin},
+    journal={SIAM Journal on scientific Computing},
+    volume={20},
+    number={1},
+    pages={359--392},
+    year={1998},
+    publisher={SIAM}
+    }
+
+@article{devine2002zoltan,
+  title={Zoltan data management services for parallel dynamic applications},
+  author={Devine, Karen and Boman, Erik and Heaphy, Robert and Hendrickson, Bruce and Vaughan, Courtenay},
+  journal={Computing in Science \& Engineering},
+  volume={4},
+  number={2},
+  pages={90--96},
+  year={2002},
+  publisher={IEEE}
+}
+
+
+@article{ref:Gonnet2015,
+ author    = {Pedro Gonnet},
+  title     = {Efficient and Scalable Algorithms for Smoothed Particle Hydrodynamics
+               on Hybrid Shared/Distributed-Memory Architectures},
+  journal   = {{SIAM} J. Scientific Computing},
+  volume    = {37},
+  number    = {1},
+  year      = {2015},
+  url       = {http://dx.doi.org/10.1137/140964266},
+  doi       = {10.1137/140964266},
+  timestamp = {Thu, 12 Mar 2015 10:30:34 +0100},
+  biburl    = {http://dblp.uni-trier.de/rec/bib/journals/siamsc/Gonnet15},
+  bibsource = {dblp computer science bibliography, http://dblp.org}
+}
+
diff --git a/theory/paper_pasc/pasc_paper.tex b/theory/paper_pasc/pasc_paper.tex
new file mode 100644
index 0000000000000000000000000000000000000000..629ff7bc1b01b629dc1b909b7675dfadc8c1c14d
--- /dev/null
+++ b/theory/paper_pasc/pasc_paper.tex
@@ -0,0 +1,825 @@
+\documentclass{sig-alternate-05-2015}
+\usepackage{times,amsmath,amsfonts,amssymb,epstopdf,xspace}
+\usepackage{graphicx}
+\usepackage{hyperref}
+\usepackage[usenames]{color}
+
+
+\newcommand{\red}[1]{{\textcolor{red}{#1}}}
+
+\pdfminorversion=7
+
+
+%Journals
+\newcommand{\mnras}{MNRAS}
+\newcommand{\jcap}{JCAP}
+\newcommand{\physrep}{Phys.~Rep.}   % Physics Reports
+\newcommand{\apjs}{ApJS}
+
+% Latex tricks
+\newcommand{\oh}[1]{\mbox{$ {\mathcal O}( #1 ) $}}
+\newcommand{\eqn}[1] {(\ref{eqn:#1})}
+\makeatletter
+\newcommand{\pushright}[1]{\ifmeasuring@#1\else\omit\hfill$\displaystyle#1$\fi\ignorespaces}
+\makeatother
+
+% Some acronyms
+\newcommand{\gadget}{{\sc Gadget-2}\xspace}
+\newcommand{\swift}{{\sc swift}\xspace}
+\newcommand{\qs}{{\sc QuickSched}\xspace}
+
+% Webpage
+\newcommand{\web}{\url{www.swiftsim.com}}
+
+
+%#####################################################################################################
+
+\begin{document}
+
+%Conference
+\conferenceinfo{PASC '16}{June 8--10, 2016, Lausanne, Switzerland}
+
+\title{{\ttlit SWIFT}: Using task-based parallelism, fully asynchronous
+communication, and graph partition-based domain decomposition for
+strong scaling on more than 100\,000 cores.}
+% \title{{\ttlit SWIFT}: A task-based hybrid-parallel strongly scalable code for
+%   particle-based cosmological simulations}
+
+\numberofauthors{6}
+  
+\author{
+\alignauthor
+       Matthieu~Schaller\\
+       \affaddr{Institute for Computational Cosmology (ICC)}\\
+       \affaddr{Department of Physics}\\
+       \affaddr{Durham University}\\
+       \affaddr{Durham DH1 3LE, UK}\\
+       \email{\footnotesize \url{matthieu.schaller@durham.ac.uk}}
+\alignauthor
+       Pedro~Gonnet\\
+       \affaddr{School of Engineering and Computing Sciences}\\
+       \affaddr{Durham University}\\
+       \affaddr{Durham DH1 3LE, UK}\\
+\alignauthor
+       Aidan~B.~G.~Chalk\\
+       \affaddr{School of Engineering and Computing Sciences}\\
+       \affaddr{Durham University}\\
+       \affaddr{Durham DH1 3LE, UK}\\
+\and
+\alignauthor
+       Peter~W.~Draper\\
+       \affaddr{Institute for Computational Cosmology (ICC)}\\
+       \affaddr{Department of Physics}\\
+       \affaddr{Durham University}\\
+       \affaddr{Durham DH1 3LE, UK}\\
+       %% \alignauthor
+       %% Tom Theuns\\
+       %% \affaddr{Institute for Computational Cosmology}\\
+       %% \affaddr{Department of Physics}\\
+       %% \affaddr{Durham University}\\
+       %% \affaddr{Durham DH1 3LE, UK}      
+}
+
+
+\date{\today}
+
+\maketitle
+
+%#####################################################################################################
+
+\begin{abstract}
+  We present a new open-source cosmological code, called \swift, designed to
+  solve the equations of hydrodynamics using a particle-based approach (Smooth
+  Particle Hydrodynamics) on hybrid shared / distributed-memory architectures.
+  \swift was designed from the bottom up to provide excellent {\em strong scaling}
+  on both commodity clusters (Tier-2 systems) and Top100-supercomputers
+  (Tier-0 systems), without relying on architecture-specific features
+  or specialized accelerator hardware.
+  This performance is due to three main computational approaches:
+
+  \begin{itemize}
+    
+    \item \textbf{Task-based parallelism} for shared-memory
+      parallelism, which provides fine-grained load balancing and
+      thus strong scaling on large numbers of cores.
+
+    \item \textbf{Graph-based domain decomposition}, which uses
+      the task graph to decompose the simulation
+      domain such that the {\em work}, as opposed to just the {\em data},
+      as is the case with most partitioning schemes, is equally distributed
+      across all nodes.
+
+    \item \textbf{Fully dynamic and asynchronous communication},
+      in which communication is modelled as just another task in
+      the task-based scheme, sending data whenever it is ready and
+      deferring on tasks that rely on data from other nodes
+      until it arrives.
+
+  \end{itemize}
+  
+  %% These three main aspects alongside improved cache-efficient
+  %% algorithms for neighbour finding allow the code to be 40x faster on
+  %% the same architecture than the standard code Gadget-2 widely used by
+  %% researchers.
+
+  In order to use these approaches, the code had to be re-written from
+  scratch, and the algorithms therein adapted to the task-based paradigm.
+  As a result, we can show upwards of 60\% parallel efficiency for 
+  moderate-sized problems when increasing the number of cores 512-fold,
+  on both x86-based and Power8-based architectures.
+  
+  %% As a result, our code present excellent \emph{strong}
+  %% scaling on a variety of architectures, ranging from x86 Tier-2 systems to the
+  %% largest Tier-0 machines currently available. It displays, for instance, a
+  %% \emph{strong} scaling parallel efficiency of more than 60\% when going from
+  %% 512 to 131072 cores on a Blue Gene architecture. Similar results are obtained
+  %% on standard clusters of x86 CPUs.
+  
+  %% The task-based library, \qs, used as the backbone of the code is
+  %% itself also freely available and can be used in a wide variety of
+  %% other numerical problems.
+  
+\end{abstract}
+
+
+\keywords{Physics; Cosmology; Fluid dynamics; Smooth Particle Hydrodynamics;
+  Task-based parallelism; Asynchronous data transfer; Extreme scaling}
+
+%#####################################################################################################
+
+
+\section{Introduction}
+
+For the past decade physical limitations have kept the speed of
+individual processor cores constrained, so instead of getting {\em
+  faster}, computers are getting {\em more parallel}.  Systems
+containing up to 64 general-purpose cores are becoming commonplace,
+and the number of cores can be expected to continue growing
+exponentially, e.g.~following Moore's law, much in the same way
+processor speeds were up until a few years ago.
+
+As a consequence, in order to get faster, computer programs need to
+rely on better exploitation of this massive parallelism, i.e.~ they
+need to exhibit {\em strong scaling}, the ability to run roughly $N$
+times faster when executed on $N$ times as many processors.  Without
+strong scaling, massive parallelism can still be used to tackle ever
+{\em larger} problems, but not make fixed-size problems {\em faster}.
+
+Although this switch from growth in speed to growth in parallelism
+has been anticipated and observed for quite some time, very little
+has changed in terms of how we design and implement parallel
+computations.
+Branch-and-bound synchronous parallelism using
+OpenMP\cite{ref:Dagum1998} and MPI\cite{ref:Snir1998}, as well as domain
+decompositions based on geometry or space-filling curves \cite{warren1993parallel}
+are still commonplace, despite both the
+architectures and problem scales having changed dramatically since
+their introduction.
+
+The design and implementation of \swift\footnote{
+\swift is an open-source software project and the latest version of
+the source code, along with all the data needed to run the test cased
+presented in this paper, can be downloaded at \web.}
+\cite{gonnet2013swift,theuns2015swift,gonnet2015efficient}, a large-scale
+cosmological simulation code built from scratch, provided the perfect
+opportunity to test some newer
+approaches, i.e.~task-based parallelism, fully asynchronous communication, and
+graph partition-based domain decompositions.
+
+This paper describes these techniques, which are not exclusive to
+cosmological simulations or any specific architecture, as well as
+the results obtained with them.
+
+
+%#####################################################################################################
+
+\section{Particle-based hydrodynamics}
+
+Smoothed Particle Hydrodynamics \cite{Gingold1977,Price2012} (SPH) uses
+particles to represent fluids.  Each particle $p_i$ has a position $\mathbf
+x_i$, velocity $\mathbf v_i$, internal energy $u_i$, mass $m_i$, and a smoothing
+length $h_i$.  The particles are used to interpolate any quantity $Q$ at any
+point in space as a weighted sum over the particles:
+%
+\begin{equation}
+    Q(\mathbf r) = \sum_i m_i \frac{Q_i}{\rho_i} W( \|\mathbf r - \mathbf r_i\| , h )
+    \label{eqn:interp}
+\end{equation}
+%
+where $Q_i$ is the quantity at the $i$th particle, $h$ is the {\em smoothing
+  length}, i.e.~the radius of the sphere within which data will be considered
+for the interpolation, and $W(r,h)$ is the {\em smoothing kernel} or {\em
+  smoothing function}.  Several different forms for $W(r,h)$ exist, each with
+their own specific benefits and drawbacks.
+
+The particle density $\rho_i$ used in \eqn{interp} is itself computed similarly:
+%
+\begin{equation}
+    \rho_i = \sum_{j,~r_{ij} < h_i} m_j W(r_{ij},h_i)
+    \label{eqn:rho}
+\end{equation}
+%
+where $r_{ij} = \|\mathbf{r_i}-\mathbf{r_j}\|$ is the Euclidean distance between
+particles $p_i$ and $p_j$.  In compressible simulations, the smoothing length
+$h_i$ of each particle is chosen such that the number of neighbours with which
+it interacts is kept more or less constant, and can result in smoothing lengths
+spanning several orders of magnitudes within the same simulation.
+
+Once the densities $\rho_i$ have been computed, the time derivatives of the
+velocity and internal energy, which require $\rho_i$, are
+computed as follows:
+%
+\begin{align}
+    \frac{dv_i}{dt} & = -\sum_{j,~r_{ij} < \hat{h}_{ij}} m_j \left[
+        \frac{P_i}{\Omega_i\rho_i^2}\nabla_rW(r_{ij},h_i)\right. + \label{eqn:dvdt}\\
+        & \pushright{\left.\frac{P_j}{\Omega_j\rho_j^2}\nabla_rW(r_{ij},h_j) \right], \nonumber} \\ 
+    \frac{du_i}{dt} & = \frac{P_i}{\Omega_i\rho_i^2} \sum_{j,~r_{ij} < h_i} m_j(\mathbf v_i - \mathbf v_j) \cdot \nabla_rW(r_{ij},h_i), \label{eqn:dudt}
+\end{align}
+%
+where $\hat{h}_{ij} = \max\{h_i,h_j\}$, and the particle pressure $P_i=\rho_i
+u_i (\gamma-1)$ and correction term $\Omega_i=1 +
+\frac{h_i}{3\rho_i}\frac{\partial \rho}{\partial h}$ are computed on the fly.
+
+The computations in \eqn{rho}, \eqn{dvdt}, and \eqn{dudt} involve finding all
+pairs of particles within range of each other.  Any particle $p_j$ is {\em
+  within range} of a particle $p_i$ if the distance between $p_i$ and $p_j$ is
+smaller or equal to the smoothing distance $h_i$ of $p_i$, e.g.~as is done in
+\eqn{rho}.  Note that since particle smoothing lengths may vary between
+particles, this association is not symmetric, i.e.~$p_j$ may be in range of
+$p_i$, but $p_i$ not in range of $p_j$.  If $r_{ij} < \max\{h_i,h_j\}$, as is
+required in \eqn{dvdt}, then particles $p_i$ and $p_j$ are within range {\em of
+each other}.
+
+The computation thus proceeds in two distinct stages that are evaluated
+separately:
+\begin{enumerate}
+    \item {\em Density} computation: For each particle $p_i$,
+        loop over all particles $p_j$ within range of $p_i$ and evaluate
+        \eqn{rho}.
+    \item {\em Force} computation: For each particle $p_i$,
+        loop over all particles $p_j$
+        within range of each other and evaluate \eqn{dvdt} and \eqn{dudt}.
+\end{enumerate}
+
+Finding the interacting neighbours for each particle constitutes
+the bulk of the computation.
+Many codes, e.g. in Astrophysics simulations \cite{Gingold1977},
+rely on spatial {\em trees}
+for neighbour finding \cite{Gingold1977,Hernquist1989,Springel2005,Wadsley2004},
+i.e.~$k$-d trees \cite{Bentley1975} or octrees \cite{Meagher1982}
+are used to decompose the simulation space.
+In Astrophysics in particular, spatial trees are also a somewhat natural
+choice as they are used to compute long-range gravitational interactions
+via a Barnes-Hut \cite{Barnes1986} or Fast Multipole
+\cite{Carrier1988} method. 
+The particle interactions are then computed by traversing the list of
+particles and searching for their neighbours in the tree.
+
+Although such tree traversals are trivial to parallelize, they
+have several disadvantages, e.g.~with regards to computational
+efficiency, cache efficiency, and exploiting symmetries in the
+computation (see \cite{gonnet2015efficient} for a more detailed
+analysis).
