cometadata/test-preprints-extracted-funding huggingface dataset:
This work was supported by National Natural Science Foundation of China (No. 61906185), Youth Innovation Promotion Association of CAS China (No. 2020357), Shenzhen Science and Technology Innovation Program (Grant No. KQTD20190929172835662), Shenzhen Basic Research Foundation (No. JCYJ20210324115614039 and No. JCYJ20200109113441941). This work was supported by Alibaba Group through Alibaba Research Intern Program.
† Department of Mathematics, University College London, Gower Street, London WC1E 6BT, UK. Email: s.letzter @ ucl.ac.uk . Research supported by the Royal Society.
∗ Department of Mathematics, Faculty of Science, University of Zagreb, Croatia. Email: nina.kamcev@math.hr . Research supported by the European Union's Horizon 2020 research and innovation programme [MSCA GA No 101038085].
All authors except the last are supported by the Institute for Basic Science (IBS-R029-C1). The first author is supported by the Institute for Basic Science (IBS-R029-Y3) and in part by the Slovenian Research and Innovation Agency (research project N1-0370). The second author is also supported by the Australian Research Council. The third author is also supported by the National Research Foundation of Korea (NRF) grant funded by the Ministry of Science and ICT (No. NRF-2021K2A9A2A11101617 and RS-2023-00211670). The last author is partially supported by NSERC PGSD2-532637.
The authors would like to thank ´ Angel Castro for valuable discussions. This work has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program through the Consolidator Grant agreement 862342 (A.E.) and the Marie Curie Fellowship 101063565 (F.T.L.). It is partially supported by the grants CEX2019-000904-S, RED2018-102650-T and PID2019-106715GB GB-C21 (D.P.-S.) funded by MCIN/ AEI/10.13039/501100011033, and a Fields Ontario Postdoctoral Fellowship (F.T.L.) financed by the NSERC grant RGPIN-2019-05209. D.P.-S. and F.T.L. also acknowledge partial support from the grant 'Computational, dynamical and geometrical complexity in fluid dynamics', Ayudas Fundacion BBVA a Proyectos de Investigacion Cient´ ıfica 2021.
The authors would like to recognize the Air Force Office of Scientific Research (AFOSR) for financial support of this work under grant no. FA9550-21-1-0387. T.S. was partially funded by the U.S. Department of Energy (DOE) under grant no. DE-SC0019098. C.C., G.M., and T.W. gratefully acknowledge support from the Department of Energy, Basic Energy Sciences Division, under Award No. DEF-G02-08ER15983.
R. H. Guterres acknowledges support form FACEPE Grant BFP-0067-1.01/19. W. Melo acknowledges support from Bolsa PQ CNPq - 309880/2021-1. C.J. Niche acknowledges support from PROEX CAPES - UFRJ. C. F. Perusato was partially supported by CAPES PRINT88881.311964/2018-01.
Acknowledgments. I am very thankful to several colleagues who inspired me and motivated me to work on the topics presented in this paper, including: Myriam Benisty, Carsten Dominik, Nicolas Kurtovic, Feng Long, Antonella Natta, Luca Ricci, Aleks Scholz, and Leonardo Testi. In addition, thanks to Jun Hashimoto, Feng Long, and Nienke van der Marel for helping me to collect the ALMA observations presented in this paper. I also thank Mat´ ıas Garate for his help implementing the stellar evolution in Dustpy . I acknowledge support provided by the Alexander von Humboldt Foundation in the framework of the Sofja Kovalevskaja Award endowed by the Federal Ministry of Education and Research.
Acknowledgments This work was supported by the Institute of Information &amp; communications Technology Planning &amp; Evaluation (IITP) grant funded by the Korean government (MSIT) (No. 2019-0-00075, Artificial Intelligence Graduate School Program (KAIST) and No. 20210-01778, Development of human image synthesis and discrimination technology below the perceptual threshold) and the National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIT) (No. NRF2022R1A2B5B02001913).
