Hi Frank, I've been going through the paper this weekend, fixing some of the details like the three definitions of rho, etc. Have we decided to submit it to CQG? If so, I've got some style files and related packages to produce the suggested format. It definitely changes the look of the references a bit. If we have decided to publish there, I'll commit everything tomorrow night after I get a chance to read through the tests section.
Cheers, J
On Sat, Nov 5, 2011 at 11:53 PM, knarf@cct.lsu.edu wrote:
User: knarf Date: 2011/11/05 10:53 PM
Modified: / ET.tex, plot_defaults.py
Log: tbd author list, fix reference, use uft8
File Changes:
Directory: /
File [modified]: ET.tex Delta lines: +16 -26 =================================================================== --- ET.tex 2011-10-28 01:52:58 UTC (rev 157) +++ ET.tex 2011-11-06 03:53:03 UTC (rev 158) @@ -8,7 +8,6 @@ \usepackage{dcolumn} \usepackage{float} \usepackage{graphicx} -\usepackage[latin9]{inputenc} \usepackage{multirow} \usepackage{rotating} \usepackage{subfigure} @@ -18,6 +17,7 @@ \usepackage{wrapfig} \usepackage{multicol} \usepackage{widetext} +\usepackage[utf8]{inputenc}
\usepackage[bookmarks, bookmarksopen, bookmarksnumbered]{hyperref} \usepackage[all]{hypcap} @@ -69,32 +69,22 @@
\title[The Einstein Toolkit]{The Einstein Toolkit: A Community Computational Infrastructure for Relativistic Astrophysics}
-\author{\textbf{TBD}}
% Short list, not really sorted right now: -%\author{ -%Eloisa Bentivegna, -%Bruno Mundim, -%Christian D. Ott, -%Peter Diener, -%Erik Schnetter, -%Ian Hinder, -%Frank Löffler, -%Roland Haas, -%Tanja Bode, +\author{ +Frank Löffler, +Eloisa Bentivegna, +Tanja Bode, +Peter Diener, +Joshua Faber, +Roland Haas, +Ian Hinder, +Bruno Mundim, +Christian D. Ott, +Erik Schnetter, +Gabrielle Allen, +Manuela Campanelli, +Pablo Laguna}
-% POTENTIAL AUTHORS: M. Alcubierre, G. Allen, M. Ansorg, L. Baiotti, -% E. Bentivegna, S. Bernuzzi, T. Bode, S. Brandt, G. Corvino, R. De -% Pietri, P. Diener, H. Dimmelmeier, Y. El Khamra, J. Faber, T. Font, J. -% Frieben, B. Giacomazzo, T. Goodale, C. Gundlach, R. Haas, I. Hawke, -% S. Hawley, I. Hinder, T. Kellermann, G. Lanfermann, F. L"{o}ffler, -% J. Masso, M. Miller, P. Montero, B. Mundim, C. Ott, R. Paruchuri, D. Pollney, -% T. Radke, L. Rezzolla, D. Rideout, M. Ripeanu, E. Schnetter, E. -% Seidel, E. L. Seidel, J. Shalf, N. Stergioulas, R. Takahashi, J. -% Thornburg, A. Tonita, P. Walker
%\thanks{{}$^{(1)}$ Department of Computer Science, % Louisiana State University, Baton Rouge, LA 70803, USA} %\thanks{{}$^{(2)}$ Department of Physics & Astronomy, @@ -244,7 +234,7 @@
This success prompted usage of the {\tt Cactus} computational toolkit in other areas, such as ocean forecast models \cite{Djikstra2005} and chemical reaction -simulations \cite{Camarada2001}. At the same time, the growing +simulations \cite{Camarda2001}. At the same time, the growing number of results in numerical relativity increased the need for commonly available utilities such as comparison and analysis tools, typically those specifically designed for astrophysical problems. Including them
File [modified]: plot_defaults.py Delta lines: +0 -1 =================================================================== --- plot_defaults.py 2011-10-28 01:52:58 UTC (rev 157) +++ plot_defaults.py 2011-11-06 03:53:03 UTC (rev 158) @@ -39,5 +39,4 @@ M_sol = 1.98892e30 # kg # convertion factors M_to_ms = 1./(1000*M_sol*G/(c*c*c)) -# fix this - what is 7e10? M_to_density = c*c*c*c*c*c / (G*G*G * M_sol*M_sol) # kg/m^3
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