+
+
+%#####################################################################################################
+
+\section{Parallelization strategy}
+
+One of the main concerns when developing \swift was to break
+with the branch-and-bound type parallelism inherent to parallel
+codes using OpenMP and MPI, and the constant synchronization
+between computational steps it results in.
+
+If {\em synchronization} is the main problem, then {\em
+  asynchronicity} is the obvious solution.  We therefore opted for a
+{\em task-based} approach for maximum single-node, or shared-memory,
+performance.  This approach not only provides excellent load-balancing
+on a single node, it also provides a powerful model of the computation
+that can be used to distribute the work equitably over a set of
+distributed-memory nodes using general-purpose graph partitioning
+algorithms.  Finally, the necessary communication between nodes can
+itself be modelled in a task-based way, interleaving communication
+seamlessly with the rest of the computation.
+
+
+\subsection{Task-based parallelism}
+
+Task-based parallelism is a shared-memory parallel programming
+paradigm in which a computation is broken-down in to a set of
+{\em tasks} which can be executed  concurrently.
+In order to ensure that the tasks are executed in the right
+order, e.g.~that data needed by one task is only used once it
+has been produced by another task, {\em dependencies} between
+tasks are specified and strictly enforced by a task scheduler.
+Additionally, if two tasks require exclusive access to the same
+resource, yet in no particular order, they are treated as
+{\em conflicts} and the scheduler ensures that they are not executed
+concurrently.
+Computations described in this way then parallelize trivially:
+each processor repeatedly grabs a task for which all dependencies
+have been satisfied and executes it until there are no tasks left.
+
+The main advantages of using a task-based approach are
+%
+\begin{itemize}
+    \item The order in which the tasks are processed, and how they
+        are assigned to each processor is completely
+        dynamic and adapts automatically to load imbalances.
+    \item If the dependencies and conflicts are specified correctly,
+        there is no need for expensive explicit locking, synchronization,
+        or atomic operations to deal with most concurrency problems.
+    \item Each task has exclusive access to the data it is working on,
+        thus improving cache locality and efficiency.
+\end{itemize}
+%
+Task-based parallelism is not a particularly new concept and therefore
+several implementations thereof exist, e.g.~Cilk \cite{ref:Blumofe1995},
+QUARK \cite{ref:QUARK}, StarPU \cite{ref:Augonnet2011},
+SMP~Superscalar \cite{ref:SMPSuperscalar}, OpenMP~3.0 \cite{ref:Duran2009},
+and Intel's TBB \cite{ref:Reinders2007}.
+
+For convenience, and to make experimenting with different scheduling
+techniques easier, we chose to implement our own task scheduler
+in \swift, which has since been back-ported as the general-purpose
+\qs task scheduler \cite{gonnet2013quicksched}.
+This also allowed us to extend the scheduler with the concept of
+task conflicts.
+
+Despite its advantages, and the variety of implementations,
+task-based parallelism is rarely used in
+practice (notable exceptions include the PLASMA project
+\cite{ref:Agullo2009} which uses QUARK/StarPU, and the {\tt deal.II} project
+\cite{ref:Bangerth2007} which uses Intel's TBB).
+The main problem is that to effectively use task-based parallelism,
+most computations need to be completely redesigned to fit the paradigm,
+which is usually not an option for large and complex codebases.
+
+Since we were re-implementing \swift from scratch, this was not an issue.
+The tree-based neighbour-finding described above was replaced with a more
+task-friendly approach as described in \cite{gonnet2015efficient}.
+Particle interactions are computed within, and between pairs, of
+hierarchical {\em cells} containing one or more particles.
+The dependencies between the tasks are set following
+equations \eqn{rho}, \eqn{dvdt}, and \eqn{dudt}, i.e.~such that for any cell,
+all the tasks computing the particle densities therein must have
+completed before the particle forces can be computed, and all the
+force computations must have completed before the particle velocities
+may be updated.
+The task hierarchy is shown in Fig.~\ref{tasks}, where the particles in each
+cell are first sorted (round tasks) before the particle densities
+are computed (first layer of square tasks).
+Ghost tasks (triangles) are used to ensure that all density computations
+on a cell of particles have completed before the force evaluation tasks
+(second layer of square tasks) execute.
+Once all the force tasks on a cell of particles have completed,
+the integrator tasks (inverted triangles) update the particle positions 
+and velocities.
+
+Due to the cache-friendly nature of the task-based computations, 
+and their ability to exploit symmetries in the particle interactions,
+the task-based approach is already more efficient than the tree-based
+neighbour search on a single core, and scales efficiently to all
+cores of a shared-memory machine \cite{gonnet2015efficient}.
+
+\begin{figure}
+\centering
+\includegraphics[width=\columnwidth]{Figures/Hierarchy3}
+\caption{Task hierarchy for the SPH computations in \swift,
+  including communication tasks. Arrows indicate dependencies,
+  i.e.~an arrow from task $A$ to task $B$ indicates that $A$
+  depends on $B$. The task color corresponds to the cell or
+  cells it operates on, e.g.~the density and force tasks work
+  on individual cells or pairs of cells.
+  The blue cell data is on a separate rank as the yellow and
+  purple cells, and thus its data must be sent across during
+  the computation using {\tt send}/{\tt recv} tasks (diamond-shaped).}
+\label{tasks}
+\end{figure}  
+
+
+\subsection{Task-based domain decomposition}
+
+Given a task-based description of a computation, partitioning it over
+a fixed number of {\em ranks} (using the MPI terminology)
+is relatively straight-forward: we create
+a {\em cell hypergraph} in which:
+\begin{itemize}
+  \item Each {\em node} represents a single cell of particles, and,
+  \item each {\em edge} represents the tasks, connecting the
+    cells.
+\end{itemize}
+Since in the particular case of \swift each task references at most
+two cells, the cell hypergraph is just a regular {\em cell graph}.
+
+Any partition of the cell graph represents a partition of the
+computation, i.e.~the nodes belonging to each partition each belong
+to a rank, and the
+data belonging to each cell resides on the partition/rank to which
+it has been assigned.
+Any task spanning cells that belong to the same partition needs only
+to be evaluated on that rank/partition, and tasks spanning more than
+one partition need to be evaluated on both ranks/partitions.
+
+If we then weight each edge with the computational cost associated with
+the tasks, then finding a {\em good} cell distribution reduces to finding a
+partition of the cell graph such that the maximum sum of the weight
+of all edges within and spanning in a partition is minimal
+(see Fig.~\ref{taskgraphcut}).
+Since the sum of the weights is directly proportional to the amount
+of computation per rank/partition, minimizing the maximum sum
+corresponds to minimizing the time spent on the slowest rank.
+Computing such a partition is a standard graph problem and several
+software libraries which provide good solutions\footnote{Computing
+the optimal partition for more than two nodes is considered NP-hard.},
+e.g.~METIS \cite{ref:Karypis1998} and Zoltan \cite{devine2002zoltan},
+exist.
+
+Note that this approach does not explicitly consider any geometric
+constraints, or strive to partition the {\em amount} of data equitably.
+The only criteria is the computational cost of each partition, for
+which the task decomposition provides a convenient model.
+We are therefore partitioning the {\em computation}, as opposed
+to just the {\em data}.
+
+Note also that the proposed partitioning scheme takes neither the
+task hierarchy, nor the size of the data that needs to be exchanged
+between partitions/ranks into account.
+This approach is therefore only reasonable in situations in which
+the task hierarchy is wider than flat, i.e.~the length of the critical
+path in the task graph is much smaller than the sum of all tasks,
+and in which communication latencies are negligible.
+
+\begin{figure}
+\centering
+\includegraphics[width=0.8\columnwidth]{Figures/task_graph_cut}
+\caption{Illustration of the task-based domain decomposition
+  in which the tasks (circles) are {\em hyperedges} that connect one or
+  more resources (rectangles). The resources are partitioned
+  along the thick dotted line. The blue and orange tasks are
+  executed on the respective partitions, whereas the green
+  tasks/hyperedges along the cut line are executed on both.
+  The cost of this partition is the sum of the green tasks,
+  which are computed twice, as well as the cost imbalance
+  of the tasks executed in each partition.}
+\label{taskgraphcut}
+\end{figure}  
+
+
+\subsection{Asynchronous communications}
+
+Although each particle cell resides on a specific rank, the particle
+data will still need to be sent to any neighbouring ranks that have
+tasks that depend on this data, e.g.~the the green tasks in
+Fig.~\ref{taskgraphcut}.
+This communication must happen twice at each time-step: once to send
+the particle positions for the density computation, and then again
+once the densities have been aggregated locally for the force
+computation.
+
+Most distributed-memory codes based on MPI \cite{ref:Snir1998}
+separate computation and communication into distinct steps, i.e.~all
+the ranks first exchange data, and only when the data exchange is
+complete does computation start. Further data exchanges only happen
+once computation has finished, and so on.
+This approach, although conceptually simple and easy to implement,
+has three major drawbacks:
+\begin{itemize}
+  \item The frequent synchronization points between communication
+    and computation exacerbate load imbalances,
+  \item the communication phase consists mainly of waiting on
+    latencies, during which the node's CPUs usually run idle, and
+  \item during the computation phase, the communication network
+    is left completely unused, whereas during the communication
+    phase, all ranks attempt to use it at the same time.
+\end{itemize}
+
+It is for these reasons that in \swift we opted for a fully
+{\em dynamic and asynchronous} communication model in which local
+data is sent whenever it is ready, data from other ranks is
+only acted on once it has arrived, and there is no separation into
+communication and computational phases.
+In practice this means that no rank will sit idle waiting on
+communication if there is any computation that can be done.
+
+This fits in quite naturally within the task-based framework
+by modelling communication as just another task type, i.e.~adding
+tasks that send and receive particle data between ranks.
+For every task that uses data that resides on a different rank,
+{\tt send} and {\tt recv} tasks are generated automatically on the source
+and destination ranks respectively.
+At the destination, the task is made dependent of the {\tt recv}
+task, i.e.~the task can only execute once the data has actually
+been received.
+This is illustrated in Fig.~\ref{tasks}, where data is exchanged across
+two ranks for the density and force computations and the extra
+dependencies are shown in red.
+
+The communication itself is implemented using the non-blocking
+{\tt MPI\_Isend} and {\tt MPI\_Irecv} primitives to initiate
+communication, and {\tt MPI\_Test} to check if the communication was
+successful and resolve the communication task's dependencies.  In the
+task-based scheme, strictly local tasks which do not rely on
+communication tasks are executed first.  As data from other ranks
+arrive, the corresponding non-local tasks are unlocked and are
+executed whenever a thread picks them up.
+
+One direct consequence of this approach is that instead of a single
+{\tt send}/{\tt recv} call between each pair of neighbouring ranks,
+one such pair is generated for each particle cell.
+This type of communication, i.e.~several small messages instead of
+one large message, is usually strongly discouraged since the sum of
+the latencies for the small messages is usually much larger than
+the latency of the single large message.
+This, however, is of no concern in \swift since nobody is actively
+waiting to receive the messages in order, and the communication
+latencies are covered by local computations.
+A nice side-effect of this approach is that communication no longer
+happens in bursts involving all the ranks at the same time, but
+is more or less evenly spread over the entire computation, and is
+therefore less demanding of the communication infrastructure.
+
+
+
+%#####################################################################################################
+
+\section{Scaling tests}
+
+In this section we present some strong scaling tests of the \swift code on different
+architectures for a representative cosmology problem.
+
+\subsection{Simulation setup}
+
+In order to provide a realistic setup, 
+the initial particle distributions used in our tests were extracted by
+resampling low-redshift outputs of the EAGLE project \cite{Schaye2015}, a
+large suite of state-of-the-art cosmological simulations. By selecting outputs
+at late times (redshift $z=0.5$), we constructed a simulation setup which is
+representative of the most expensive part of these simulations, i.e.~when the
+particles are highly-clustered and no longer uniformly distributed. This
+distribution of particles is shown on Fig.~\ref{fig:ICs}.
+In order to fit our simulation setup into the limited
+memory of some of the systems tested, we have randomly down-sampled the particle
+count of the output to $800^3=5.12\times10^8$, $600^3=2.16\times10^8$ and
+$376^3=5.1\times10^7$ particles with periodic boundary conditions 
+respectively. Scripts to generate these initial
+conditions are provided with the source code. We then run the \swift code for
+100 time-steps and average the wall clock time of these time-steps after having
+removed the first and last ones, where disk I/O occurs.
+
+\begin{figure}
+\centering
+\includegraphics[width=\columnwidth]{Figures/cosmoVolume}
+\caption{The initial density field computed from the initial particle
+  distribution used for our tests. The density $\rho_i$ of the particles spans 8
+  orders of magnitude, requiring smoothing lengths $h_i$ changing by a factor of
+  almost $1000$ across the simulation volume. \label{fig:ICs}}
+\end{figure}  
+
+On all the machines, the code was compiled out of the box,
+without any tuning, explicit vectorization, or exploiting any
+other specific features of the underlying hardware. 
+
+\subsection{x86 architecture: COSMA-5}
+
+For our first test, we ran \swift on the COSMA-5 DiRAC2 Data Centric
+System\footnote{\url{icc.dur.ac.uk/index.php?content=Computing/Cosma}}
+located at the University of Durham. The system consists of 420 nodes
+with 2 Intel Sandy Bridge-EP Xeon
+E5-2670\footnote{\url{http://ark.intel.com/products/64595/Intel-Xeon-Processor-E5-2670-20M-Cache-2_60-GHz-8_00-GTs-Intel-QPI}}
+CPUs clocked at $2.6~\rm{GHz}$ with each $128~\rm{GByte}$ of RAM. The
+16-core nodes are connected using a Mellanox FDR10 Infiniband 2:1 blocking
+configuration.
+
+This system is similar to many Tier-2 systems available in most universities or
+computing facilities. Demonstrating strong scaling on such a machine is
+essential to show that the code can be efficiently used even on the type of
+commodity hardware available to most researchers.
+
+The code was compiled with the Intel compiler version \textsc{2016.0.1} and
+linked to the Intel MPI library version \textsc{5.1.2.150} and METIS library
+version \textsc{5.1.0}.
+
+The simulation setup with $376^3$ particles was run on that system using 1 to
+256 threads on 1 to 16 nodes, the results of which are shown on
+Fig.~\ref{fig:cosma}. For this strong scaling test, we used one MPI rank per node and 16
+threads per node (i.e.~one thread per physical core). We also ran on one single
+node using up to 32 threads, i.e.~up to one thread per physical and
+virtual core. Fig.~\ref{fig:domains} shows the domain decomposition
+obtained via the task-graph decomposition algorithm described above for
+the 16 node run.