Acknowledegments - The authors acknowledge fundings from the European Union's Horizon 2020 Research and Innovation programme under the Marie Sklodowska-Curie entitled STiBNite (N ◦ 956923), from the European Union's Horizon 2020 Research Project and Innovation Program - Graphene Flagship Core3 (N ◦ 881603), from the Federation Wallonie-Bruxelles through the ARC on Dynamically Reconfigurable Moire Materials (N ◦ 21/26-116), from the Flag-Era JTC projects 'TATTOOS' (N ◦ R.8010.19) and 'MINERVA' (N ◦ R.8006.21), from the EOS project 'CONNECT' (N ◦ 40007563) and from the Belgium F.R.S.-FNRS through the research project (N ◦ T.029.22F). Computational resources have been provided by the CISM supercomputing facilities of UCLouvain and the C ´ ECI consortium funded by F.R.S.-FNRS of Belgium (N ◦ 2.5020.11).
We acknowledge financial support from the German Research Foundation (CRC902: Molecular Principles of RNA Based Regulation) and the Max Planck Society. L.S.S thanks ReALity (Resilience, Adaptation and Longevity), M 3 ODEL(Mainz Institute of Multiscale Modeling) and Forschungsinitiative des Landes Rheinland-Pfalz for their support. Funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - Project number 233630050 - TRR 146.
The authors thank Olivier Pfister (University of Virginia) for useful discussions. This work is supported in part by the National Science Foundation (NSF) (OMA2138174, ECCS-1810169, ECCS-1842691), the Defense Threat Reduction Agency-Joint Science and Technology Office for Chemical and Biological Defense (grant No. HDTRA11810047), and the Defense Advanced Research Projects Agency (DARPA) LUMOS program under Agreement No. HR001-20-2-0044. This work was performed in part at the Cornell NanoScale Facility, a member of the National Nanotechnology Coordinated Infrastructure (NNCI), which is supported by the National Science Foundation (Grant NNCI-2025233).
The work of A.N. is supported by the grants PID2019-108122GB-C32 from the Spanish Ministry of Science and Innovation, Unit of Excellence Mar´ ıa de Maeztu 2020-2023 of ICCUB (CEX2019-000918-M) and AGAUR2017-SGR754. A.N. is grateful to the IFPU (SISSA, Trieste) and to the Physics Department of the University of Florence for the hospitality during the course of this work.
The authors thank Di Luo, Hong-ye Hu, and Pengyuan Bill Zhai for insightful discussion, Simone Colombo for pointing out how a QP can be used for time-reversal, and Bailey Renger, an intern researcher at Harvard University during the Spring of 2022 who tested the simulations in Sec. II C. RAB acknowledges support from National Science Foundation (NSF) Graduate Research Fellowship under Grant No. DGE1745303. XG kindly acknowledges support from the Harvard-MPQ Center for Quantum Optics, the Templeton Religion Trust (TRT) under Grant No. 0159, and by the Army Research Office under Grant No. W911NF1910302 and the Multidisciplinary University Research Initiative (MURI) under Grant No. W911NF-20-1-0082.SFY acknowledges funding from NSF Q-IDEAS HDR Institute, the Q-SeNSE QCLI and the CUA PFC, and the Air Force Office for Scientific Research (AFOSR).
CMCthanks the National Science Foundation for support through grants AST-1814034 and AST-2009577 as well as the University of Texas at Austin College of Natural Sciences for support; CMC also acknowledges support from the Research Corporation for Science Advancement from a 2019 Cottrell Scholar Award sponsored by IF/THEN, an initiative of Lyda Hill Philanthropies. JSK acknowledges support from the College of Science and the Laboratory for Multiwavelength Astrophysics at the Rochester Institute of Technology. JSK acknowledges the important contributions to this paper, and the COSMOS-Web proposal, made by Shran and T'Pol, who attended every planning telecon and kept everyone's spirits up in the early days of the COVID-19 pandemic.
