<commit_before>\chapter*{Credits}

The Ames Stereo Pipeline was developed in the Intelligent Robotics
Group (IRG), a part of the Intelligent Systems Division at NASA Ames
Research Center in Moffett Field, CA.  It represents over ten years of
work leveraging IRG's extensive experience developing surface
reconstruction tools for terrestrial robotic field tests and planetary
exploration. \\ 

{\bf Lead Developer \& Project Lead:}
\begin {itemize} 
\item <NAME> (NASA/Carnegie Mellon University)\\ {\tt
  <EMAIL>})\\
\end{itemize}

{\bf Development Team:}
\begin{itemize}
\item <NAME> (NASA),
\item Dr. <NAME> (NASA)
\item Dr. <NAME> (NASA/SETI Institute)
\item <NAME> (Kansas State University)
\item Dr. <NAME> (NASA/Carnegie Mellon University)
\item <NAME> (NASA/Stinger-Ghaffarian Technologies)\\ 
\item <NAME> (NASA/Stinger-Ghaffarian Technologies)
\end{itemize}

A number of student interns have made substantial contributions to the
Stereo Pipeline over the years: <NAME> (Washington State
University), <NAME> (California Polytechnic Institute), <NAME> (Stanford University), <NAME> (Arizona State
University), <NAME> (Massachusetts Institute of Technology),
<NAME> (UC Berkeley), <NAME> (Bard Colege), <NAME>
(Standford University), and <NAME> (UC San Diego).

This version of the Stereo Pipeline is based on an earlier version of
the Stereo Pipeline written by <NAME>, <NAME>, and <NAME> of the Intelligent Systems Division at NASA Ames Research
Center.

\section*{Acknowledgements}

The initial adaptation of the stereo pipeline to orbital imagers was a
result of a NASA project led by Dr. <NAME> of Malin Space
Science Systems (MSSS) working in collaboration with Dr. <NAME> and <NAME> to develop automated Digital Elevation
Model generation techniques for the Mars Global Surveyor (MGS)
mission.  We thank <NAME>, <NAME>, and others at Malin
Space Science Systems for providing the seed funding that made the
current version of the Stereo Pipeline possible.

We'd also like to thank our friends and collaborators <NAME>,
<NAME>, <NAME>, and <NAME> of the USGS Astrology
Branch in Flagstaff, AZ for their encouragement and willingness to
share their experience and expertise by answering many of our
technical questions.  We also thank them for their ongoing effort to
help us evaluate our work.  Thanks also to the USGS ISIS team,
especially <NAME> and <NAME>, for their help in
intergrating the Stereo Pipeline with the USGS ISIS software package.

Thanks go also to <NAME>, <NAME>, <NAME>,
<NAME>, and <NAME> at Arizona State University for their
help in adapting the Stereo Pipeline to lunar data sets including the
Apollo Metric Camera.

Finally, we thank <NAME>, Dr. <NAME>, and <NAME> and
for their contributions to this documentation, and Dr. <NAME> (IRG
Group Lead) for his management and support of the open source \& public
software release process.

Portions of this software were developed with support from the
following NASA funding sources: the Mars Technology Program, the Mars
Critical Data Products Initiative, the Mars Reconnaissance Orbiter
mission, the Applied Information Systems Research program grant
\#06-AISRP06-0142, the Lunar Advanced Science and Exploration Research
(LASER) program grant \#07-LASER07-0148, and the ESMD Lunar Mapping and
Modeling Program.

\section*{Copyright and License}

This software and documentation is Copyright \copyright\ 2009 United
States Government as represented by the Administrator of the National
Aeronautics and Space Administration (NASA).  All Rights Reserved.

This software is distributed under the NASA Open Source Agreement
(NOSA), version 1.3.  The NOSA has been approved by the Open Source
Initiative.  See the file ``COPYING'' at the top of the distribution
directory tree for the complete NOSA document.

THE SUBJECT SOFTWARE IS PROVIDED "AS IS" WITHOUT ANY WARRANTY OF ANY
KIND, EITHER EXPRESSED, IMPLIED, OR STATUTORY, INCLUDING, BUT NOT
LIMITED TO, ANY WARRANTY THAT THE SUBJECT SOFTWARE WILL CONFORM TO
SPECIFICATIONS, ANY IMPLIED WARRANTIES OF MERCHANTABILITY, FITNESS FOR
A PARTICULAR PURPOSE, OR FREEDOM FROM INFRINGEMENT, ANY WARRANTY THAT
THE SUBJECT SOFTWARE WILL BE ERROR FREE, OR ANY WARRANTY THAT
DOCUMENTATION, IF PROVIDED, WILL CONFORM TO THE SUBJECT SOFTWARE.
<commit_msg>Changed the teaming lineup, minor word smithing, modified the Malin paragraph, made titles consistent, and corrected various typos.<commit_after>
\chapter*{Credits}