+
+\begin{figure}
+\centering
+\includegraphics[width=\columnwidth]{Figures/domains}
+\caption{The particles for the initial conditions shown on Fig.~\ref{fig:ICs}
+  colored according to the node they belong to after a load-balancing call on
+  32 nodes. As can be seen, the domain decomposition follows the cells in the mesh
+  but is not made of regular cuts. Domains have different shapes and
+  sizes. \label{fig:domains}}
+\end{figure}  
+
+
+\begin{figure*}
+\centering
+\includegraphics[width=\textwidth]{Figures/scalingCosma}
+\caption{Strong scaling test on the COSMA-5 machine (see text for hardware
+  description). \textit{Left panel:} Code Speed-up. \textit{Right panel:}
+  Corresponding parallel efficiency.  Using 16 threads per node (no use of
+  hyper-threading) with one MPI rank per node, a good parallel efficiency (60\%)
+  is achieved when increasing the thread count from 1 (1 node) to 128 (8 nodes)
+  even on this relatively small test case. The dashed line indicates the
+  efficiency when running on one single node but using all the physical and
+  virtual cores (hyper-threading). As these CPUs only have one FPU per core, we
+  see no benefit from hyper-threading.
+  \label{fig:cosma}}
+\end{figure*}
+
+
+
+\subsection{x86 architecture: SuperMUC}
+
+For our next test, we ran \swift on the SuperMUC x86 phase~1 thin
+nodes \footnote{\url{https://www.lrz.de/services/compute/supermuc/systemdescription/}}
+located at the Leibniz Supercomputing Center in Garching near Munich. This
+system consists of 9\,216 nodes with 2 Intel Sandy Bridge-EP Xeon E5-2680
+8C\footnote{\url{http://ark.intel.com/products/64583/Intel-Xeon-Processor-E5-2680-(20M-Cache-2_70-GHz-8_00-GTs-Intel-QPI)}}
+at $2.7~\rm{GHz}$ CPUS. Each 16-core node has $32~\rm{GByte}$ of RAM.
+The nodes are split in 18
+``islands'' of 512 nodes within which communications are handled via an
+Infiniband FDR10 non-blocking Tree. These islands are then connected using a 4:1
+Pruned Tree.
+
+This system is similar in nature to the COSMA-5 system used in the previous set
+of tests but is much larger, allowing us to test scalability at a much larger
+scale.
+
+The code was compiled with the Intel compiler version \textsc{2015.5.223} and
+linked to the Intel MPI library version \textsc{5.1.2.150} and METIS library
+version \textsc{5.0.2}.
+
+The simulation setup with $800^3$ particles was run using 16 to
+2048 nodes (4 islands) and the results of this strong scaling test are shown in
+Fig.~\ref{fig:superMUC}. For this test, we used one MPI rank per node and 16
+threads per node, i.e.~one thread per physical core.
+
+\begin{figure*}
+\centering
+\includegraphics[width=\textwidth]{Figures/scalingSuperMUC}
+\caption{Strong scaling test on the SuperMUC phase~1 machine (see text
+  for hardware description). \textit{Left panel:} Code
+  Speed-up. \textit{Right panel:} Corresponding parallel efficiency.
+  Using 16 threads per node (no use of hyper-threading) with one MPI rank
+  per node, an almost perfect parallel efficiency is achieved when
+  increasing the node count from 16 (256 cores) to 2\,048 (32\,768
+  cores).
+  \label{fig:superMUC}}
+\end{figure*}
+
+
+\subsection{Blue Gene architecture: JUQUEEN}
+
+For our last set of tests, we ran \swift on the JUQUEEN IBM Blue Gene/Q
+system\footnote{\url{http://www.fz-juelich.de/ias/jsc/EN/Expertise/Supercomputers/JUQUEEN/Configuration/Configuration_node.html}}
+located at the J\"ulich Supercomputing Center. This system consists of
+28\,672 nodes with an IBM PowerPC A2 processor running at
+$1.6~\rm{GHz}$ and $16~\rm{GByte}$ of RAM each. Of notable interest
+is the presence of two floating units per compute core. The system is
+composed of 28 racks containing each 1\,024 nodes. The network uses a
+5D torus to link all the racks.
+
+This system is larger than the SuperMUC supercomputer described above and
+uses a completely different processor and instruction set.
+We use it here to demonstrate that our results are not dependant
+on the hardware being used.
+
+The code was compiled with the IBM XL compiler version \textsc{30.73.0.13} and
+linked to the corresponding MPI and METIS library
+versions \textsc{4.0.2}.
+
+The simulation setup with $600^3$ particles was first run using
+512 nodes with one MPI rank per node and varying only the number of threads per
+node. The results of this test are shown in Fig.~\ref{fig:JUQUEEN1}.
+
+We later repeated the test, this time varying the number of nodes from 32 to
+8192 (8 racks).  For this test, we used one MPI rank per node and 32 threads per
+node, i.e.~two threads per physical core. The results of this strong scaling
+test are shown in Fig.~\ref{fig:JUQUEEN2}.
+
+
+\begin{figure}
+\centering
+\includegraphics[width=\columnwidth]{Figures/scalingInNode}
+\caption{Strong scaling test of the hybrid component of the code. The
+  same calculation is performed on 512 node of the JUQUEEN Blue Gene
+  supercomputer (see text for hardware description) using a single MPI
+  rank per node and varying only the number of
+  threads per node. The code displays excellent scaling even when all the cores and
+  hardware multi-threads are in use. \label{fig:JUQUEEN1}}
+\end{figure}  
+
+
+
+\begin{figure*}
+\centering
+\includegraphics[width=\textwidth]{Figures/scalingBlueGene}
+\caption{Strong scaling test on the JUQUEEN Blue Gene machine (see text
+  for hardware description). \textit{Left panel:} Code
+  Speed-up. \textit{Right panel:} Corresponding parallel efficiency.
+  Using 32 threads per node (2 per physical core) with one MPI rank
+  per node, a parallel efficiency of more than $60\%$ is achieved when
+  increasing the node count from 32 (512 cores) to 8\,192 (131\,072
+  cores). On 8\,192 nodes there are fewer than 27\,000 particles per
+  node and only a few hundred tasks, making the whole problem
+  extremely hard to load-balance effectively.
+  \label{fig:JUQUEEN2}}
+\end{figure*}
+
+
+
+
+
+%#####################################################################################################
+
+\section{Discussion \& conclusions}
+
+The strong scaling results presented in the previous sections on
+three different machines demonstrate the ability of our framework
+to scale on both small commodity
+machines, thanks to the use of task-based parallelism at the node level, and on
+the largest machines (Tier-0 systems) currently available, thanks to the
+task-based domain distribution and asynchronous communication schemes.
+We would like to emphasize that these results were obtained for a
+realistic test case without any micro-level optimization or explicit
+vectorization.
+
+Excellent strong scaling is also achieved when increasing the number of threads
+per node (i.e.~per MPI rank, see fig.~\ref{fig:JUQUEEN1}), demonstrating that
+the description of MPI (asynchronous) communications as tasks within our
+framework is not a bottleneck. One common conception in HPC is that the number
+of MPI communications between nodes should be kept to a minimum to optimize the
+efficiency of the calculation. Our approach does exactly the opposite with large
+number of point-to-point communications between pairs of nodes occurring over the
+course of a time-step. For example, on the SuperMUC machine with 32 nodes (512
+cores), each MPI rank contains approximately $1.6\times10^7$ particles in
+$2.5\times10^5$ cells. \swift will generate around $58\,000$ point-to-point
+asynchronous MPI communications (a pair of \texttt{send} and \texttt{recv} tasks)
+{\em per node} and {\em per timestep}. Such an insane number of messages is
+discouraged by most practitioners.
+Dispatching communications
+over the course of the calculation and not in short bursts, as is commonly done,
+may also help lower the load on the network.
+
+One time-step on $8\,192$ nodes of the JUQUEEN machine takes $63~\rm{ms}$ of
+wall-clock time. All the loading of the tasks, communications and running of the
+tasks takes place in that short amount of time. Our framework can therefore
+load-balance a calculation over $2.6\times10^5$ threads with remarkable
+efficiency.
+
+We emphasize, as was previously demonstrated in \cite{ref:Gonnet2015}, that \swift
+is also much faster than the \gadget code \cite{Springel2005}, the
+\emph{de-facto} standard in the field of particle-based cosmological
+simulations. The simulation setup that was run on the COSMA-5
+system takes $2.9~\rm{s}$ of wall-clock time per time-step on $256$ cores using
+\swift whilst the default \gadget code on exactly the same setup with the same
+number of cores requires $32~\rm{s}$.
+The excellent scaling
+performance of \swift allows us to push this number further by simply increasing
+the number of cores, whilst \gadget reaches its peak speed (for this problem) at
+around 300 cores and stops scaling beyond that. This unprecedented scaling
+ability combined with future work on vectorization of the calculations within
+each task will hopefully make \swift an important tool for future simulations in
+cosmology and help push the entire field to a new level.
+
+\swift, its documentation, and the test cases presented in this paper are all
+available at the address \web.
+
+
+%#####################################################################################################
+
+\section{Acknowledgements}
+This work would not have been possible without Lydia Heck's help and
+expertise. We acknowledge the help of Tom Theuns, James Willis, Bert
+Vandenbroucke, Angus Lepper and other contributors to the \swift
+code. \\ We thank Heinrich Bockhorst and Stephen Blair-Chappell from {\sc
+  intel} as well as Dirk Brommel from the J\"ulich Computing Center
+and Nikolay J. Hammer from the Leibniz Rechnenzentrum for their help
+at various stages of this project.\\ This work used the DiRAC Data
+Centric system at Durham University, operated by the Institute for
+Computational Cosmology on behalf of the STFC DiRAC HPC Facility
+(\url{www.dirac.ac.uk}). This equipment was funded by BIS National
+E-infrastructure capital grant ST/K00042X/1, STFC capital grant
+ST/H008519/1, and STFC DiRAC Operations grant ST/K003267/1 and Durham
+University. DiRAC is part of the National E-Infrastructure. This work
+was supported by the Science and Technology Facilities Council
+ST/F001166/1 and the European Research Council under the European
+Union's ERC Grant agreements 267291 ``Cosmiway'', and by {\sc intel}
+through establishment of the ICC as an {\sc intel} parallel computing
+centre (IPCC).
+
+\nocite{*}
+\bibliographystyle{abbrv}
+\bibliography{biblio}
+
+
+\end{document}
diff --git a/theory/paper_pasc/sig-alternate-05-2015.cls b/theory/paper_pasc/sig-alternate-05-2015.cls
new file mode 100644
index 0000000000000000000000000000000000000000..b922ec29955e93ac892c369320a5accdddbc15a4
--- /dev/null
+++ b/theory/paper_pasc/sig-alternate-05-2015.cls
@@ -0,0 +1,1893 @@
+% SIG-ALTERNATE.CLS - VERSION 2.8
+% "COMPATIBLE" WITH THE "ACM_PROC_ARTICLE-SP.CLS" V3.2SP
+% Gerald Murray - May 23rd 2012
+% Boris Veytsman - April 23 2013
+% Boris Veytsman - May 12 2013
+% Boris Veytsman - June 09 2013
+% Boris Veytsman - August 12 2013
+%
+% ---- Start of 'updates'  ----
+% Added new permission/copyright statement - BV
+% Changed $10 fee to $15 -- May 2012  --  Gerry
+% Changed $5 fee to $10 --  April 2009 -- Gerry
+% April 22nd. 2009 - Fixed 'Natbib' incompatibility problem - Gerry
+% April 22nd. 2009 - Fixed 'Babel' incompatibility problem - Gerry
+% April 22nd. 2009 - Inserted various bug-fixes and improvements - Gerry
+%
+% To produce Type 1 fonts in the document plus allow for 'normal LaTeX accenting' in the critical areas;
+% title, author block, section-heads, confname, etc. etc. 
+% i.e. the whole purpose of this version update is to NOT resort to 'inelegant accent patches'.
+% After much research, three extra .sty packages were added to the the tail (ae, aecompl, aeguill) to solve,
+% in particular, the accenting problem(s). We _could_ ask authors (via instructions/sample file) to 'include' these in
+% the source .tex file - in the preamble - but if everything is already provided ('behind the scenes' - embedded IN the .cls)
+% then this is less work for authors and also makes everything appear 'vanilla'.
+% NOTE: all 'patchwork accenting" has been commented out (here) and is no longer 'used' in the sample .tex file (either).
+% Gerry June 2007
+%
+% Patch for accenting in conference name/location. Gerry May 3rd. 2007
+% Rule widths changed to .5, author count (>6) fixed, roll-back for Type 3 problem. Gerry March 20th. 2007
+% Changes made to 'modernize' the fontnames but esp. for MikTeX users V2.4/2.5 - Nov. 30th. 2006
+% Updated the \email definition to allow for its use inside of 'shared affiliations' - Nov. 30th. 2006
+% Fixed the 'section number depth value' - Nov. 30th. 2006
+%
+% Footnotes inside table cells using \minipage (Oct. 2002)
+% Georgia fixed bug in sub-sub-section numbering in paragraphs (July 29th. 2002)
+% JS/GM fix to vertical spacing before Proofs (July 30th. 2002)
+%
+% Made the Permission Statement / Conference Info / Copyright Info
+% 'user definable' in the source .tex file OR automatic if
+% not specified.
+%
+% Allowance made to switch default fonts between those systems using
+% normal/modern font names and those using 'Type 1' or 'Truetype' fonts.
+% See LINE NUMBER 255 for details.
+% Also provided for enumerated/annotated Corollaries 'surrounded' by
+% enumerated Theorems (line 848).
+% Gerry November 11th. 1999
+%
+% ---- End of 'updates' ----
+%
+\def\fileversion{v2.9}          % for ACM's tracking purposes
+\def\filedate{August 12, 2013}    % Gerry Murray's tracking data
+\def\docdate {\filedate}
+\usepackage{epsfig}
+\usepackage{amssymb}
+\usepackage{amsmath}
+\usepackage{amsfonts}
+% Need this for accents in Arial/Helvetica
+%\usepackage[T1]{fontenc}  % Gerry March 12, 2007 - causes Type 3 problems (body text)
+%\usepackage{textcomp}
+%
+% SIG-ALTERNATE DOCUMENT STYLE
+% G.K.M. Tobin August-October 1999
+%    adapted from ARTICLE document style by Ken Traub, Olin Shivers
+%    also using elements of esub2acm.cls
+% HEAVILY MODIFIED, SUBSEQUENTLY, BY GERRY MURRAY 2000
+% ARTICLE DOCUMENT STYLE -- Released 16 March 1988
+%    for LaTeX version 2.09
+% Copyright (C) 1988 by Leslie Lamport
+%
+%
+%%% sig-alternate.cls is an 'ALTERNATE' document style for producing
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+%%% THIS FILE DOES NOT STRICTLY ADHERE TO THE SIGS (BOARD-ENDORSED)
+%%% PROCEEDINGS STYLE. It has been designed to produce a 'tighter'
+%%% paper in response to concerns over page budgets.