Support for this work was provided by NASA through grant JWST-GO-01727 and HST-AR-15802 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140. JDR was supported by JPL, which is under a contract for NASA by Caltech. This research is also partly supported by the Centre National d'Etudes Spatiales (CNES). OI, CL, HHMCC acknowledge the funding of the French Agence Nationale de la Recherche for the project iMAGE (grant ANR-22-CE31-0007). BER was supported in part by NASA grant 80NSSC22K0814. MT and FG acknowledge the support from grant PRIN MIUR 2017 20173ML3WW 001. BT acknowledges support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement 950533) and from the Israel Science Foundation (grant 1849/19)
The authors acknowledge Research Computing at the Rochester Institute of Technology (2019) for providing computational resources and support for the work reported in this publication. This work used the CANDIDE computer system at the IAP supported by grants from the PNCG, CNES and the DIM-ACAV and maintained by S. Rouberol. We acknowledge use of the lux supercomputer at UC Santa Cruz, funded by NSF MRI
The authors thank Prof. Dion´ ısio Bazeia and Prof. Lukasz Stepien for motivating discussions. This work was financed in part by the Coordena¸ c˜ ao de Aperfei¸ coamento de Pessoal de N´ ıvel Superior -Brasil (CAPES) - Finance Code 001, the Conselho Nacional de Pesquisa e Desenvolvimento Cient´ ıfico e Tecnologico -CNPq and the Funda¸ c˜ ao de Amparo ` a Pesquisa e ao Desenvolvimento Cient´ ıfico e Tecnologico do Maranh˜ ao -FAPEMA (Brazilian agencies). In particular, J. A. and A. C. S. thank the full support from CAPES (via a PhD scholarship and a Postdoctoral fellowship, respectively), R. C. acknowledges the support from the grants CNPq/306724/2019-7, FAPEMA/Universal01131/17 and FAPEMA/Universal-00812/19, and E. H. thanks the support from the grant CNPq/309604/2020-6.
Acknowledgments. The authors thank A. Aggarwal, A. Auffinger, and A. Fribergh for helpful discussions. P.L. is partially supported by NSF postdoctoral fellowship DMS-220289. A.J. acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC). Cette recherche a ´ ete financee par le Conseil de recherches en sciences naturelles et en genie du Canada (CRSNG), [RGPIN-2020-04597, DGECR-2020-00199].
§ Corresponding author. Division of Mathematical Sciences, School of Physical and Mathematical Sciences, Nanyang Technological University, 637371, Singapore (lilian@ntu.edu.sg). The research of this author is partially supported by Singapore MOE AcRF Tier 1 Grant: MOE2021-T1-RG15/21.
† School of Mathematics and Statistics, Central South University, Changsha 410083, China (desongkong@csu.edu.cn, xiangsh@csu.edu.cn). The work of S. Xiang and D. Kong is supported by the National Natural Science Foundation of China (No. 12271528, No. 12001280). The first author is partially supported by the Fundamental Research Funds for the Central Universities of Central South University (No. 2020zzts031).
This research was supported in part by the National Natural Science Foundation of China (Nos. 62002136 and 62272196), Natural Science Foundation of Guangdong Province (No. 2022A1515011861), Guangzhou Basic and Applied Basic Research Foundation (No. 202102020277), Fundamental Research Funds for the Central Universities of Jinan University (No. 21622416), and the Young Scholar Program of Pazhou Lab (No. PZL2021KF0023). Dr. Wensheng Gan is the corresponding author of this paper.
