cometadata/test-preprints-extracted-funding huggingface dataset:
B.-H. Hwang was supported by Basic Science Research Program through the National Research Foundation of Korea(NRF) funded by the Ministry of Education (No. NRF2019R1A6A1A10073079). S.-B. Yun was supported by Basic Science Research Program through the National Research Foundation of Korea(NRF) funded by the Ministry of Education (No. NRF-2023R1A2C1005737).
M.B. and Y.D. would like to thank Hessam Babaee and Simon Kern for discussions about the OTD modes. Financial support by the Swedish Research Council (VR) grant no. 2016-03541 is gratefully acknowledged. The computations were enabled by resources provided by the Swedish National Infrastructure for Computing (SNIC) partially funded by the Swedish Research Council through grant agreement no. 2018-05973. The authors report no conflict of interest.
The authors would like to thank to VR-1 staff headed by F. Fejt for their effective help during the experiments and for the precise monitoring of the reactor power. The VR-1 operation was supported by LM2018118 project: VR-1 - Support for reactor operation for research activities, which was granted by The Ministry of Education, Youth and Sports of the Czech Republic.
The presented work was financially supported by the Project CZ.02.1.01/0.0/0.0/15_008/0000293: Sustainable energy (SUSEN) - 2nd phase, realized in the framework of the European Structural and Investment Funds and with use of infrastructures Reactors LVR-15 and LR-0, which were financially supported by the Ministry of Education, Youth and Sports - projects LM2015093 and LM2015074.
The authors would like to thank Prof. Junjie Mao (Tsinghua University) and Prof. B. Luo (Nanjing University) for helpful discussions. This work was supported in part by the Ministry of Science and Technology of China through Grant 2018YFA0404502 and the National Natural Science Foundation of China through Grants E3GJ251110 and 11821303. RH acknowledges support from the China Scholarship Council. GP acknowledges funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 865637) and from 'Bando per il Finanziamento della Ricerca Fondamentale 2022 dell'Istituto Nazionale di Astrofisica (INAF): Canale: GO Large program'
This work was supported by the National Key Research and Development Program of China (No. 2017YFA0304100, 2024YFA1409403), the National Natural Science Foundation of China (Grant No. 11774335, No. 11734015, and No. 12204455), the Key Research Program of Frontier Sciences, CAS (Grant No. QYZDYSSWSLH003), and the Innovation Program for Quantum Science and Technology (Grant No. 2021ZD0301604 and No. 2021ZD0301200).
DP was partially supported by the ERC Advanced Grant 'ERMiD' and by the Janos Bolyai Research Scholarship of the Hungarian Academy of Sciences, and by the New National Excellence Program ´ UNKP-22-5 and by the Thematic Excellence Program TKP2021-NKTA-62 of the National Research, Development and Innovation Office.
Patkos's research is partially supported by NKFIH grants SNN 129364 and FK 132060.
This work was partially supported by National Nature Science Foundation of China (62372155 and 32371877), Aeronautical Science Fund (2022Z071108001), Joint Fund of Ministry of Education for Equipment Pre-research (8091B022123), Water Science and Technology Project of Jiangsu Province under grant No. 2021063, Technology Winter Olympics Special Project (201001D) Forest Fire Comprehensive System Construction-Unmanned Aerial Patrol Monitoring System of Chongli (DA2-20001), and Qinglan Project of Jiangsu Province.
Acknowledgements S. V. thanks the Max Planck Society for support through a Max Planck Lise Meitner Group and funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (LEDA: grant agreement No 758853). G. V. has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodovska-Curie grant agreement No 897124. G. D. was supported by a Gliese Fellowship. C. D. F acknowledges support for this work from the National Science Foundation under Grant No. AST-1715611. D. G. was partially supported by a HQP grant from the McDonald Institute (reference number HQP 2019-4-2). Y. H. and L. P. are supported by a generous donation by Eric and Wendy Schmidt with the recommendation of the Schmidt Futures Foundation, as well as the National Sciences and Engineering Council of Canada, the Fonds de recherche du Québec, and the Canada Research Chairs Program. J. P. M. acknowledges support from the Netherlands Organization for Scientific Research (NWO, project number 629.001.023) and the Chinese Academy of Sciences (CAS, project number 114A11KYSB20170054).