+%%% The main features of this style are:
+%%%
+%%% 1)  Two columns.
+%%% 2)  Side and top margins of 4.5pc, bottom margin of 6pc, column gutter of
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+%%% 3)  First page has title information, and an extra 6pc of space at the
+%%%     bottom of the first column for the ACM copyright notice.
+%%% 4)  Text is 9pt on 10pt baselines; titles (except main) are 9pt bold.
+%%%
+%%%
+%%% There are a few restrictions you must observe:
+%%%
+%%% 1)  You cannot change the font size; ACM wants you to use 9pt.
+%%% 3)  You must start your paper with the \maketitle command.  Prior to the
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+%%% 5)  The `figure' environment will produce a figure one column wide; if you
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+%%%
+%
+%%% Copyright Space:
+%%% This style automatically reserves 1" blank space at the bottom of page 1/
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+%%%
+%%% A typical usage looks like this:
+%%%     \toappear{To appear in the Ninth AES Conference on Medievil Lithuanian
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+%%% This will be included in the preprint, and left out of the conference
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+%%%
+%%% WARNING:
+%%% Some dvi-ps converters heuristically allow chars to drift from their
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+%%% bold font used for section headers.
+%%% You may turn this hackery off via the -e option:
+%%%     dvips -e 0 foo.dvi >foo.ps
+%%%
+\typeout{Document Class 'sig-alternate' <9th June '13>.  Modified by
+  G.K.M. Tobin/Gerry Murray/Boris Veytsman}
+\typeout{Based in part upon document Style `acmconf' <22 May 89>. Hacked 4/91 by}
+\typeout{shivers@cs.cmu.edu, 4/93 by theobald@cs.mcgill.ca}
+\typeout{Excerpts were taken from (Journal Style) 'esub2acm.cls'.}
+\typeout{****** Bugs/comments/suggestions/technicalities to Gerry Murray -- murray@hq.acm.org ******}
+\typeout{Questions on the style, SIGS policies, etc. to Adrienne Griscti griscti@acm.org}
+
+% New option code by BV
+
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+\newcommand\printccsdesc{%
+  \ifx\@concepts\@empty\else
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+
+\@lowpenalty   51       % Produced by \nopagebreak[1] or \nolinebreak[1]
+\@medpenalty  151       % Produced by \nopagebreak[2] or \nolinebreak[2]
+\@highpenalty 301       % Produced by \nopagebreak[3] or \nolinebreak[3]
+
+\@beginparpenalty -\@lowpenalty % Before a list or paragraph environment.
+\@endparpenalty   -\@lowpenalty % After a list or paragraph environment.
+\@itempenalty     -\@lowpenalty % Between list items.
+
+
+\RequirePackage{ifpdf}%
+\ifpdf
+\pdfpagewidth=8.5in
+\pdfpageheight=11in
+\fi
+
+
+\lineskip 2pt           % \lineskip is 1pt for all font sizes.
+\normallineskip 2pt
+\def\baselinestretch{1}
+
+
+\ifnum\ACM@basesize=9\relax
+\abovedisplayskip 9pt plus2pt minus4.5pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip  \z@ plus3pt%
+\belowdisplayshortskip  5.4pt plus3pt minus3pt%
+\let\@listi\@listI     % Setting of \@listi added 9 Jun 87
+
+\def\small{\@setsize\small{9pt}\viiipt\@viiipt
+\abovedisplayskip 7.6pt plus 3pt minus 4pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip \z@ plus2pt%
+\belowdisplayshortskip 3.6pt plus2pt minus 2pt
+\def\@listi{\leftmargin\leftmargini %% Added 22 Dec 87
+\topsep 4pt plus 2pt minus 2pt\parsep 2pt plus 1pt minus 1pt
+\itemsep \parsep}}
+
+\def\footnotesize{\@setsize\footnotesize{9pt}\ixpt\@ixpt
+\abovedisplayskip 6.4pt plus 2pt minus 4pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip \z@ plus 1pt%
+\belowdisplayshortskip 2.7pt plus 1pt minus 2pt
+\def\@listi{\leftmargin\leftmargini %% Added 22 Dec 87
+\topsep 3pt plus 1pt minus 1pt\parsep 2pt plus 1pt minus 1pt
+\itemsep \parsep}}
+\fi
+
+\ifnum\ACM@basesize=10\relax
+\abovedisplayskip 10pt plus2pt minus4.5pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip  \z@ plus3pt%
+\belowdisplayshortskip  6pt plus3pt minus3pt%
+\let\@listi\@listI     % Setting of \@listi added 9 Jun 87
+
+\def\small{\@setsize\small{10pt}\ixpt\@ixpt
+\abovedisplayskip 8.5pt plus 3pt minus 4pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip \z@ plus2pt%
+\belowdisplayshortskip 4pt plus2pt minus 2pt
+\def\@listi{\leftmargin\leftmargini %% Added 22 Dec 87
+\topsep 4.5pt plus 2pt minus 2pt\parsep 2pt plus 1pt minus 1pt
+\itemsep \parsep}}
+
+\def\footnotesize{\@setsize\footnotesize{10pt}\xpt\@xpt
+\abovedisplayskip 7.6pt plus 2pt minus 4pt%
+\belowdisplayskip \abovedisplayskip
+\abovedisplayshortskip \z@ plus 1pt%
+\belowdisplayshortskip 3.0pt plus 1pt minus 2pt
+\def\@listi{\leftmargin\leftmargini %% Added 22 Dec 87
+\topsep 3.2pt plus 1pt minus 1pt\parsep 2pt plus 1pt minus 1pt
+\itemsep \parsep}}
+\fi
+
+
+\newcount\aucount
+\newcount\originalaucount
+\newdimen\auwidth
+\auwidth=\textwidth
+\newdimen\auskip
+\newcount\auskipcount
+\newdimen\auskip
+\global\auskip=1pc
+\newdimen\allauboxes
+\allauboxes=\auwidth
+\newtoks\addauthors
+\newcount\addauflag
+\global\addauflag=0 %Haven't shown additional authors yet
+
+\newtoks\subtitletext
+\gdef\subtitle#1{\subtitletext={#1}}
+
+\gdef\additionalauthors#1{\addauthors={#1}}
+
+\gdef\numberofauthors#1{\global\aucount=#1
+\ifnum\aucount>3\global\originalaucount=\aucount \global\aucount=3\fi %g}  % 3 OK - Gerry March 2007
+\global\auskipcount=\aucount\global\advance\auskipcount by 1
+\global\multiply\auskipcount by 2
+\global\multiply\auskip by \auskipcount
+\global\advance\auwidth by -\auskip
+\global\divide\auwidth by \aucount}
+
+% \and was modified to count the number of authors.  GKMT 12 Aug 1999
+\def\alignauthor{%                  % \begin{tabular}
+\end{tabular}%
+  \begin{tabular}[t]{p{\auwidth}}\centering}%
+
+%  *** NOTE *** NOTE *** NOTE *** NOTE ***
+%  If you have 'font problems' then you may need
+%  to change these, e.g. 'arialb' instead of "arialbd".
+%  Gerry Murray 11/11/1999
+%  *** OR ** comment out block A and activate block B or vice versa.
+% **********************************************
+%
+%  -- Start of block A -- (Type 1 or Truetype fonts)
+%\newfont{\secfnt}{timesbd at 12pt} % was timenrb originally - now is timesbd
+%\newfont{\secit}{timesbi at 12pt}   %13 Jan 00 gkmt
+%\newfont{\subsecfnt}{timesi at 11pt} % was timenrri originally - now is timesi
+%\newfont{\subsecit}{timesbi at 11pt} % 13 Jan 00 gkmt -- was times changed to timesbi gm 2/4/2000
+%                         % because "normal" is italic, "italic" is Roman
+%\newfont{\ttlfnt}{arialbd at 18pt} % was arialb originally - now is arialbd
+%\newfont{\ttlit}{arialbi at 18pt}    % 13 Jan 00 gkmt
+%\newfont{\subttlfnt}{arial at 14pt} % was arialr originally - now is arial
+%\newfont{\subttlit}{ariali at 14pt} % 13 Jan 00 gkmt
+%\newfont{\subttlbf}{arialbd at 14pt}  % 13 Jan 00 gkmt
+%\newfont{\aufnt}{arial at 12pt} % was arialr originally - now is arial
+%\newfont{\auit}{ariali at 12pt} % 13 Jan 00 gkmt
+%\newfont{\affaddr}{arial at 10pt} % was arialr originally - now is arial
+%\newfont{\affaddrit}{ariali at 10pt} %13 Jan 00 gkmt
+%\newfont{\eaddfnt}{arial at 12pt} % was arialr originally - now is arial
+%\newfont{\ixpt}{times at 9pt} % was timenrr originally - now is times
+%\newfont{\confname}{timesi at 8pt} % was timenrri - now is timesi
+%\newfont{\crnotice}{times at 8pt} % was timenrr originally - now is times
+%\newfont{\ninept}{times at 9pt} % was timenrr originally - now is times
+
+% *********************************************
+%  -- End of block A --
+%
+%
+% -- Start of block B -- UPDATED FONT NAMES
+% *********************************************
+% Gerry Murray 11/30/2006
+% *********************************************
+\ifnum\ACM@basesize=9\relax
+\newfont{\secfnt}{ptmb8t at 12pt}
+\newfont{\secit}{ptmbi8t at 12pt}    %13 Jan 00 gkmt
+\newfont{\subsecfnt}{ptmri8t at 11pt}
+\newfont{\subsecit}{ptmbi8t at 11pt}  % 
+\newfont{\ttlfnt}{phvb8t at 18pt}
+\newfont{\ttlit}{phvbo8t at 18pt}    % GM 2/4/2000
+\newfont{\subttlfnt}{phvr8t at 14pt}
+\newfont{\subttlit}{phvro8t at 14pt} % GM 2/4/2000
+\newfont{\subttlbf}{phvb8t at 14pt}  % 13 Jan 00 gkmt
+\newfont{\aufnt}{phvr8t at 12pt}
+\newfont{\auit}{phvro8t at 12pt}     % GM 2/4/2000
+\newfont{\affaddr}{phvr8t at 10pt}
+\newfont{\affaddrit}{phvro8t at 10pt} % GM 2/4/2000
+\newfont{\eaddfnt}{phvr8t at 12pt}
+\newfont{\ixpt}{ptmr8t at 9pt}
+\newfont{\confname}{ptmri8t at 8pt}
+\newfont{\crnotice}{ptmr8t at 8pt}
+\newfont{\ninept}{ptmr8t at 9pt}
+\fi
+\ifnum\ACM@basesize=10\relax
+\newfont{\secfnt}{ptmb8t at 13pt}
+\newfont{\secit}{ptmbi8t at 13pt}    %13 Jan 00 gkmt
+\newfont{\subsecfnt}{ptmri8t at 12pt}
+\newfont{\subsecit}{ptmbi8t at 12pt}  % 
+\newfont{\ttlfnt}{phvb8t at 20pt}
+\newfont{\ttlit}{phvbo8t at 20pt}    % GM 2/4/2000
+\newfont{\subttlfnt}{phvr8t at 15pt}
+\newfont{\subttlit}{phvro8t at 15pt} % GM 2/4/2000
+\newfont{\subttlbf}{phvb8t at 15pt}  % 13 Jan 00 gkmt
+\newfont{\aufnt}{phvr8t at 12pt}
+\newfont{\auit}{phvro8t at 12pt}     % GM 2/4/2000
+\newfont{\affaddr}{phvr8t at 11pt}
+\newfont{\affaddrit}{phvro8t at 11pt} % GM 2/4/2000
+\newfont{\eaddfnt}{phvr8t at 12pt}
+\newfont{\ixpt}{ptmr8t at 10pt}
+\newfont{\confname}{ptmri8t at 9pt}
+\newfont{\crnotice}{ptmr8t at 9pt}
+\newfont{\ninept}{ptmr8t at 10pt}
+\fi
+% +++++++++++++++++++++++++++++++++++++++++++++
+% -- End of block B --
+
+%\def\email#1{{{\eaddfnt{\vskip 4pt#1}}}}
+% If we have an email, inside a "shared affiliation" then we need the following instead
+\def\email#1{{{\eaddfnt{\par #1}}}}       % revised  - GM - 11/30/2006
+
+\def\addauthorsection{\ifnum\originalaucount>6  % was 3 - Gerry March 2007
+    \section{Additional Authors}\the\addauthors
+  \fi}
+
+\newcount\savesection
+\newcount\sectioncntr
+\global\sectioncntr=1
+
+\setcounter{secnumdepth}{3}
+
+\def\appendix{\par
+\section*{APPENDIX}
+\setcounter{section}{0}
+ \setcounter{subsection}{0}
+ \def\thesection{\Alph{section}} }
+
+\leftmargini 22.5pt
+\leftmarginii 19.8pt    % > \labelsep + width of '(m)'
+\leftmarginiii 16.8pt   % > \labelsep + width of 'vii.'
+\leftmarginiv 15.3pt    % > \labelsep + width of 'M.'