This open source version of the Ames Stereo Pipeline (OSP) was
developed by the Intelligent Robotics Group (IRG), in the Intelligent
Systems Division at NASA Ames Research Center in Moffett Field, CA. It
builds on over ten years of IRG experience developing surface
reconstruction tools for terrestrial robotic field tests and planetary
exploration. \\

{\bf Lead Developer \& IRG Project Lead:}
\begin {itemize} 
\item <NAME> (NASA/Carnegie Mellon University)\\ {\tt
  <EMAIL>})\\
\end{itemize}

{\bf Development Team:}
\begin{itemize}
\item <NAME> (NASA)
\item Dr. <NAME> (NASA/SETI Institute)
\item <NAME> (Kansas State University)
\item Dr. <NAME> (NASA/Carnegie Mellon University)
\item <NAME> (NASA/Stinger-Ghaffarian Technologies)\\ 
\item Vinh To (NASA/Stinger-Ghaffarian Technologies)
\end{itemize}

{\bf Contributing Developer \& Former IRG Terrain Reconstruction Lead:}
\begin{itemize}
\item Dr. <NAME> (NASA)
\end{itemize}

A number of student interns have made significant contributions to
this project over the years: <NAME> (Washington State
University), <NAME> (California Polytechnic Institute), <NAME> (Stanford University), <NAME> (Arizona State
University), <NAME> (Massachusetts Institute of Technology),
<NAME> (UC Berkeley), <NAME> (<NAME>), <NAME>
(Stanford University), and <NAME> (UC San Diego).

The open source stereo pipeline leverages stereo image processing
work, past and present, led by Dr. <NAME>, <NAME>
(formerly NASA/QSS Inc.), Dr. <NAME> (NASA), and others in the
Intelligent Systems Division at NASA Ames Research Center. It has
benefited substantially from the contributions of Dr. <NAME>
(formerly NASA/Stanford), <NAME> (NASA/Carnegie Mellon
University), Dr. <NAME> (formerly NASA/QSS Inc.), <NAME>
(formerly NASA/QSS Inc.), and Dr. <NAME> (NASA).

\section*{Acknowledgements}

The initial adaptation of Ames' stereo surface reconstruction tools to
orbital imagers was a result of a NASA funded, industry led, project
to develop automated Digital Elevation Model generation techniques for
the Mars Global Surveyor (MGS) mission. Our work with the project's
Principle Investigator, Dr. <NAME> of Malin Space Science
Systems (MSSS), and Co-Investigator, Dr. <NAME> of NASA
Ames, inspired the idea of making stereo surface reconstruction
technology available and accessible to a broader community.  We thank
Dr. Malin and Dr. Edwards for providing the initial impetus that in no
small way made this open source stereo pipeline possible, and we thank
Dr. <NAME>, <NAME> and others at MSSS for their help and
technical assistance.

We'd also like to thank our friends and collaborators Dr. <NAME>, Dr. <NAME>, <NAME>, and Dr. <NAME> of the USGS
Astrogeology Branch in Flagstaff, AZ for their encouragement and
willingness to share their experience and expertise by answering many
of our technical questions.  We also thank them for their ongoing
effort to help us evaluate our work.  Thanks also to the USGS ISIS
team, especially <NAME> and <NAME>, for their help in
integrating this version of the stereo pipeline with the USGS ISIS
software package.

Thanks go also to Prof. <NAME>, <NAME>, <NAME>, <NAME>, and <NAME> at Arizona State
University for their help in adapting the Ames' stereo pipeline to
lunar data sets including the Apollo Metric Camera.

Finally, we thank <NAME>, Dr. <NAME>, and Dr. Laurence
Edwards for their contributions to this documentation, and Dr. Terry
Fong (IRG Group Lead) for his management and support of the open
source \& public software release process.

Portions of this software were developed with support from the
following NASA funding sources: the Mars Technology Program, the Mars
Critical Data Products Initiative, the Mars Reconnaissance Orbiter
mission, the Applied Information Systems Research program grant
\#06-AISRP06-0142, the Lunar Advanced Science and Exploration Research
(LASER) program grant \#07-LASER07-0148, and the ESMD Lunar Mapping and
Modeling Program.

{'fraction_non_alphanumeric': 0.0736503396496246, 'fraction_numerical': 0.004528661661303778, 'mean_word_length': 5.050468637346792, 'pattern_counts': {'":': 0, '<': 87, '<?xml version=': 0, '>': 87, 'https://': 0, 'lorem ipsum': 0, 'www.': 0, 'xml': 0}, 'pii_count': 0, 'substrings_counts': 0, 'word_list_counts': {'cursed_substrings.json': 5, 'profanity_word_list.json': 0, 'sexual_word_list.json': 0, 'zh_pornsignals.json': 0}}
{'dir': 'git-commits-cleaned', 'id': '2337479', 'n_tokens_mistral': 2395, 'n_tokens_neox': 2210, 'n_words': 1176}