Editing Appendix/References (section)

===Decade9===
====TH90====

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<tr><td align="left">Acknowledgements (p. 406):<br /><font color="darkgreen">"We wish to acknowledge useful discussions that we have had on this topic with R. Durisen, J. Frank, J. Goodman, J. Pringle, and B. Schutz.  Most of the text of this paper was written while J. E. T. was visiting the Physics Department of the University of Wales/College of Cardiff and the Department of Aeronautical Engineering at Kyoto University; the hospitality that was extended to him by the staff at both of these institutions is greatly appreciated.  The extensive computational work required for this study was conducted, in part, at Louisiana State University's System Network Computer Center and, in part, using the Cornell National Supercomputer Facility, a resource of the Center for Theory and Simulation in Science and Engineering at Cornell University, which is funded in part by the National Science Foundation, New York State, and the IBM Corporation.  The graphics and imaging tasks that have provided an essential diagnostic tool for the present study would not have been successfully completed at L.S.U. without the continuous efforts of M. Lee and J. Anderson and without the facilities provided by a grant to L.S.U. through A. Landolt by the U.S. Air Force Office of Scientific Research.  J. E. T. was supported in part by the U. S. National Science Foundation through grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=8701503 AST 87-01503] and I. H. was financially supported in part by a Grant-in-Aid for Scientific Research of the Ministry of Education, Science, and Culture of Japan (No. 63540196)."</font>
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<tr><td align="left">Acknowledgements:&nbsp; n/a
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<tr><td align="left">Acknowledgements (p. L66):<br /><font color="darkgreen">"We thank L. Bildsten, J. Goodman, K. Thorne, and C. Will for useful discussions.  This work was supported in part by NSF grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9119475 AST 91-19475] and NASA Grant NAGW-2364 to Cornell University.  Partial support was also provided by NASA through Grant HF-1037.01-92A awarded by the Space Telescope Science Institute which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract NAS5-26555."</font>
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<tr><td align="left">Acknowledgements (p. 248):<br /><font color="darkgreen">"This work was supported by NSF grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9015451 AST 90-15451] and NASA grant NAGW-2364 to Cornell University.  Partial support was also provided by NASA through grant HF-1037.01-92A awarded by the Space Telescope Science Institute which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract NAS5-26555.  Computations were performed on the Cornell National Supercomputer Facility, a resource of the Center for Theory and Simulation in Science and Engineering at Cornell University, which receives major funding from the NSF and from the IBM Corporation, with additional support from New York State and members of its Corporate Research Institute."</font>
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====WTH94====

