[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 158)

[knarf at cct.lsu.edu]

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