We thank the anonymous referee for detailed comments, which were useful to improve the clarity of the manuscript. This work has been supported by the Basic Science Research Program through the National Research Foundation of the Korean Government (grant No. NRF-2021R1A2C3008486). A.A. acknowledges support from China Scholarship Council for the Ph.D. Program (No. 2017SLJ021244). S.R. acknowledges the partial support of SRG-SERB, DST, New Delhi through grant no. SRG/2021/001334.
† Department of Mathematics, University of Florida, Gainesville, FL 32611 (chunmei.wang@ufl.edu). The research of Chunmei Wang was partially supported by National Science Foundation Grants DMS-2136380 and DMS-2206332.
‡ Division of Mathematical Sciences, National Science Foundation, Alexandria, VA 22314 (jwang@nsf.gov). The research of Junping Wang was supported by the NSF IR/D program, while working at National Science Foundation. However, any opinion, finding, and conclusions or recommendations expressed in this material are those of the author and do not necessarily reflect the views of the National Science Foundation.
∗ Jiangsu Key Laboratory for NSLSCS, School of Mathematical Sciences, Nanjing Normal University, Nanjing 210023, China (danlimath@163.com). The research of Dan Li was supported by Jiangsu Funding Program for Excellent Postdoctoral Talent and China National Natural Science Foundation Grant (No. 12071227).
We would like to thank Jing Liu, Tao Xu and Daneng Yang for the very useful discussions. This work was supported by the National Natural Science Foundation of China (NNSFC) under grant Nos. 12105118, 11947118 11821505, 12075300 and 1233500, by Peng-Huan-Wu Theoretical Physics Innovation Center (12047503), and by the Key Research Program of the Chinese Academy of Sciences, grant No. XDPB15. CH acknowledges support from the Sun Yat-Sen University Science Foundation and the Fundamental Research Funds for the Central Universities, Sun Yat-sen University under Grant No. 23qnpy58.
Acknowledgments: We thank members of the LIGO Suspension Working Group for useful discussions. J.S. and D. M. acknowledge the support of the Institute for Gravitational Wave Astronomy at the University of Birmingham, STFC Quantum Technology for Fundamental Physics schemes (Grant No. ST/T006609/1 and ST/W006375/1), and EPSRC New Investigator Award (Grant No. EP/V008617/1). D.M. is supported by the 2021 Philip Leverhulme Prize.
Funding: This research was funded by STFC grant numbers ST/T006609/1 and ST/W006375/1 and EPSRC grant numbers EP/V008617/1.
The authors thank the Science and Engineering Research Board (CRG/2019/002808); the Department of Science and Technology, Ministry of Science and Technology, India (DST-FIST project (PSI195/2014) for financial support. Istvan Csarnovics acknowledges the János Bolyai Research Scholarship from the Hungarian Academy of Sciences (BO/348/20). The New National Excellence Program's ÚNKP-22-3-II-DE-53 and ÚNKP-22-5-DE-407 also provided support from the National Research, Development, and Innovation Fund. The US National Science Foundation is acknowledged for supporting (DMR-2123131) this international collaboration that was established through International Materials Institute for New Functionality in Glass (DMR-0844014)
This work derived from the thesis entitled 'Residuals and diagnostic methods in models for polytomous data' with support from the Brazilian Foundation, Coordena¸ c˜ ao de 'Coordena¸ c˜ ao de Aperfei¸ coamento de Pessoal de N´ ıvel Superior' (CAPES) process number 88882 . 378344 / 2019 -01. This publication also had the additional support from Brazilian Fundation-CAPES process number 88887 . 716582 / 2022 -00 and from Science Foundation Ireland under grant number 18 /CRT/ 6049.