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<tr><td align="left">Acknowledgements (p. 265):<br /><font color="darkgreen">"This work has been supported in part by the US National Science Foundation through grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=8701503 AST-8701503] and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9008166 AST-9008166], and in part by NASA through grant NAGW-2447.  The extensive computational work required for this study has been conducted primarily at the Cornell National Supercomputer Facility, a resource of the Center for Theory and Simulation in Science and Engineering at Cornell University, which is funded in part by the National Science Foundation, New York State, and the IBM Corporation."</font>
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<tr><td align="left">Acknowledgements (p. 495):<br /><font color="darkgreen">
"We thank M. Ando, J. Brill, D. Brydges, B. Deaver, Jr., M. Elitzur, G. Hess, P. Mannheim, Q. Shafi, and J. Straley for stimulating discussions and I. Hachisu and N. Lebovitz for useful correspondence.  We are especially grateful to C. McKee and to R. Narayan for in-depth discussions of the physical concepts presented in this paper.  We are indebted to the graphics department of NRAO for assistance in producing Figure 3.  I. S. is grateful to the Gauss Foundation for support and to K. Fricke, director of Universit&auml;ts-Sternwarte G&ouml;ttingen, for hospitality during a stay in which much of this work has been accomplished.  I. S. also thanks the Center for Computational Studies of the University of Kentucky for continuing support.  This work was supported in part by NASA grants NAGW-1510, NAGW-2447, NAGW-2376, and NAGW-3839, by NSF grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9008166 AST 90-08166], and by grants from the San Diego Supercomputer Center and the National Center for Supercomputing Applications.</font>
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<tr><td align="left">Acknowledgements (p. 519):<br /><font color="darkgreen">
"We thank C. McKee and R. Narayan for stimulating discussions and I. Hachisu and N. Lebovitz for useful correspondence.  We also thank the main referee of this series of papers for comments that led to improvements in the presentation of results.  I. S. is grateful to the Gauss Foundation for support and to K. Fricke, director of Universit&auml;ts-Sternwarte G&ouml;ttingen, for hospitality during a stay in which much of this work has been accomplished.  I. S. also thanks the Center for Computational Studies of the University of Kentucky for continuing support.  This work was supported in part by NASA grants NAGW-1510, NAGW-2447, NAGW-2376, and NAGW-3839, by NSF grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9008166 AST 90-08166], and grants from the San Diego Supercomputer Center and the National Center for Supercomputing Applications.</font>
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====KP96====
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<tr><td align="left">Acknowledgements (p. 190):<br /><font color="darkgreen">"This work was partially supported by PPARC grant No. GR/H/09454.  D. G. K. would like to thank UCO/Lick Observatories for its hospitality and support and acknowledge a special NASA Astrophysical Theory program that supports a joint Center for Star Formation Studies at NASA Ames Research Center, UC Berkeley, and UC Santa [C]ruz.  Support was also provided by NASA Grant NAGW 3599 and NSF grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=8022876 AST-93-15578]."</font>
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<tr><td align="left">Acknowledgements (p. 712):<br /><font color="darkgreen">"The research reported here was supported by the National Science Foundation through grants DMS 9207808</font> [should be, [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9207080 DMS 9207080]] <font color="darkgreen">with the University of Chicago (N. R. L.) and IRI 9924605 with the University of Illinois at Chicago (A. L.)."</font>
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<tr><td align="left">Acknowledgements (p. 946):<br /><font color="darkgreen">"We thank Peter Constantin, David Livermore and Carlos Kenig for their advice and help.  This work was supported by the National Science Foundation through grants number [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9207080 DMS9207080] with the University of Chicago (N. R. L.) and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9924605 IRI9924605] with the University of Illinois at Chicago (A. L.)."</font>
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<tr><td align="left">Acknowledgements (p. 737):<br /><font color="darkgreen">"The authors thank M. S. Johnson for preparing animations of the <math>n' = 0.0, ~T/|W|=0.327</math> and <math>n' = 2.0, ~T/|W|=0.207</math> calculations.  These animations and other related images can be viewed via the World Wide Web at [https://enif.astro.indiana.edu/personnel/pickettb/picts.html <https://enif.astro.indiana.edu/personnel/pickettb/picts.html>].  This work is supported by NASA Grant NAGW-3399.  R. H. D. thanks the Max Planck Institute for Extraterrestrial Physics, where he was a Fulbright Scholar and a visiting scientist during portions of this research.  The authors would also like to thank F. C. Adams, P. Bodenheimer, A. P. Boss, A. Burkett, P. Cassen, D. M. Christodoulou, F. H. Shu, I. Hachisu, T. W. Hartquist, J. N. Imamura, D. N. C. Lin, G. E. Morfill, T. Y. Steiman-Cameron, J. E. Tohline, H. A. Williams, S. Yank, and C. Yuan for useful encouragement and support for this research over the years.  Some of the calculations were completed using Cray Y/MP time at the National Center for Supercomputing Applications."</font>
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<tr><td align="left">Acknowledgements (pp. 326 - 327):<br /><font color="darkgreen">"This work has been supported, in part, by funding from the National Science Foundation through grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9008166 AST 90-08166], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9528424 AST 95-28424], and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9208914 PHY 92-08914], from NASA through grants NAGW-2447 and NAG 5-2777, from the Louisiana State Board of Regents through grant LEQSF(1995-1998)-115-35-4412, from the Baton Rouge, Louisiana Branch of the American Association of University Women through a Doctoral Candidate Scholarship, and by computational resources from the Pittsburgh Supercomputing Center through grant PHY 91-0018P.  The great majority of the numerical simulations presented herein were carried out on computers in the Department of Physics and Astronomy's Concurrent Computing Laboratory for Materials Simulation, which was established through grants LEQSF(1990-92)-ENH-12 and LEQSF(1993-94)-ENH-TR05 from the Louisiana State Board of Regents.  Several of the numerical simulations also were carried out at the Scalable Computing Laboratory of the Department of Energy Ames Laboratory at Iowa State University.  We would also like to thank Joan Centrella, Dimitris Christodoulou, Greg Cook, Dong Lai, Dustin Laurence, Kip Thorne, and Horst V&auml;th for useful conversations and assistance."</font>
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<tr><td align="left">Acknowledgements (p. 833):<br /><font color="darkgreen">"JF thanks the Institute of Astronomy, Cambridge, for its hospitality during the completion of this paper.  PPE and RCC are grateful to the Institute of Theoretical Physics, Santa Barbara (NSF grant PH489-04035)</font> [should be [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=8904035 PHY-8904035]] <font color="darkgreen">for its hospitality at an earlier stage."</font>
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<tr><td align="left">Acknowledgements (p. 99):<br /><font color="darkgreen">"We are grateful to Dana Browne and his suggestion in 1994 to use a Gauss-Legendre integrator, which motivated our search for an analytic solution to the infinite integral.  Thanks to John Cazes for incorporating and optimizing the CCGF technique in the HPF version of our CFD code.  Thanks to Patrick Motl for his optimizing suggestion, which sped up the initialization part of the CCGF code drastically, as well as for implementing the CCGF technique in Fortran 90 with MPI.  Thanks to Eric Barnes for motivational discussions on coordinate systems.  We acknowledge support from the US National Science Foundation through grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9528424 AST-9528424] and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9355007 DGE-9355007], the latter of which has been issued through the NSF's Graduate Traineeships Program and from NASA through grant NAG5-8497.  This work also has been supported, in part, by grants of high-performance computing time on NPACI facilities at SDSC and UT, Austin, and through the PET program of NAVOCEANO DoD Major Shared Resource Center in Stennis, MS."</font>
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<tr><td align="left">Acknowledgements (p. 810):<br /><font color="darkgreen">"The author is grateful to J. Fanselow for support during the early development of this work, to L. Caroff and M. Bicay at NASA for allowing a small portion of a theoretical astrophysics grant to be used for this purpose, and to the JPL Director's Research and Development Fund for support to complete this work.  Discussions with numerous people were very helpful, including G. Lozenge and A. Raefsky on the finite element method, M. Norman on adaptive gridding, P. Godon on spectral methods and multigrain methods, and W. Cannon, S. Finn, M. Holst, K. Thorne, and J. York on the use of these techniques for general relativity.  This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, and under contract to the National Aeronautics and Space Administration."</font>
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