[Hadstruct] Correct Funding Sources in Acknowledgments
Colin Egerer
cegerer at jlab.org
Tue Mar 7 17:05:09 EST 2023
Hi All,
I am about to submit the final proofs for the quark helicity draft. Before doing so, I wanted to ensure all funding sources were correct.
I have pasted the relevant section from our draft below. Please check your funding source is correct. I will submit the final proofs tomorrow afternoon. Otherwise, the paper is accepted and will be published.
All members of the HadStruc collaboration are thanked for their support and fruitful and
stimulating exchanges. The authors thank J. Green for constructive feedback on an initial
version of this manuscript. This material is based upon work supported by the U.S. De-
partment of Energy, Office of Science, Office of Nuclear Physics under contract DE-AC05-
06OR23177. JK is supported by U.S. DOE grant #DE-SC0011941. NK, KO, and RSS
are also supported by U.S. DOE Grant #DE-FG02-04ER41302. AR and WM are also
supported by U.S. DOE Grant #DE-FG02-97ER41028. CJM is supported by U.S.
DOE Grant #DE-SC0023047. We acknowledge the facilities of the USQCD Collab-
oration used for this research in part, which are funded by the Office of Science of the U.S.
Department of Energy. This work used the Extreme Science and Engineering Discovery En-
vironment (XSEDE), which is supported by the National Science Foundation under Grant
No. ACI- 1548562 [221]. We further acknowledge the Texas Advanced Computing Center
(TACC) at the University of Texas at Austin for HPC resources on Frontera [222] that
have contributed greatly to the results in this work. We gratefully acknowledge computing
cycles provided by facilities at William and Mary, which were provided by contributions
from the National Science Foundation (MRI Grant No. PHY-1626177), and the Common-
wealth of Virginia Equipment Trust Fund. The authors acknowledge William and Mary
Research Computing for providing computational resources and/or technical support that
have contributed to the results reported within this paper.
This work was furthermore made possible using results obtained at NERSC, a DOE
Office of Science User Facility supported by the Office of Science of the U.S. Department of
Energy under Contract No. DE-AC02-05CH11231, as well as resources of the Oak Ridge
Leadership Computing Facility (ALCC and INCITE) at the Oak Ridge National Labora-
tory, which is supported by the Office of Science of the U.S. Department of Energy under
Contract No. DE-AC05-00OR22725. Calculations were performed using the Chroma [223],
QUDA [224, 225], QDP-JIT [226], and QPhiX [227, 228] software libraries which were de-
veloped with support from the U.S. Department of Energy, Office of Science, Office of
Advanced Scientific Computing Research and Office of Nuclear Physics, Scientific Discov-
ery through Advanced Computing (SciDAC) program. This research was also supported
by the Exascale Computing Project No. (17-SC-20-SC), a collaborative effort of the U.S.
Department of Energy Office of Science and the National Nuclear Security Administration.
We acknowledge PRACE (Partnership for Advanced Computing in Europe) for award-
ing us access to the high performance computing system Marconi100 at CINECA (Con-
sorzio Interuniversitario per il Calcolo Automatico dell’Italia Nord-orientale) under the
grant 2021240076. Results were obtained also by using Piz Daint at Centro Svizzero di
Calcolo Scientifico (CSCS), via the project with ID s994. We thank the staff of CSCS for
access to the computational resources and for their support. This work also benefited from
access to the Jean Zay supercomputer at the Institute for Development and Resources in
Intensive Scientific Computing (IDRIS) in Orsay, France under project No. A0080511504.
Thanks,
Colin
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