+\leftmarginv 9pt
+\leftmarginvi 9pt
+
+\leftmargin\leftmargini
+\labelsep 4.5pt
+\labelwidth\leftmargini\advance\labelwidth-\labelsep
+
+\def\@listI{\leftmargin\leftmargini \parsep 3.6pt plus 2pt minus 1pt%
+\topsep 7.2pt plus 2pt minus 4pt%
+\itemsep 3.6pt plus 2pt minus 1pt}
+
+\let\@listi\@listI
+\@listi
+
+\def\@listii{\leftmargin\leftmarginii
+   \labelwidth\leftmarginii\advance\labelwidth-\labelsep
+   \topsep 3.6pt plus 2pt minus 1pt
+   \parsep 1.8pt plus 0.9pt minus 0.9pt
+   \itemsep \parsep}
+
+\def\@listiii{\leftmargin\leftmarginiii
+    \labelwidth\leftmarginiii\advance\labelwidth-\labelsep
+    \topsep 1.8pt plus 0.9pt minus 0.9pt
+    \parsep \z@ \partopsep 1pt plus 0pt minus 1pt
+    \itemsep \topsep}
+
+\def\@listiv{\leftmargin\leftmarginiv
+     \labelwidth\leftmarginiv\advance\labelwidth-\labelsep}
+
+\def\@listv{\leftmargin\leftmarginv
+     \labelwidth\leftmarginv\advance\labelwidth-\labelsep}
+
+\def\@listvi{\leftmargin\leftmarginvi
+     \labelwidth\leftmarginvi\advance\labelwidth-\labelsep}
+
+\def\labelenumi{\theenumi.}
+\def\theenumi{\arabic{enumi}}
+
+\def\labelenumii{(\theenumii)}
+\def\theenumii{\alph{enumii}}
+\def\p@enumii{\theenumi}
+
+\def\labelenumiii{\theenumiii.}
+\def\theenumiii{\roman{enumiii}}
+\def\p@enumiii{\theenumi(\theenumii)}
+
+\def\labelenumiv{\theenumiv.}
+\def\theenumiv{\Alph{enumiv}}
+\def\p@enumiv{\p@enumiii\theenumiii}
+
+\def\labelitemi{$\bullet$}
+\def\labelitemii{\bf --}
+\def\labelitemiii{$\ast$}
+\def\labelitemiv{$\cdot$}
+
+\def\verse{\let\\=\@centercr
+  \list{}{\itemsep\z@ \itemindent -1.5em\listparindent \itemindent
+          \rightmargin\leftmargin\advance\leftmargin 1.5em}\item[]}
+\let\endverse\endlist
+
+\def\quotation{\list{}{\listparindent 1.5em
+    \itemindent\listparindent
+    \rightmargin\leftmargin \parsep 0pt plus 1pt}\item[]}
+\let\endquotation=\endlist
+
+\def\quote{\list{}{\rightmargin\leftmargin}\item[]}
+\let\endquote=\endlist
+
+\def\descriptionlabel#1{\hspace\labelsep \bf #1}
+\def\description{\list{}{\labelwidth\z@ \itemindent-\leftmargin
+       \let\makelabel\descriptionlabel}}
+
+\let\enddescription\endlist
+
+\def\theequation{\arabic{equation}}
+
+
+\ifnum\ACM@basesize=9\relax
+\arraycolsep 4.5pt   % Half the space between columns in an array environment.
+\tabcolsep 5.4pt    % Half the space between columns in a tabular environment.
+\arrayrulewidth .5pt % Width of rules in array and tabular environment. % (was .4) updated Gerry March 20 2007
+\doublerulesep 1.8pt % Space between adjacent rules in array or tabular env.
+
+\fi
+
+\ifnum\ACM@basesize=10\relax
+\arraycolsep 5pt   % Half the space between columns in an array environment.
+\tabcolsep 6pt    % Half the space between columns in a tabular environment.
+\arrayrulewidth .5pt % Width of rules in array and tabular environment. % (was .4) updated Gerry March 20 2007
+\doublerulesep 1.8pt % Space between adjacent rules in array or tabular env.
+
+\fi
+
+\tabbingsep \labelsep   % Space used by the \' command.  (See LaTeX manual.)
+
+\skip\@mpfootins =\skip\footins
+
+\fboxsep =2.7pt      % Space left between box and text by \fbox and \framebox.
+\fboxrule =.5pt      % Width of rules in box made by \fbox and \framebox. % (was .4) updated Gerry March 20 2007
+
+\def\thepart{\Roman{part}} % Roman numeral part numbers.
+\def\thesection       {\arabic{section}}
+\def\thesubsection    {\thesection.\arabic{subsection}}
+%\def\thesubsubsection {\thesubsection.\arabic{subsubsection}} % GM 7/30/2002
+%\def\theparagraph     {\thesubsubsection.\arabic{paragraph}}  % GM 7/30/2002
+\def\thesubparagraph  {\theparagraph.\arabic{subparagraph}}
+
+\def\@pnumwidth{1.55em}
+\def\@tocrmarg {2.55em}
+\def\@dotsep{4.5}
+\setcounter{tocdepth}{3}
+
+%\def\tableofcontents{\@latexerr{\tableofcontents: Tables of contents are not
+%  allowed in the `acmconf' document style.}\@eha}
+
+\def\tableofcontents{\ClassError{%
+    \string\tableofcontents\space is not allowed in the `acmconf' document	% January 2008
+    style}\@eha}
+
+\def\l@part#1#2{\addpenalty{\@secpenalty}
+   \addvspace{2.25em plus 1pt}  % space above part line
+   \begingroup
+   \@tempdima 3em       % width of box holding part number, used by
+     \parindent \z@ \rightskip \@pnumwidth      %% \numberline
+     \parfillskip -\@pnumwidth
+     {\large \bf        % set line in \large boldface
+     \leavevmode        % TeX command to enter horizontal mode.
+     #1\hfil \hbox to\@pnumwidth{\hss #2}}\par
+     \nobreak           % Never break after part entry
+   \endgroup}
+
+\def\l@section#1#2{\addpenalty{\@secpenalty} % good place for page break
+   \addvspace{1.0em plus 1pt}   % space above toc entry
+   \@tempdima 1.5em             % width of box holding section number
+   \begingroup
+    \parindent  \z@ \rightskip \@pnumwidth
+     \parfillskip -\@pnumwidth
+     \bf                        % Boldface.
+     \leavevmode                % TeX command to enter horizontal mode.
+      \advance\leftskip\@tempdima %% added 5 Feb 88 to conform to
+      \hskip -\leftskip           %% 25 Jan 88 change to \numberline
+     #1\nobreak\hfil \nobreak\hbox to\@pnumwidth{\hss #2}\par
+   \endgroup}
+
+
+\def\l@subsection{\@dottedtocline{2}{1.5em}{2.3em}}
+\def\l@subsubsection{\@dottedtocline{3}{3.8em}{3.2em}}
+\def\l@paragraph{\@dottedtocline{4}{7.0em}{4.1em}}
+\def\l@subparagraph{\@dottedtocline{5}{10em}{5em}}
+
+%\def\listoffigures{\@latexerr{\listoffigures: Lists of figures are not
+%  allowed in the `acmconf' document style.}\@eha}
+
+\def\listoffigures{\ClassError{%
+    \string\listoffigures\space is not allowed in the `acmconf' document	% January 2008
+    style}\@eha}
+
+\def\l@figure{\@dottedtocline{1}{1.5em}{2.3em}}
+
+%\def\listoftables{\@latexerr{\listoftables: Lists of tables are not
+%  allowed in the `acmconf' document style.}\@eha}
+%\let\l@table\l@figure
+
+\def\listoftables{\ClassError{%
+    \string\listoftables\space is not allowed in the `acmconf' document		% January 2008
+    style}\@eha}
+ \let\l@table\l@figure
+
+\def\footnoterule{\kern-3\p@
+  \hrule width .5\columnwidth   % (was .4) updated Gerry March 20 2007
+  \kern 2.6\p@}                 % The \hrule has default height of .4pt % (was .4) updated Gerry March 20 2007
+% ------
+\long\def\@makefntext#1{\noindent 
+%\hbox to .5em{\hss$^{\@thefnmark}$}#1}   % original
+\hbox to .5em{\hss\textsuperscript{\@thefnmark}}#1}  % C. Clifton / GM Oct. 2nd. 2002
+% -------
+
+\long\def\@maketntext#1{\noindent
+#1}
+
+\long\def\@maketitlenotetext#1#2{\noindent
+            \hbox to 1.8em{\hss$^{#1}$}#2}
+
+\setcounter{topnumber}{2}
+\def\topfraction{.7}
+\setcounter{bottomnumber}{1}
+\def\bottomfraction{.3}
+\setcounter{totalnumber}{3}
+\def\textfraction{.2}
+\def\floatpagefraction{.5}
+\setcounter{dbltopnumber}{2}
+\def\dbltopfraction{.7}
+\def\dblfloatpagefraction{.5}
+
+%
+\long\def\@makecaption#1#2{
+   \vskip \baselineskip
+   \setbox\@tempboxa\hbox{\textbf{#1: #2}}
+   \ifdim \wd\@tempboxa >\hsize % IF longer than one line:
+       \textbf{#1: #2}\par               %   THEN set as ordinary paragraph.
+     \else                      %   ELSE  center.
+       \hbox to\hsize{\hfil\box\@tempboxa\hfil}\par
+   \fi}
+
+%
+
+\long\def\@makecaption#1#2{
+   \vskip 10pt
+   \setbox\@tempboxa\hbox{\textbf{#1: #2}}
+   \ifdim \wd\@tempboxa >\hsize % IF longer than one line:
+       \textbf{#1: #2}\par                %   THEN set as ordinary paragraph.
+     \else                      %   ELSE  center.
+       \hbox to\hsize{\hfil\box\@tempboxa\hfil}
+   \fi}
+
+\@ifundefined{figure}{\newcounter {figure}} % this is for LaTeX2e
+
+\def\fps@figure{tbp}
+\def\ftype@figure{1}
+\def\ext@figure{lof}
+\def\fnum@figure{Figure \thefigure}
+\def\figure{\@float{figure}}
+%\let\endfigure\end@float
+\def\endfigure{\end@float} 		% Gerry January 2008
+\@namedef{figure*}{\@dblfloat{figure}}
+\@namedef{endfigure*}{\end@dblfloat}
+
+\@ifundefined{table}{\newcounter {table}} % this is for LaTeX2e
+
+\def\fps@table{tbp}
+\def\ftype@table{2}
+\def\ext@table{lot}
+\def\fnum@table{Table \thetable}
+\def\table{\@float{table}}
+%\let\endtable\end@float
+\def\endtable{\end@float}		% Gerry January 2008
+\@namedef{table*}{\@dblfloat{table}}
+\@namedef{endtable*}{\end@dblfloat}
+
+\newtoks\titleboxnotes
+\newcount\titleboxnoteflag
+
+\def\maketitle{\par
+ \begingroup
+   \def\thefootnote{\fnsymbol{footnote}}
+   \def\@makefnmark{\hbox
+       to 0pt{$^{\@thefnmark}$\hss}}
+     \twocolumn[\@maketitle]
+\@thanks
+ \endgroup
+ \setcounter{footnote}{0}
+ \let\maketitle\relax
+ \let\@maketitle\relax
+ \gdef\@thanks{}\gdef\@author{}\gdef\@title{}\gdef\@subtitle{}\let\thanks\relax
+ \@copyrightspace}
+
+%% CHANGES ON NEXT LINES
+\newif\if@ll % to record which version of LaTeX is in use
+
+\expandafter\ifx\csname LaTeXe\endcsname\relax % LaTeX2.09 is used
+\else% LaTeX2e is used, so set ll to true
+\global\@lltrue
+\fi
+
+\if@ll
+  \NeedsTeXFormat{LaTeX2e}
+  \ProvidesClass{sig-alternate} [2013/05/12 v2.7 based on acmproc.cls V1.3 <Nov. 30 '99>]
+  \RequirePackage{latexsym}% QUERY: are these two really needed?
+  \let\dooptions\ProcessOptions
+\else
+  \let\dooptions\@options
+\fi
+%% END CHANGES
+
+\def\@height{height}
+\def\@width{width}
+\def\@minus{minus}
+\def\@plus{plus}
+\def\hb@xt@{\hbox to}
+\newif\if@faircopy
+\@faircopyfalse
+\def\ds@faircopy{\@faircopytrue}
+
+\def\ds@preprint{\@faircopyfalse}
+
+\@twosidetrue
+\@mparswitchtrue
+\def\ds@draft{\overfullrule 5\p@}
+%% CHANGE ON NEXT LINE
+\dooptions
+
+\lineskip \p@
+\normallineskip \p@
+\def\baselinestretch{1}
+\def\@ptsize{0} %needed for amssymbols.sty
+
+%% CHANGES ON NEXT LINES
+\if@ll% allow use of old-style font change commands in LaTeX2e
+\@maxdepth\maxdepth
+%
+\DeclareOldFontCommand{\rm}{\ninept\rmfamily}{\mathrm}
+\DeclareOldFontCommand{\sf}{\normalfont\sffamily}{\mathsf}
+\DeclareOldFontCommand{\tt}{\normalfont\ttfamily}{\mathtt}
+\DeclareOldFontCommand{\bf}{\normalfont\bfseries}{\mathbf}
+\DeclareOldFontCommand{\it}{\normalfont\itshape}{\mathit}
+\DeclareOldFontCommand{\sl}{\normalfont\slshape}{\@nomath\sl}
+\DeclareOldFontCommand{\sc}{\normalfont\scshape}{\@nomath\sc}
+\DeclareRobustCommand*{\cal}{\@fontswitch{\relax}{\mathcal}}
+\DeclareRobustCommand*{\mit}{\@fontswitch{\relax}{\mathnormal}}
+\fi
+%
+\if@ll
+ \renewcommand{\rmdefault}{cmr}  % was 'ttm'
+% Note! I have also found 'mvr' to work ESPECIALLY well.