The authors gratefully acknowledge financial support through the German Research Association and the Spanish Ministry of Science. Matthias Eckardt was funded by the Walter Benjamin grant 467634837 from the German Research Foundation. Jorge Mateu was partially funded by grant PID2019-107392RB-I00, from the Spanish Ministry of Science. Carles Comas was partially funded by grant PID2020-115442RB-I00 from MCIN/AEI/ 10.13039/501100011033 (Spanish Ministry of Science)
Michael Zevin for helpful discussions. Y.D. is supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE-1842165. T.E. is supported by NASA through the NASA Hubble Fellowship grant HST-HF2-51504.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS526555. S.B. is supported by the Dutch Research Council (NWO) Veni Fellowship (VI.Veni.212.058). W.F. gratefully acknowledges support by the David and Lucile Packard Foundation, the Alfred P. Sloan Foundation, and the Research Corporation for Science Advancement through Cottrell Scholar Award #28284. C.D.K. is partly supported by a CIERA postdoctoral fellowship. B.M. acknowledges financial support from the State Agency for Research of the Spanish Ministry of Science and Innovation under grant PID2019-105510GBC31/AEI/10.13039/501100011033 and through the Unit of Excellence Mar´ ıa de Maeztu 2020-2023 award to the Institute of Cosmos Sciences (CEX2019-000918-M). N.S. acknowledges the support from NASA (grant number 80NSSC22K0332), NASA FINESST (grant number 80NSSC22K1597), and Columbia University Dean's fellowship. Y.D., T.E., W.F., A.C.G., C.D.K., A.G.M., J.X.P., S.S., and N.T. acknowledge support from NSF grants AST1911140, AST-1910471 and AST-2206490 as members of the Fast and Fortunate for FRB Follow-up team. The Fong Group at Northwestern acknowledges support by the National Science Foundation under grant Nos. AST-1814782, AST-1909358 and CAREER grant No. AST-2047919.
The data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. W. M. Keck Observatory access was supported by Northwestern University and the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA).
supported by the dust extinction of A V ∼ 1 -1 . 5 mag as measured from SED fitting (Fong et al. 2021; Piro et al. 2021; Ravi et al. 2022).
§ Hefei National Laboratory, University of Science and Technology of China, Hefei 230088, China. Research supported by Innovation Program for Quantum Science and Technology 2021ZD0302902.
‡ School of Mathematical Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China. Resserach supported by National Key Research and Development Program of China 2020YFA0713100, National Natural Science Foundation of China grant 12125106, and Anhui Initiative in Quantum Information Technologies grant AHY150200. Email: jiema@ustc.edu.cn.
Acknowledgments. We are grateful to Prof. Thomas Delzant for helpful communications, in particular, for providing the proof of Lemma 6.2. Thanks go to Sam Hughes and Alice Kerr for pointing out the references and for several very helpful comments. We greatly thank the referee for many helpful comments and criticism on the writing, which helped much improve the exposition. W. Y. is supported by National Key R &amp; D Program of China (SQ2020YFA070059), and National Natural Science Foundation of China (No. 12131009 and No. 12326601).