We thank Prof. Ido Kaminer for useful discussions. J.S. acknowledges support a Mathworks fellowship, as well as ear-
lier support from a National Defense Science and Engineering Graduate Fellowship of the Department of Defense (F1730184536). N.R. acknowledges the support of a Junior Fellowship from the Harvard Society of Fellows, as well as earlier support from a Computational Science Graduate Fellowship of the Department of Energy (DE-FG02-97ER25308), and a Dean's Fellowship from the MIT School of Science. This material is based on work supported in part by the Defense Advanced Research Projects Agency (DARPA) under agreement no. HR00112090081. This material is based upon work supported in part by the Air Force Office of Scientific Research under the award number FA9550-20-1-0115; the work is also supported in part by the U. S. Army Research Office through the Institute for Soldier Nanotechnologies at MIT, under Collaborative Agreement Number W911NF-182-0048.
Work partially supported by the DOR funds and the biennial project BIRD 192932 of the University of Padova, and by the INdAM-GNCS 2022 Project 'Methods and software for multivariate integral models'. This research has been accomplished within the RITA 'Research ITalian network on Approximation', and within the UMI Group TAA 'Approximation Theory and Applications' (A. Sommariva).
∗ Jiahui Cheng and Minshuo Chen contributed equally to this work. Jiahui Cheng and Wenjing Liao are affiliated with the School of Mathematics at Georgia Institute of Technology. Minshuo Chen is affiliated with the Department of Electrical and Computer Engineering at Princeton University. Hao Liu is affiliated with the Department of Mathematics at Hong Kong Baptist University. Tuo Zhao is affiliated with the School of Industrial and Systems Engineering at Georgia Institute of Technology. Email: { jcheng328,tourzhao,wliao60 } @gatech.edu, mc0750@princeton.edu, haoliu@hkbu.edu.hk. This research is partially supported by NSF DMS 2012652 and NSF CAREER 2145167.
The authors are very grateful to Dr. Sef Tongay for his kind invitation and inspiration for this focused review, and to Dr. Yu Zheng, Dr. Lei Liu, Dr. Duo Wang, Chia-Hao Lee, Dr. Sangmin Kang, Dr. Wenjuan Zhu, Xinyu Jiang, Yu Liu, Justine Ilyssa Vidallon for their contributions to the work on disordered solid-state materials discussed in this review, and to Dr. Sal Torquato, Dr. Ge Zhang, and Dr. Jaeuk Kim for very helpful discussions. Y. J. was supported by the Army Research Office under Cooperative Agreement Number W911NF-22-2-0103. P. H. was supported by U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under award number DE-SC0020190
MCA06N030), NASA TCAN award 80NSSC21K1053, and the Simons Foundation (grant 822237). ECO and CGK acknowledge support from the Simons Foundation (888968). CGK acknowledges support from NASA ATP award 80NSSC22K0717. This work was supported by the Simons Collaboration on 'Learning the Universe'
UPS thanks Matt Orr, Viraj Pandya, Eliot Quataert and Romain Teyssier for helpful discussions. UPS thanks Daniel J. Price for making the software splash publicly available (Price 2007). UPS acknowledges the computing time provided on SuperMuc-NG in Garching under the project number pn72bu. RSS is supported by the Simons Foundation. GLB acknowledges support from the NSF (AST-2108470, XSEDE grant budget as in our simulations hot and warm mass and energy loading are more similar to one another than in Kim et al. (2020a) and Fielding et al. (2018).
1 I am grateful to Lawrence Wong, Bartosz Wcis/suppress lo, Mateusz /suppress Le/suppress lyk, Jim Schmerl, Roman Kossak, Kentaro Fujimoto, Cezary Cieslinski, Lev Beklemishev, and Athar Abdul-Quader (in reverse alphabetical order) for their feedback and keen interest in this work. The research presented in this paper was partially supported by the National Science Centre, Poland (NCN), grant number 2019/34/A/HS1/00399.