+% Gerry - October 1999
+% You may need to change your LV1times.fd file so that sc is
+% mapped to cmcsc - -for smallcaps -- that is if you decide
+% to change {cmr} to {times} above. (Not recommended)
+\ifnum\ACM@basesize=9\relax
+  \renewcommand{\@ptsize}{}
+  \renewcommand{\normalsize}{%
+    \@setfontsize\normalsize\@ixpt{10.5\p@}%\ninept%
+    \abovedisplayskip 6\p@ \@plus2\p@ \@minus\p@
+    \belowdisplayskip \abovedisplayskip
+    \abovedisplayshortskip 6\p@ \@minus 3\p@
+    \belowdisplayshortskip 6\p@ \@minus 3\p@
+    \let\@listi\@listI}
+\fi
+\ifnum\ACM@basesize=10\relax
+  \renewcommand{\@ptsize}{}
+  \renewcommand{\normalsize}{%
+    \@setfontsize\normalsize\@xpt{11.5\p@}%\ninept%
+    \abovedisplayskip 6.5\p@ \@plus2\p@ \@minus\p@
+    \belowdisplayskip \abovedisplayskip
+    \abovedisplayshortskip 6.5\p@ \@minus 3\p@
+    \belowdisplayshortskip 6.5\p@ \@minus 3\p@
+    \let\@listi\@listI}
+\fi
+\else
+  \def\@normalsize{%changed next to 9 from 10
+    \@setsize\normalsize{9\p@}\ixpt\@ixpt
+   \abovedisplayskip 6\p@ \@plus2\p@ \@minus\p@
+    \belowdisplayskip \abovedisplayskip
+    \abovedisplayshortskip 6\p@ \@minus 3\p@
+    \belowdisplayshortskip 6\p@ \@minus 3\p@
+    \let\@listi\@listI
+  }%
+\fi
+\if@ll
+\ifnum\ACM@basesize=9\relax
+  \newcommand\scriptsize{\@setfontsize\scriptsize\@viipt{8\p@}}
+  \newcommand\tiny{\@setfontsize\tiny\@vpt{6\p@}}
+  \newcommand\large{\@setfontsize\large\@xiipt{14\p@}}
+  \newcommand\Large{\@setfontsize\Large\@xivpt{18\p@}}
+  \newcommand\LARGE{\@setfontsize\LARGE\@xviipt{20\p@}}
+  \newcommand\huge{\@setfontsize\huge\@xxpt{25\p@}}
+  \newcommand\Huge{\@setfontsize\Huge\@xxvpt{30\p@}}
+\fi
+\ifnum\ACM@basesize=10\relax
+  \newcommand\scriptsize{\@setfontsize\scriptsize\@viiipt{9\p@}}
+  \newcommand\tiny{\@setfontsize\tiny\@vipt{7\p@}}
+  \newcommand\large{\@setfontsize\large\@xiiipt{15\p@}}
+  \newcommand\Large{\@setfontsize\Large\@xvpt{20\p@}}
+  \newcommand\LARGE{\@setfontsize\LARGE\@xixpt{22\p@}}
+  \newcommand\huge{\@setfontsize\huge\@xixpt{30\p@}}
+  \newcommand\Huge{\@setfontsize\Huge30pt{36\p@}}
+\fi
+\else
+  \def\scriptsize{\@setsize\scriptsize{8\p@}\viipt\@viipt}
+  \def\tiny{\@setsize\tiny{6\p@}\vpt\@vpt}
+  \def\large{\@setsize\large{14\p@}\xiipt\@xiipt}
+  \def\Large{\@setsize\Large{18\p@}\xivpt\@xivpt}
+  \def\LARGE{\@setsize\LARGE{20\p@}\xviipt\@xviipt}
+  \def\huge{\@setsize\huge{25\p@}\xxpt\@xxpt}
+  \def\Huge{\@setsize\Huge{30\p@}\xxvpt\@xxvpt}
+\fi
+\normalsize
+
+% make aubox hsize/number of authors up to 3, less gutter
+% then showbox gutter showbox gutter showbox -- GKMT Aug 99
+\newbox\@acmtitlebox
+\ifnum\ACM@basesize=9\relax
+\def\@maketitle{\newpage
+ \null
+ \setbox\@acmtitlebox\vbox{%
+\baselineskip 20pt
+\vskip 2em                   % Vertical space above title.
+   \begin{center}
+    {\ttlfnt \@title\par}       % Title set in 18pt Helvetica (Arial) bold size.
+    \vskip 1.5em                % Vertical space after title.
+%This should be the subtitle.
+{\subttlfnt \the\subtitletext\par}\vskip 1.25em%\fi
+    {\baselineskip 16pt\aufnt   % each author set in \12 pt Arial, in a
+     \lineskip .5em             % tabular environment
+     \begin{tabular}[t]{c}\@author
+     \end{tabular}\par}
+    \vskip 1.5em               % Vertical space after author.
+   \end{center}}
+ \dimen0=\ht\@acmtitlebox
+ \advance\dimen0 by -12.75pc\relax % Increased space for title box -- KBT
+ \unvbox\@acmtitlebox
+ \ifdim\dimen0<0.0pt\relax\vskip-\dimen0\fi}
+\fi
+\ifnum\ACM@basesize=10\relax
+\def\@maketitle{\newpage
+ \null
+ \setbox\@acmtitlebox\vbox{%
+\baselineskip 22pt
+\vskip 2.2em                   % Vertical space above title.
+   \begin{center}
+    {\ttlfnt \@title\par}       % Title set in 18pt Helvetica (Arial) bold size.
+    \vskip 2em                % Vertical space after title.
+%This should be the subtitle.
+{\subttlfnt \the\subtitletext\par}\vskip 1.25em%\fi
+    {\baselineskip 18pt\aufnt   % each author set in \12 pt Arial, in a
+     \lineskip .5em             % tabular environment
+     \begin{tabular}[t]{c}\@author
+     \end{tabular}\par}
+    \vskip 2em               % Vertical space after author.
+   \end{center}}
+ \dimen0=\ht\@acmtitlebox
+ \advance\dimen0 by -12.75pc\relax % Increased space for title box -- KBT
+ \unvbox\@acmtitlebox
+ \ifdim\dimen0<0.0pt\relax\vskip-\dimen0\fi}
+\fi
+
+\newcount\titlenotecount
+\global\titlenotecount=0
+\newtoks\tntoks
+\newtoks\tntokstwo
+\newtoks\tntoksthree
+\newtoks\tntoksfour
+\newtoks\tntoksfive
+
+\def\abstract{
+\ifnum\titlenotecount>0 % was =1
+    \insert\footins{%
+    \reset@font\footnotesize
+        \interlinepenalty\interfootnotelinepenalty
+        \splittopskip\footnotesep
+        \splitmaxdepth \dp\strutbox \floatingpenalty \@MM
+        \hsize\columnwidth \@parboxrestore
+        \protected@edef\@currentlabel{%
+        }%
+        \color@begingroup
+\ifnum\titlenotecount=1
+      \@maketntext{%
+         \raisebox{4pt}{$\ast$}\rule\z@\footnotesep\ignorespaces\the\tntoks\@finalstrut\strutbox}%
+\fi
+\ifnum\titlenotecount=2
+      \@maketntext{%
+      \raisebox{4pt}{$\ast$}\rule\z@\footnotesep\ignorespaces\the\tntoks\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\dagger$}\rule\z@\footnotesep\ignorespaces\the\tntokstwo\@finalstrut\strutbox}%
+\fi
+\ifnum\titlenotecount=3
+      \@maketntext{%
+         \raisebox{4pt}{$\ast$}\rule\z@\footnotesep\ignorespaces\the\tntoks\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\dagger$}\rule\z@\footnotesep\ignorespaces\the\tntokstwo\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\ddagger$}\rule\z@\footnotesep\ignorespaces\the\tntoksthree\@finalstrut\strutbox}%
+\fi
+\ifnum\titlenotecount=4
+      \@maketntext{%
+         \raisebox{4pt}{$\ast$}\rule\z@\footnotesep\ignorespaces\the\tntoks\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\dagger$}\rule\z@\footnotesep\ignorespaces\the\tntokstwo\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\ddagger$}\rule\z@\footnotesep\ignorespaces\the\tntoksthree\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\S$}\rule\z@\footnotesep\ignorespaces\the\tntoksfour\@finalstrut\strutbox}%
+\fi
+\ifnum\titlenotecount=5
+      \@maketntext{%
+         \raisebox{4pt}{$\ast$}\rule\z@\footnotesep\ignorespaces\the\tntoks\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\dagger$}\rule\z@\footnotesep\ignorespaces\the\tntokstwo\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\ddagger$}\rule\z@\footnotesep\ignorespaces\the\tntoksthree\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\S$}\rule\z@\footnotesep\ignorespaces\the\tntoksfour\par\@finalstrut\strutbox}%
+\@maketntext{%
+         \raisebox{4pt}{$\P$}\rule\z@\footnotesep\ignorespaces\the\tntoksfive\@finalstrut\strutbox}%
+\fi
+   \color@endgroup} %g}
+\fi
+\setcounter{footnote}{0}
+\section*{ABSTRACT}\normalsize%\ninept
+}
+
+\def\endabstract{\if@twocolumn\else\endquotation\fi}
+
+\def\keywords{\if@twocolumn
+\section*{Keywords}
+\else \small
+\quotation
+\fi}
+
+\def\terms#1{%
+%\if@twocolumn
+%\section*{General Terms}
+%\else \small
+%\quotation
+%\fi
+}
+
+% -- Classification needs to be a bit smart due to optionals - Gerry/Georgia November 2nd. 1999
+\newcount\catcount
+\global\catcount=1
+
+\def\category#1#2#3{%
+\ifnum\catcount=1
+\section*{Categories and Subject Descriptors}
+\advance\catcount by 1\else{\unskip; }\fi
+    \@ifnextchar [{\@category{#1}{#2}{#3}}{\@category{#1}{#2}{#3}[]}%
+}
+
+
+\def\@category#1#2#3[#4]{%
+    \begingroup
+        \let\and\relax
+            #1 [\textbf{#2}]%
+            \if!#4!%
+                \if!#3!\else : #3\fi
+            \else
+                :\space
+                \if!#3!\else #3\kern\z@---\hskip\z@\fi
+                \textit{#4}%
+            \fi
+    \endgroup
+}
+%
+
+
+
+
+
+
+%%% This section (written by KBT) handles the 1" box in the lower left
+%%% corner of the left column of the first page by creating a picture,
+%%% and inserting the predefined string at the bottom (with a negative
+%%% displacement to offset the space allocated for a non-existent
+%%% caption).
+%%%
+\newtoks\copyrightnotice
+\def\ftype@copyrightbox{8}
+\def\@copyrightspace{
+\@float{copyrightbox}[b]
+\begin{center}
+\setlength{\unitlength}{1pc}
+\ifnum\ACM@basesize=9
+\begin{picture}(20,6) %Space for copyright notice
+\put(0,-0.95){\crnotice{\@toappear}}
+\end{picture}
+\fi
+\ifnum\ACM@basesize=10
+\begin{picture}(20,7) %Space for copyright notice
+\put(0,-0.95){\crnotice{\@toappear}}
+\end{picture}
+\fi
+\end{center}
+\end@float}
+
+\def\@toappear{} % Default setting blank - commands below change this.
+\long\def\toappear#1{\def\@toappear{\parbox[b]{20pc}{\baselineskip 9pt#1}}}
+\def\toappearbox#1{\def\@toappear{\raisebox{5pt}{\framebox[20pc]{\parbox[b]{19pc}{#1}}}}}
+
+\newtoks\conf
+\newtoks\confinfo
+\def\conferenceinfo#1#2{\global\conf={#1}\global\confinfo{#2}}
+
+
+%\def\marginpar{\@latexerr{The \marginpar command is not allowed in the
+%  `acmconf' document style.}\@eha}
+
+\def\marginpar{\ClassError{%
+    \string\marginpar\space is not allowed in the `acmconf' document		% January 2008
+    style}\@eha}
+
+\mark{{}{}}     % Initializes TeX's marks
+
+\def\today{\ifcase\month\or
+  January\or February\or March\or April\or May\or June\or
+  July\or August\or September\or October\or November\or December\fi
+  \space\number\day, \number\year}
+
+\def\@begintheorem#1#2{%
+    \parskip 0pt % GM July 2000 (for tighter spacing)
+    \trivlist
+    \item[%
+        \hskip 10\p@
+        \hskip \labelsep
+        {{\sc #1}\hskip 5\p@\relax#2.}%
+    ]
+    \it
+}
+\def\@opargbegintheorem#1#2#3{%
+    \parskip 0pt % GM July 2000 (for tighter spacing)
+    \trivlist
+    \item[%
+        \hskip 10\p@
+        \hskip \labelsep
+        {\sc #1\ #2\             % This mod by Gerry to enumerate corollaries
+   \setbox\@tempboxa\hbox{(#3)}  % and bracket the 'corollary title'
+        \ifdim \wd\@tempboxa>\z@ % and retain the correct numbering of e.g. theorems
+            \hskip 5\p@\relax    % if they occur 'around' said corollaries.
+            \box\@tempboxa       % Gerry - Nov. 1999.
+        \fi.}%
+    ]
+    \it
+}
+\newif\if@qeded
+\global\@qededfalse
+
+% -- original
+%\def\proof{%
+%  \vspace{-\parskip} % GM July 2000 (for tighter spacing)
+%    \global\@qededfalse
+%    \@ifnextchar[{\@xproof}{\@proof}%
+%}
+% -- end of original
+
+% (JSS) Fix for vertical spacing bug - Gerry Murray July 30th. 2002
+\def\proof{%
+\vspace{-\lastskip}\vspace{-\parsep}\penalty-51%
+\global\@qededfalse
+\@ifnextchar[{\@xproof}{\@proof}%
+}
+
+\def\endproof{%
+    \if@qeded\else\qed\fi
+    \endtrivlist
+}
+\def\@proof{%
+    \trivlist
+    \item[%
+        \hskip 10\p@
+        \hskip \labelsep
+        {\sc Proof.}%
+    ]
+    \ignorespaces
+}
+\def\@xproof[#1]{%
+    \trivlist
+    \item[\hskip 10\p@\hskip \labelsep{\sc Proof #1.}]%
+    \ignorespaces
+}
+\def\qed{%
+    \unskip
+    \kern 10\p@
+    \begingroup
+        \unitlength\p@
+        \linethickness{.4\p@}%
+        \framebox(6,6){}%
+    \endgroup
+    \global\@qededtrue
+}
+
+\def\newdef#1#2{%
+    \expandafter\@ifdefinable\csname #1\endcsname
+        {\@definecounter{#1}%
+         \expandafter\xdef\csname the#1\endcsname{\@thmcounter{#1}}%
+         \global\@namedef{#1}{\@defthm{#1}{#2}}%
+         \global\@namedef{end#1}{\@endtheorem}%
+    }%
+}
+\def\@defthm#1#2{%
+    \refstepcounter{#1}%
+    \@ifnextchar[{\@ydefthm{#1}{#2}}{\@xdefthm{#1}{#2}}%
+}
+\def\@xdefthm#1#2{%
+    \@begindef{#2}{\csname the#1\endcsname}%
+    \ignorespaces
+}
+\def\@ydefthm#1#2[#3]{%
+    \trivlist
+    \item[%
+        \hskip 10\p@
+        \hskip \labelsep
+        {\it #2%
+%         \savebox\@tempboxa{#3}%
+         \saveb@x\@tempboxa{#3}%		% January 2008
+         \ifdim \wd\@tempboxa>\z@
+            \ \box\@tempboxa
+         \fi.%
+        }]%
+    \ignorespaces
+}
+\def\@begindef#1#2{%
+    \trivlist
+    \item[%
+        \hskip 10\p@
+        \hskip \labelsep
+        {\it #1\ \rm #2.}%
+    ]%
+}
+\def\theequation{\arabic{equation}}
+
+\newcounter{part}
+\newcounter{section}
+\newcounter{subsection}[section]
+\newcounter{subsubsection}[subsection]
+\newcounter{paragraph}[subsubsection]
+\def\thepart{\Roman{part}}
+\def\thesection{\arabic{section}}
+\def\thesubsection{\thesection.\arabic{subsection}}
+\def\thesubsubsection{\thesubsection.\arabic{subsubsection}} %removed \subsecfnt 29 July 2002 gkmt
+\def\theparagraph{\thesubsubsection.\arabic{paragraph}} %removed \subsecfnt 29 July 2002 gkmt
+\newif\if@uchead
+\@ucheadfalse
+
+%% CHANGES: NEW NOTE
+%% NOTE: OK to use old-style font commands below, since they were
+%% suitably redefined for LaTeX2e
+%% END CHANGES
+\setcounter{secnumdepth}{3}
+\def\part{%
+    \@startsection{part}{9}{\z@}{-10\p@ \@plus -4\p@ \@minus -2\p@}
+        {4\p@}{\normalsize\@ucheadtrue}%
+}
+\def\section{%
+    \@startsection{section}{1}{\z@}{-10\p@ \@plus -4\p@ \@minus -2\p@}% GM
+    {4\p@}{\baselineskip 14pt\secfnt\@ucheadtrue}%
+}
+
+\def\subsection{%
+    \@startsection{subsection}{2}{\z@}{-8\p@ \@plus -2\p@ \@minus -\p@}
+    {4\p@}{\secfnt}%
+}
+\def\subsubsection{%
+    \@startsection{subsubsection}{3}{\z@}{-8\p@ \@plus -2\p@ \@minus -\p@}%
+    {4\p@}{\subsecfnt}%
+}
+%\def\paragraph{%
+%    \vskip 12pt\@startsection{paragraph}{3}{\z@}{6\p@ \@plus \p@}% original
+%    {-5\p@}{\subsecfnt}%
+%}
+%  If one wants sections, subsections and subsubsections numbered,
+%  but not paragraphs, one usually sets secnumepth to 3.