- This material is based upon work supported by the National Aeronautics and Space Administration under Grant - Number 80NSSC21K0650 for the ADAP program, 80NSSC20K0257 for the XRP program, and 80NSSC22K0181 1 2 - through the TESS Guest Investigator program issued through the Science Mission Directorate. 3 - C.V.M. acknowledges support from the Alfred P. Sloan Foundation under grant number FG-2021-16592. 4 - Support for program HST-AR-15805.001-A was provided by NASA through a grant from the Space Telescope Science 5 - Institute, which is operated by the Associations of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5- 26555. 6 7 - Based on observations obtained with the Hobby-Eberly Telescope (HET), which is a joint project of the University of 8 - Texas at Austin, the Pennsylvania State University, Ludwig-Maximillians-Universitaet Muenchen, and Georg-August 9 - Universitaet Goettingen. Eberly. 10 11 - The HET is named in honor of its principal benefactors, William P. Hobby and Robert E. - These results are based on observations obtained with the Habitable-zone Planet Finder Spectrograph on the HET. The HPF team acknowledges support from NSF grants AST-1006676, AST-1126413, AST-1310885, AST1517592, AST-1310875, ATI 2009889, ATI-2009982, AST-2108512, AST-2108801, and the NASA Astrobiology Institute (NNA09DA76A) in the pursuit of precision radial velocities in the NIR. The HPF team also acknowledges support from the Heising-Simons Foundation via grant 2017-0494. 12 13 14 15 16 - The Center for Exoplanets and Habitable Worlds is supported by the Pennsylvania State University and the Eberly College of Science. 17 18 - GS acknowledges support provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51519.001-A 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. 19 20 21
The work of J. C. Garc´ ıa-Ardila has been supported by the Comunidad de Madrid multiannual agreement with the Universidad Rey Juan Carlos under the grant Proyectos I+D para Jovenes Doctores, Ref. M2731, project NETA-MM. The work of F. Marcellan has been supported by FEDER/Ministerio de Ciencia e Innovacion-Agencia Estatal de Investigacion of Spain, grant PID2021-122154NB-I00, and the Madrid Government (Comunidad de Madrid-Spain) under the Multiannual Agreement with UC3M in the line of Excellence of University Professors, grant EPUC3M23 in the context of the V PRICIT (Regional Program of Research and Technological Innovation).
Funding: The work of the second author was supported by the University of Macau (MYRG2022-00108-FST, MYRG-CRG2022-00010-ICMS), The Science and Technology Development Fund, Macau S.A.R (0036/2021/AGJ). The work of the third author was supported in part by the National Key Research and Development Program of China (2022YFE0112200), the National Natural Science Foundation of China (U21A20520, 62325204), Science and Technology Project of Guangdong Province (2022A0505050014), the Key-Area Research and Development Program of Guangzhou City (202206030009). The work of the fourth author was supported by the Science and Technology Planning Project of Guangzhou City, China (201907010043).
Funding The first author was funded by the Science and Technology Research Program of Chongqing Municipal Education Commission (Grant Nos. KJQN202100505, KJQN202200512), the Natural Science Foundation Project of Chongqing (Grant Nos. cstc2021jcyj-msxmX0195, CSTB2022NSCQ-MSX0896). The third author was funded by National Natural Science Foundation of China (No. 12101136), Guangdong Basic and Applied Basic Research Foundations (Nos. 2023A1515011633, 2020A1515110967), Project of Science and Technology of Guangzhou (No. 202102020273), the Open Project of Key Laboratory, School of Mathematical Sciences, Chongqing Normal University (No. CSSXKFKTQ202002).
CNPq through grant 308900/2019-7. R. Clemente acknowledges partial support from CNPq through grant 304454/2022-2.
Funding: J.M. do ´ O acknowledges partial support from CNPq through grants 312340/2021-4 and 429285/2016-7 and Pará ıba State Research Foundation (FAPESQ), grant no 3034/2021. E. Medeiros acknowledges partial support from
This material is based on work supported by the National Science Foundation under Grant No. CHE-2152521. K.S. was supported by a fellowship from the Molecular Sciences Software Institute under the National Science Foundation Grant No. CHE-2136142. This work was completed in part with resources provided by the University of Chicago Research Computing Center. We gratefully acknowledge computing time on the University of Chicago high-performance GPU-based cyberinfrastructure supported by the National Science Foundation under Grant No. DMR-1828629. We thank Adri` a Perez for their help in sharing the coarse-grained trajectories. We are grateful to D.E. Shaw Research for sharing the protein simulation trajectories.
G.K. acknowledges the funding from the European Union's Horizon 2020 Research and Innovation program under the Marie Skłodowska-Curie grant agreement no. 101024237. E.A.A gratefully acknowledges the support of King Abdulaziz City for Science and Technology (KACST), Saudi Arabia. S.R.P.S., D.K. and A.P gratefully acknowledges the support of MUSICODE H2020, the European collaborative research and innovation project led by a multi-disciplinary consortium.