Acknowledgements We thank Drs L. N. Wu, Y. Q. Zou, X. Y. Luo, J. L. Yu, M. Xue and S. F. Guo for helpful discussions. This work is supported by the National Natural Science Foundation of China (NSFC) (Grants No. 11654001 and No. U1930201), by Natural Science Foundation of Zhejiang Province (Grant No. LY22A050002), by the Key-Area Research and Development Program of GuangDong Province (Grant No. 2019B030330001), and by the National Key R&amp;D Program of China (Grants No. 2018YFA0306504 and No. 2018YFA0306503).
We thank Prof. Wenhui Duan and Xingxing Li for discussion of evaluation of MAE. We thank Doctor Rui Li for discussion of orbital-resolved MAE. We thank doctor Yang Li for discussion of LDA+U. This work was supported by the financial support from the Natural Science Foundation of China (Grant No. 11904203), and the Fundamental Research Funds of Shandong University (Grant No. 2019GN065). The authors are grateful to Beijing PARATERA Tech Corp., Ltd. for the computation resource in the National Supercomputer Center of Guangzhou. The scientific calculations in this paper have been done on the HPC Cloud Platform of Shandong University. The authors also acknowledge the Beijing Super Cloud Computing Center (BSCC), Shanghai Supercomputer Center and Tencent Quantum Laboratory for providing HPC resources.
The work of W. K. New, K.-K. Wong and K.-F. Tong is supported by the Engineering and Physical Sciences Research Council (EPSRC) under grant EP/W026813/1. The work of C.-B. Chae is supported by the Institute for Information and Communication Technology Promotion (IITP) grant funded by the Ministry of Science and ICT (MSIT), Korea (No. 2021-0-02208, No. 20210-00486). The work of H. Xu is supported by the European Union's Horizon 2020 Research and Innovation Programme under Marie Sklodowska-Curie Grant No. 101024636.
∗ Prepared for the Conference in Honor of James L. Powell at UC Berkeley, March 25-26, 2022. We thank the conference participants for their comments, as well as two reviewers, an Associate Editor, and co-Editor Elie Tamer for their feedback. Cattaneo gratefully acknowledges financial support from the National Science Foundation through grants SES-1947805 and DMS-2210561, Jansson gratefully acknowledges financial support from the National Science Foundation through grant SES-1947662, and Masini gratefully acknowledges financial support from the National Science Foundation through grant DMS-2210561.
The authors thank Marco Lopes for his support during the fabrication and measurement of these samples. The sample fabrication and project coordination were funded by the Swiss National Science Foundation through an Ambizione Fellowship (#PZ00P2_185848). The oxide growth was supported by the European Research Council under the European Union's Seventh Framework Program (FP7/2007-2013)/ERC Grant Agreement 319286 Q-MAC and the Swiss National Science Foundation Project no. 200020-179155. W.R. was supported by the U.S. Office of Naval Research through the NICOP Grant N62909-21-1-2028. s-SNOM measurements were supported by the Swiss National Science Foundation through a Research Grant #200020_201096. Simulations were funded by the French ANR project "MoMA" ANR-19-CE30-0020. T. L. acknowledges support by the Cusanuswerk, Bischöfliche Studienförderung. J.d.V acknowledges support from the Spanish Ministry of Science through a Ramón y Cajal Fellowship (#RYC2021030952-I).
IN was supported in part by the Simons Foundation Investigator program, the Simons-Emory Consortium on Motor Control, NSF grant BCS/1822677 and NIH grant 2R01NS084844. AS was supported in part by NIH grant 1RF1MH130413-01 and by startup funds from the University of Minnesota Medical School. The authors acknowledge the Minnesota Supercomputing Institute (MSI) at the University of Minnesota for providing resources that contributed to the research results reported within this paper.
The views and opinions expressed herein do not necessarily reflect those of the ITER organization. This work was supported by DOE SciDAC ISEP, INCITE, and the ITPA-EP group. This material is based upon work supported by the U.S. DOE, Office of Science, Office of Fusion Energy Sciences, using the DIII-D National Fusion Facility, a DOE Office of Science user facility, under Award(s) DE-FC02-04ER54698, as well as computing resources from ORNL (DOE Contract DE-AC05-00OR22725), NERSC (DOE Contract DE- AC02-05CH11231), and PPPL (DOE Contract DE-AC02-09CH11466).