+%  For that, the "depth" of paragraphs must be given correctly
+%  in the definition (``4'' instead of ``3'' as second argument
+%  of @startsection):
+\def\paragraph{%
+    \vskip 12pt\@startsection{paragraph}{4}{\z@}{6\p@ \@plus \p@}%    % GM and Wolfgang May - 11/30/06
+    {-5\p@}{\subsecfnt}%
+}
+\let\@period=.
+\def\@startsection#1#2#3#4#5#6{%
+        \if@noskipsec  %gkmt, 11 aug 99
+        \global\let\@period\@empty
+        \leavevmode
+        \global\let\@period.%
+    \fi
+      \par %
+    \@tempskipa #4\relax
+    \@afterindenttrue
+    \ifdim \@tempskipa <\z@
+        \@tempskipa -\@tempskipa
+        \@afterindentfalse
+    \fi
+    \if@nobreak
+    \everypar{}%
+    \else
+        \addpenalty\@secpenalty
+        \addvspace\@tempskipa
+    \fi
+\parskip=0pt % GM July 2000 (non numbered) section heads
+    \@ifstar
+        {\@ssect{#3}{#4}{#5}{#6}}
+        {\@dblarg{\@sect{#1}{#2}{#3}{#4}{#5}{#6}}}%
+}
+\def\@sect#1#2#3#4#5#6[#7]#8{%
+    \ifnum #2>\c@secnumdepth
+        \let\@svsec\@empty
+    \else
+        \refstepcounter{#1}%
+        \edef\@svsec{%
+            \begingroup
+                %\ifnum#2>2 \noexpand\rm \fi % changed to next 29 July 2002 gkmt
+            \ifnum#2>2 \noexpand#6 \fi
+                \csname the#1\endcsname
+            \endgroup
+            \ifnum #2=1\relax .\fi
+            \hskip 1em
+        }%
+    \fi
+    \@tempskipa #5\relax
+    \ifdim \@tempskipa>\z@
+        \begingroup
+            #6\relax
+            \@hangfrom{\hskip #3\relax\@svsec}%
+            \begingroup
+                \interlinepenalty \@M
+                \if@uchead
+                    \uppercase{#8}%
+                \else
+                    #8%
+                \fi
+                \par
+            \endgroup
+        \endgroup
+        \csname #1mark\endcsname{#7}%
+        \vskip -12pt  %gkmt, 11 aug 99 and GM July 2000 (was -14) - numbered section head spacing
+\addcontentsline{toc}{#1}{%
+            \ifnum #2>\c@secnumdepth \else
+                \protect\numberline{\csname the#1\endcsname}%
+            \fi
+            #7%
+        }%
+    \else
+        \def\@svsechd{%
+            #6%
+            \hskip #3\relax
+            \@svsec
+            \if@uchead
+                \uppercase{#8}%
+            \else
+                #8%
+            \fi
+            \csname #1mark\endcsname{#7}%
+            \addcontentsline{toc}{#1}{%
+                \ifnum #2>\c@secnumdepth \else
+                    \protect\numberline{\csname the#1\endcsname}%
+                \fi
+                #7%
+            }%
+        }%
+    \fi
+    \@xsect{#5}\hskip 1pt
+    \par
+}
+\def\@xsect#1{%
+    \@tempskipa #1\relax
+    \ifdim \@tempskipa>\z@
+        \par
+        \nobreak
+        \vskip \@tempskipa
+        \@afterheading
+    \else
+        \global\@nobreakfalse
+        \global\@noskipsectrue
+        \everypar{%
+            \if@noskipsec
+                \global\@noskipsecfalse
+                \clubpenalty\@M
+                \hskip -\parindent
+                \begingroup
+                    \@svsechd
+                    \@period
+                \endgroup
+                \unskip
+                \@tempskipa #1\relax
+                \hskip -\@tempskipa
+            \else
+                \clubpenalty \@clubpenalty
+                \everypar{}%
+            \fi
+        }%
+    \fi
+    \ignorespaces
+}
+\def\@trivlist{%
+    \@topsepadd\topsep
+    \if@noskipsec
+        \global\let\@period\@empty
+        \leavevmode
+        \global\let\@period.%
+    \fi
+    \ifvmode
+        \advance\@topsepadd\partopsep
+    \else
+        \unskip
+        \par
+    \fi
+    \if@inlabel
+        \@noparitemtrue
+        \@noparlisttrue
+    \else
+        \@noparlistfalse
+        \@topsep\@topsepadd
+    \fi
+    \advance\@topsep \parskip
+    \leftskip\z@skip
+    \rightskip\@rightskip
+    \parfillskip\@flushglue
+    \@setpar{\if@newlist\else{\@@par}\fi}
+    \global\@newlisttrue
+    \@outerparskip\parskip
+}
+
+%%% Actually, 'abbrev' works just fine as the default
+%%% Bibliography style.
+
+\typeout{Using 'Abbrev' bibliography style}
+\newcommand\bibyear[2]{%
+    \unskip\quad\ignorespaces#1\unskip
+    \if#2..\quad \else \quad#2 \fi
+}
+\newcommand{\bibemph}[1]{{\em#1}}
+\newcommand{\bibemphic}[1]{{\em#1\/}}
+\newcommand{\bibsc}[1]{{\sc#1}}
+\def\@normalcite{%
+    \def\@cite##1##2{[##1\if@tempswa , ##2\fi]}%
+}
+\def\@citeNB{%
+    \def\@cite##1##2{##1\if@tempswa , ##2\fi}%
+}
+\def\@citeRB{%
+    \def\@cite##1##2{##1\if@tempswa , ##2\fi]}%
+}
+\def\start@cite#1#2{%
+    \edef\citeauthoryear##1##2##3{%
+        ###1%
+        \ifnum#2=\z@ \else\ ###2\fi
+    }%
+    \ifnum#1=\thr@@
+        \let\@@cite\@citeyear
+    \else
+        \let\@@cite\@citenormal
+    \fi
+    \@ifstar{\@citeNB\@@cite}{\@normalcite\@@cite}%
+}
+%\def\cite{\start@cite23}
+\DeclareRobustCommand\cite{\start@cite23}		% January 2008
+\def\citeNP{\cite*}					% No Parentheses e.g. 5
+%\def\citeA{\start@cite10}
+\DeclareRobustCommand\citeA{\start@cite10}		% January 2008
+\def\citeANP{\citeA*}
+%\def\shortcite{\start@cite23}				
+\DeclareRobustCommand\shortcite{\start@cite23}		% January 2008
+\def\shortciteNP{\shortcite*}
+%\def\shortciteA{\start@cite20}
+\DeclareRobustCommand\shortciteA{\start@cite20}		% January 2008
+\def\shortciteANP{\shortciteA*}
+%\def\citeyear{\start@cite30}
+\DeclareRobustCommand\citeyear{\start@cite30}		% January 2008
+\def\citeyearNP{\citeyear*}
+%\def\citeN{%
+\DeclareRobustCommand\citeN{%				% January 2008
+    \@citeRB
+    \def\citeauthoryear##1##2##3{##1\ [##3%
+        \def\reserved@a{##1}%
+        \def\citeauthoryear####1####2####3{%
+            \def\reserved@b{####1}%
+            \ifx\reserved@a\reserved@b
+                ####3%
+            \else
+                \errmessage{Package acmart Error: author mismatch
+                         in \string\citeN^^J^^J%
+                    See the acmart package documentation for explanation}%
+            \fi
+        }%
+    }%
+    \@ifstar\@citeyear\@citeyear
+}
+%\def\shortciteN{%
+\DeclareRobustCommand\shortciteN{%			% January 2008
+    \@citeRB
+    \def\citeauthoryear##1##2##3{##2\ [##3%
+        \def\reserved@a{##2}%
+        \def\citeauthoryear####1####2####3{%
+            \def\reserved@b{####2}%
+            \ifx\reserved@a\reserved@b
+                ####3%
+            \else
+                \errmessage{Package acmart Error: author mismatch
+                         in \string\shortciteN^^J^^J%
+                    See the acmart package documentation for explanation}%
+            \fi
+        }%
+    }%
+    \@ifstar\@citeyear\@citeyear  % GM July 2000
+}
+
+\def\@citenormal{%
+    \@ifnextchar [{\@tempswatrue\@citex;}%
+% original                 {\@tempswafalse\@citex,[]}% was ; Gerry 2/24/00
+{\@tempswafalse\@citex[]}%  	% GERRY FIX FOR BABEL 3/20/2009
+}
+
+\def\@citeyear{%
+    \@ifnextchar [{\@tempswatrue\@citex,}%
+% original                  {\@tempswafalse\@citex,[]}%
+{\@tempswafalse\@citex[]}%	%  GERRY FIX FOR BABEL 3/20/2009
+}
+
+\def\@citex#1[#2]#3{%
+    \let\@citea\@empty
+    \@cite{%
+        \@for\@citeb:=#3\do{%
+            \@citea
+% original            \def\@citea{#1 }%
+            \def\@citea{#1, }% 	% GERRY FIX FOR BABEL 3/20/2009 -- SO THAT YOU GET [1, 2] IN THE BODY TEXT
+            \edef\@citeb{\expandafter\@iden\@citeb}%
+            \if@filesw
+                \immediate\write\@auxout{\string\citation{\@citeb}}%
+            \fi
+            \@ifundefined{b@\@citeb}{%
+                {\bf ?}%
+                \@warning{%
+                    Citation `\@citeb' on page \thepage\space undefined%
+                }%
+            }%
+            {\csname b@\@citeb\endcsname}%
+        }%
+    }{#2}%
+}
+%\let\@biblabel\@gobble   % Dec. 2008 - Gerry
+% ----
+\def\@biblabelnum#1{[#1]} % Gerry's solution #1 - for Natbib -- April 2009
+\let\@biblabel=\@biblabelnum  % Gerry's solution #1 - for Natbib -- April 2009
+\def\newblock{\relax} % Gerry Dec. 2008
+% ---
+\newdimen\bibindent
+\setcounter{enumi}{1}
+\bibindent=0em
+\def\thebibliography#1{% 
+\ifnum\addauflag=0\addauthorsection\global\addauflag=1\fi
+     \section[References]{%    <=== OPTIONAL ARGUMENT ADDED HERE
+        {References} % was uppercased but this affects pdf bookmarks (SP/GM October 2004)
+          {\vskip -9pt plus 1pt} % GM Nov. 2006 / GM July 2000 (for somewhat tighter spacing) 
+         \@mkboth{{\refname}}{{\refname}}%
+     }%
+     \list{[\arabic{enumi}]}{%
+         \settowidth\labelwidth{[#1]}%
+         \leftmargin\labelwidth
+         \advance\leftmargin\labelsep
+         \advance\leftmargin\bibindent
+         \parsep=0pt\itemsep=1pt % GM July 2000
+         \itemindent -\bibindent
+         \listparindent \itemindent
+         \usecounter{enumi}
+     }%
+     \let\newblock\@empty
+     \raggedright % GM July 2000
+     \sloppy
+     \sfcode`\.=1000\relax
+}
+
+
+\gdef\balancecolumns
+{\vfill\eject
+\global\@colht=\textheight
+\global\ht\@cclv=\textheight
+}
+
+\newcount\colcntr
+\global\colcntr=0
+%\newbox\savebox
+\newbox\saveb@x				% January 2008
+
+\gdef \@makecol {%
+\global\advance\colcntr by 1
+\ifnum\colcntr>2 \global\colcntr=1\fi
+   \ifvoid\footins
+     \setbox\@outputbox \box\@cclv
+   \else
+     \setbox\@outputbox \vbox{%
+\boxmaxdepth \@maxdepth
+       \@tempdima\dp\@cclv
+       \unvbox \@cclv
+       \vskip-\@tempdima
+       \vskip \skip\footins
+       \color@begingroup
+         \normalcolor
+         \footnoterule
+         \unvbox \footins
+       \color@endgroup
+       }%
+   \fi
+   \xdef\@freelist{\@freelist\@midlist}%
+   \global \let \@midlist \@empty
+   \@combinefloats
+   \ifvbox\@kludgeins
+     \@makespecialcolbox
+   \else
+     \setbox\@outputbox \vbox to\@colht {%
+\@texttop
+       \dimen@ \dp\@outputbox
+       \unvbox \@outputbox
+   \vskip -\dimen@
+       \@textbottom
+       }%
+   \fi
+   \global \maxdepth \@maxdepth
+}
+\def\titlenote{\@ifnextchar[\@xtitlenote{\stepcounter\@mpfn
+\global\advance\titlenotecount by 1
+\ifnum\titlenotecount=1
+    \raisebox{9pt}{$\ast$}
+\fi
+\ifnum\titlenotecount=2
+    \raisebox{9pt}{$\dagger$}
+\fi
+\ifnum\titlenotecount=3
+    \raisebox{9pt}{$\ddagger$}
+\fi
+\ifnum\titlenotecount=4
+\raisebox{9pt}{$\S$}
+\fi
+\ifnum\titlenotecount=5
+\raisebox{9pt}{$\P$}
+\fi
+         \@titlenotetext
+}}
+
+\long\def\@titlenotetext#1{\insert\footins{%
+\ifnum\titlenotecount=1\global\tntoks={#1}\fi
+\ifnum\titlenotecount=2\global\tntokstwo={#1}\fi
+\ifnum\titlenotecount=3\global\tntoksthree={#1}\fi
+\ifnum\titlenotecount=4\global\tntoksfour={#1}\fi
+\ifnum\titlenotecount=5\global\tntoksfive={#1}\fi
+    \reset@font\footnotesize
+    \interlinepenalty\interfootnotelinepenalty
+    \splittopskip\footnotesep
+    \splitmaxdepth \dp\strutbox \floatingpenalty \@MM
+    \hsize\columnwidth \@parboxrestore
+    \protected@edef\@currentlabel{%
+    }%
+    \color@begingroup
+   \color@endgroup}}
+
+%%%%%%%%%%%%%%%%%%%%%%%%%
+\ps@plain
+\baselineskip=11pt
+\let\thepage\relax % For NO page numbers - GM Nov. 30th. 1999 and July 2000
+\def\setpagenumber#1{\global\setcounter{page}{#1}}
+%\pagenumbering{arabic}  % Arabic page numbers GM July 2000
+\twocolumn             % Double column.