This work is financially supported by the National Key R&amp;D Program of China, Project Number 2021YFA1002800 and Number 2020YFA0712000. The work of L. Li was partially
supported by NSFC 12371400 and 12031013, Shanghai Municipal Science and Technology Major Project 2021SHZDZX0102, Shanghai Science and Technology Commission (Grant No. 21JC1403700, 21JC1402900). The work of J.-G. Liu was partially supported by NSF DMS-2106988.
The author would like to thank Dominik Wrazidlo for posing the problem, stimulating discussions and giving important comments about an earlier version of the paper, which drastically improved the presentation of the paper. The author has been supported in part by JSPS KAKENHI Grant Numbers JP17H06128, JP22K18267. This work was also supported by the Research Institute for Mathematical Sciences, an International Joint Usage/Research Center located in Kyoto University. Finally, the author would like to express his hearty thanks to Professor Maria Aparecida Soares Ruas for her energetic and constant encouragement.
Research was carried out at the HERMES beamline of Synchrotron SOLEIL. We acknowledge SOLEIL for providing development beamtime for this research. We thank the staff of SOLEIL for their support, in particular Arafat Noureddine for his help with the camera control. We especially thank A. Besson and J.-B. Boy for their technical support, E. Fahri and F.-E. Picca for the computing support, and K. Medjoubi for his help with the reconstruction and fruitful discussions. This work was partially funded by project EU-H2020 of the Nanoscience Foundries and Fine Analysis (NFFA) program. Participation of the Canadian group was supported by the Natural Science and Engineering Research Council of Canada and funding from the Faculty of Science of McMaster University. The authors wish to acknowledge Laura Alvara Gomez, Lucas Perez from Department of Fisica de Materiales, Universidad Complutense de Madrid, Madrid Spain and IMDEA Nanosciencia, Madrid, Spain; Oliver Fruchart from Spintec (University Grenoble Alpes, CNRS, CEA), Grenoble, France for providing the permalloy nanorods. The authors also acknowledge and thank the group of Simard (NRC) for providing the CNT#1 sample and Dr. Carla Bittencourt for providing the BN nanobamboo sample.
We are thankful to A. V. Rodina, E. L. Ivchenko, M. O. Nestoklon, M. M. Glazov, and I. V. Kalitukha for fruitful discussions. We acknowledge the financial support by the Deutsche Forschungsgemeinschaft in the frame of
the Priority Programme SPP 2196 (Project YA 65/261) and the International Collaboration Research Center TRR160 (Projects A1 and B2). The work of O.H. and M.V.K. was financially supported by the Swiss National Science Foundation (grant agreement 186406, funded in conjunction with SPP2196 through DFG-SNSF bilateral program) and by the ETH Z¨ urich through the ETH+ Project SynMatLab: Laboratory for Multiscale Materials Synthesis.
A. Rotenberg, W. Huleihel and O. Shayevitz are with the Department of Electrical EngineeringSystems at Tel Aviv university, Tel Aviv 6997801, Israel (e-mail: asaf.rotenberg@gmail.com, wasimh@tauex.tau.ac.il, ofersha@tauex.tau.ac.il ). The work of A. Rotenberg was supported by the ISRAEL SCIENCE FOUNDATION (grants No. 1734/21 and 1766/22). The work of W. Huleihel was supported by the ISRAEL SCIENCE FOUNDATION (grants No. 1734/21). The work of O. Shayevitz was supported by the ISRAEL SCIENCE FOUNDATION (grant No. 1766/22). This paper was presented in part at the 2023 IEEE International Symposium on Information Theory, Taipei, Taiwan.