+\flushbottom           % Even bottom -- alas, does not balance columns at end of document
+\pagestyle{plain}
+
+% Need Copyright Year and Copyright Data to be user definable (in .tex file).
+% Gerry Nov. 30th. 1999
+\newtoks\copyrtyr
+\newtoks\acmcopyr
+\newtoks\boilerplate
+\global\acmcopyr={X-XXXXX-XX-X/XX/XX}  % Default - 5/11/2001 *** Gerry
+\global\copyrtyr={\the\year}                % Default - 3/3/2003 *** Gerry
+\def\acmPrice#1{\gdef\@acmPrice{#1}}
+\acmPrice{} %article price  % Changed to 15 - June 2012 - Gerry
+
+
+\def\CopyrightYear#1{\global\copyrtyr{#1}}
+\def\crdata#1{\global\acmcopyr{#1}}
+\def\permission#1{\global\boilerplate{#1}}
+
+% ISBN
+%
+\def\isbn#1{\global\acmcopyr={#1}}
+\isbn{978-1-4503-2138-9}
+
+\RequirePackage{url}
+\urlstyle{rm}
+\def\doi#1{\def\@doi{#1}}
+\doi{10.1145/1235}
+\def\printdoi#1{\url{#1}}
+
+
+
+% Copyright
+\RequirePackage{acmcopyright}
+\setcopyright{none}
+
+%
+\global\boilerplate={\@copyrightpermission}
+
+
+
+\newtoks\copyrightetc
+\ifnum\ACM@basesize=9\relax
+\global\copyrightetc{%
+{\noindent\confname\ \the\conf\ \the\confinfo}\par\smallskip
+  \if@printcopyright
+    \copyright\ \the\copyrtyr\ \@copyrightowner
+  \fi
+  \if@acmowned ISBN \else\ifnum\acm@copyrightmode=2 ISBN \else \par\smallskip ACM ISBN \fi\fi
+ \the\acmcopyr\ifx\@acmPrice\@empty.\else\dots\@acmPrice\fi\par\smallskip
+{DOI: \small\expandafter\printdoi\expandafter{\@doi}}} 
+\toappear{\fontsize{7pt}{8pt}\fontfamily{ptm}\selectfont
+  \the\boilerplate\par\smallskip
+ \the\copyrightetc}
+\fi
+\ifnum\ACM@basesize=10\relax
+\global\copyrightetc{%
+{\noindent\confname\ \the\conf\ \the\confinfo}\par\smallskip
+  \if@printcopyright
+    \copyright\ \the\copyrtyr\ \@copyrightowner
+  \fi
+  \if@acmowned ISBN \else\ifnum\acm@copyrightmode=2 ISBN \else \par\smallskip ACM ISBN \fi\fi
+ \the\acmcopyr\ifx\@acmPrice\@empty.\else\dots\@acmPrice\fi\par\smallskip
+{DOI: \small\expandafter\printdoi\expandafter{\@doi}}} 
+\toappear{\fontsize{7.5pt}{8.5pt}\fontfamily{ptm}\selectfont
+  \the\boilerplate\par\smallskip
+ \the\copyrightetc}
+\fi
+%\DeclareFixedFont{\altcrnotice}{OT1}{tmr}{m}{n}{8}  % << patch needed for accenting e.g. Montreal - Gerry, May 2007
+%\DeclareFixedFont{\altconfname}{OT1}{tmr}{m}{it}{8}  % << patch needed for accenting in italicized confname - Gerry, May 2007
+%
+%{\altconfname{{\the\conf}}} {\altcrnotice\the\confinfo\par} \the\copyrightetc.}  % << Gerry, May 2007
+%
+% The following section (i.e. 3 .sty inclusions) was added in May 2007 so as to fix the problems that many
+% authors were having with accents. Sometimes accents would occur, but the letter-character would be of a different
+% font. Conversely the letter-character font would be correct but, e.g. a 'bar' would appear superimposed on the
+% character instead of, say, an unlaut/diaresis. Sometimes the letter-character would NOT appear at all.
+% Using [T1]{fontenc} outright was not an option as this caused 99% of the authors to 'produce' a Type-3 (bitmapped)
+% PDF file - useless for production. 
+%
+% For proper (font) accenting we NEED these packages to be part of the .cls file i.e. 'ae', 'aecompl' and 'aeguil' 
+% ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+%% This is file `ae.sty' 
+\def\fileversion{1.3}
+\def\filedate{2001/02/12}
+\NeedsTeXFormat{LaTeX2e}
+%\ProvidesPackage{ae}[\filedate\space\fileversion\space  % GM
+% Almost European Computer Modern]                       % GM - keeping the log file clean(er)
+\newif\if@ae@slides \@ae@slidesfalse
+\DeclareOption{slides}{\@ae@slidestrue}
+\ProcessOptions
+\fontfamily{aer}
+\RequirePackage[T1]{fontenc}
+\if@ae@slides
+    \renewcommand{\sfdefault}{laess}
+    \renewcommand{\rmdefault}{laess} % no roman
+    \renewcommand{\ttdefault}{laett}
+\else
+    \renewcommand{\sfdefault}{aess}
+    \renewcommand{\rmdefault}{aer}
+    \renewcommand{\ttdefault}{aett}
+\fi
+\endinput
+%% 
+%% End of file `ae.sty'.
+%
+%
+\def\fileversion{0.9}
+\def\filedate{1998/07/23}
+\NeedsTeXFormat{LaTeX2e}
+%\ProvidesPackage{aecompl}[\filedate\space\fileversion\space   % GM
+%T1 Complements for AE fonts (D. Roegel)]                      % GM -- keeping the log file clean(er)
+ 
+\def\@ae@compl#1{{\fontencoding{T1}\fontfamily{cmr}\selectfont\symbol{#1}}}
+\def\guillemotleft{\@ae@compl{19}}
+\def\guillemotright{\@ae@compl{20}}
+\def\guilsinglleft{\@ae@compl{14}}
+\def\guilsinglright{\@ae@compl{15}}
+\def\TH{\@ae@compl{222}}
+\def\NG{\@ae@compl{141}}
+\def\ng{\@ae@compl{173}}
+\def\th{\@ae@compl{254}}
+\def\DJ{\@ae@compl{208}}
+\def\dj{\@ae@compl{158}}
+\def\DH{\@ae@compl{208}}
+\def\dh{\@ae@compl{240}}
+\def\@perthousandzero{\@ae@compl{24}}
+\def\textperthousand{\%\@perthousandzero}
+\def\textpertenthousand{\%\@perthousandzero\@perthousandzero}
+\endinput
+%
+%
+%% This is file `aeguill.sty' 
+% This file gives french guillemets (and not guillemots!)
+% built with the Polish CMR fonts (default), WNCYR fonts, the LASY fonts 
+% or with the EC fonts. 
+% This is useful in conjunction with the ae package
+% (this package loads the ae package in case it has not been loaded)
+%  and with or without the french(le) package.
+%
+% In order to get the guillemets, it is necessary to either type
+% \guillemotleft and \guillemotright, or to use an 8 bit encoding
+% (such as ISO-Latin1) which selects these two commands, 
+% or, if you use the french package (but not the frenchle package), 
+% to type << or >>.
+%
+% By default, you get the Polish CMR guillemets; if this package is loaded
+% with the `cm' option, you get the LASY guillemets; with `ec,' you
+% get the EC guillemets, and with `cyr,' you get the cyrillic guillemets.
+%
+% In verbatim mode, you always get the EC/TT guillemets.
+%
+% The default option is interesting in conjunction with PDF,
+% because there is a Type 1 version of the Polish CMR fonts
+% and these guillemets are very close in shape to the EC guillemets.
+% There are no free Type 1 versions of the EC fonts.
+%
+% Support for Polish CMR guillemets was kindly provided by 
+% Rolf Niepraschk <niepraschk@ptb.de> in version 0.99 (2000/05/22).
+% Bernd Raichle provided extensive simplifications to the code
+% for version 1.00.
+%
+% This package is released under the LPPL.
+%
+% Changes:
+%   Date        version
+%   2001/04/12  1.01    the frenchle and french package are now distinguished.
+%
+\def\fileversion{1.01}
+\def\filedate{2001/04/12}
+\NeedsTeXFormat{LaTeX2e}
+%\ProvidesPackage{aeguill}[2001/04/12 1.01 %    % GM
+%AE fonts with french guillemets (D. Roegel)]   % GM - keeping the log file clean(er)
+%\RequirePackage{ae}  % GM May 2007 - already embedded here
+
+\newcommand{\@ae@switch}[4]{#4}
+\DeclareOption{ec}{\renewcommand\@ae@switch[4]{#1}}
+\DeclareOption{cm}{\renewcommand\@ae@switch[4]{#2}}
+\DeclareOption{cyr}{\renewcommand\@ae@switch[4]{#3}}
+\DeclareOption{pl}{\renewcommand\@ae@switch[4]{#4}}
+
+
+%
+% Load necessary packages
+%
+\@ae@switch{% ec
+  % do nothing
+}{% cm
+  \RequirePackage{latexsym}%  GM - May 2007 - already 'mentioned as required' up above
+}{% cyr
+  \RequirePackage[OT2,T1]{fontenc}%
+}{% pl
+  \RequirePackage[OT4,T1]{fontenc}%
+}
+
+% The following command will be compared to \frenchname,
+% as defined in french.sty and frenchle.sty.
+\def\aeguillfrenchdefault{french}%
+
+\let\guill@verbatim@font\verbatim@font
+\def\verbatim@font{\guill@verbatim@font\ecguills{cmtt}%
+                   \let\guillemotleft\@oguills\let\guillemotright\@fguills}
+
+\begingroup \catcode`\<=13 \catcode`\>=13
+\def\x{\endgroup
+ \def\ae@lfguill{<<}%
+ \def\ae@rfguill{>>}%
+}\x
+
+\newcommand{\ecguills}[1]{%
+  \def\selectguillfont{\fontencoding{T1}\fontfamily{#1}\selectfont}%
+  \def\@oguills{{\selectguillfont\symbol{19}}}%
+  \def\@fguills{{\selectguillfont\symbol{20}}}%
+  } 
+
+\newcommand{\aeguills}{%
+  \ae@guills
+  % We redefine \guillemotleft and \guillemotright
+  % in order to catch them when they are used 
+  % with \DeclareInputText (in latin1.def for instance)
+  % We use \auxWARNINGi as a safe indicator that french.sty is used.
+  \gdef\guillemotleft{\ifx\auxWARNINGi\undefined
+                         \@oguills % neither french.sty nor frenchle.sty
+                      \else
+                         \ifx\aeguillfrenchdefault\frenchname
+                           \ae@lfguill  % french.sty
+                         \else
+                           \@oguills    % frenchle.sty
+                         \fi
+                      \fi}%
+  \gdef\guillemotright{\ifx\auxWARNINGi\undefined
+                         \@fguills % neither french.sty nor frenchle.sty
+                       \else
+                         \ifx\aeguillfrenchdefault\frenchname
+                           \ae@rfguill  % french.sty
+                         \else
+                           \@fguills    % frenchle.sty
+                         \fi
+                       \fi}%
+  }
+
+%
+% Depending on the class option
+% define the internal command \ae@guills
+\@ae@switch{% ec
+  \newcommand{\ae@guills}{%
+    \ecguills{cmr}}%
+}{% cm
+  \newcommand{\ae@guills}{%
+    \def\selectguillfont{\fontencoding{U}\fontfamily{lasy}%
+            \fontseries{m}\fontshape{n}\selectfont}%
+    \def\@oguills{\leavevmode\nobreak
+                \hbox{\selectguillfont (\kern-.20em(\kern.20em}\nobreak}%
+    \def\@fguills{\leavevmode\nobreak
+                \hbox{\selectguillfont \kern.20em)\kern-.2em)}%
+                \ifdim\fontdimen\@ne\font>\z@\/\fi}}%
+}{% cyr
+  \newcommand{\ae@guills}{%
+    \def\selectguillfont{\fontencoding{OT2}\fontfamily{wncyr}\selectfont}%
+    \def\@oguills{{\selectguillfont\symbol{60}}}%
+    \def\@fguills{{\selectguillfont\symbol{62}}}}
+}{% pl
+  \newcommand{\ae@guills}{%
+    \def\selectguillfont{\fontencoding{OT4}\fontfamily{cmr}\selectfont}%
+    \def\@oguills{{\selectguillfont\symbol{174}}}%
+    \def\@fguills{{\selectguillfont\symbol{175}}}}
+}
+
+
+\AtBeginDocument{%
+  \ifx\GOfrench\undefined
+    \aeguills
+  \else
+    \let\aeguill@GOfrench\GOfrench
+    \gdef\GOfrench{\aeguill@GOfrench \aeguills}%
+  \fi
+  }
+
+\endinput
+%
+