A.N. is supported by NSF grant DMS-2005312. G.M. and F.Y. is supported by DOE grant DE-SC0010008.
We thank Pablo Boixeda Alvarez, Francis Bonahon, Daniel Douglas, Alexander Goncharov, David Jordan, and Ivan Losev for useful discussions. This research was supported in part by a grant from the Krembil Foundation. D.G. is supported by the NSERCDiscovery Grant program and by the Perimeter Institute for Theoretical Physics. Research at Perimeter Institute is supported in part by the Government of Canada through the Department of Innovation, Science and Economic Development Canada and by the Province of Ontario through the Ministry of Colleges and Universities.
This research is supported by Grant No. P 30855-N32 from the Austrian Science Fund (FWF). The first author would like to express gratitude to Silviana Amethyst from the Department of Mathematics at the University of Wisconsin Eau Claire and Professor Jonathan Hauenstein from the Department of Applied and Computational Mathematics and Statistics at the University of Notre Dame for their valuable suggestions and technical discussions on 𝙱𝚎𝚛𝚝𝚒𝚗𝚒 and 𝙿𝚊𝚛𝚊𝚖𝚘𝚝𝚘𝚙𝚢 . Additionally, the first author would like to thank Paul Breiding for providing assistance in setting up polyhedral homotopy computations in HC.jl and for clarifying questions regarding Bézout bounds. Furthermore, the first author would like to acknowledge Aravind Baskar from the University of Notre Dame for his assistance in sharing the algorithm for finding the best grouping for minimal Bézout bounds.
It is a pleasure to thank E. Cline and R. Gilman for discussions regarding MUSE. We are grateful to J. Bernauer, as well as O. Tomalak and M. Vanderhaeghen for providing their results from [16] and [38], respectively. T.E. was supported by the German Federal Ministry for Education and Research (BMBF) under contract no. 05H21VFCAA. F.H. and V.S. acknowledge support by the Swiss National Science Foundation (SNSF) through the Ambizione Grant PZ00P2 193383. F.H. acknowledges support by the Deutsche Forschungsgemeinschaft (DFG) through the Emmy Noether Programme (grant 449369623) and the Research Unit FOR 5327 'Photon-photon interactions in the Standard Model and beyond - exploiting the discovery potential from MESA to the LHC' (grant 458854507). M.R. is supported by the SNSF Grant 200020 207386. YU acknowledges support by the UK Science and Technology Facilities Council (STFC) under grant ST/T001011/1.
This work is partially supported by Institute of Information &amp; communications Technology Planning &amp; Evaluation (IITP) grant funded by the Korea government (MSIT) (No.2022-0-00124, Development of Artificial Intelligence Technology for Self-Improving Competency-Aware Learning Capabilities) and the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2022R1A2C2005529)
We thank Adam Riess for providing feedback on this paper and for discussion on the combined analysis and peculiar velocity correction. We also thank Nandita Khetan for useful discussions on the SBF calibration. The work of the Carnegie Supernova Project has been supported by the National Science Foundation (NSF) under grants AST0306969, AST0607438, AST1008343, AST1613426, AST1613472, AST613455., and also by the Danish Agency for Science and Technology and Innovation through a Sapere Aude Level 2 grant (PI Stritzinger). S. U. acknowledges financial support from the Distinguished Professor Chair funds of N. Suntzeff. N. B. S. and K. K. gratefully acknowledge the support from the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy. We also thank the Mitchell Foundation for their support of the Cooks Branch Workshop on Supernovae. M. S. acknowledges grants from the Villum FONDEN No. 24349 and the Independent Research Fund Denmark (IRFD No. 8021-00170B). C. G. acknowledges support from research grant by the VILLUM FONDEN No. 25501. L. G. acknowledges financial support from the Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) 10.13039/501100011033, and the European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program RYC2019-027683-I and the PID2020115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Cient´ ıficas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia Mar´ ıa de Maeztu CEX2020-001058-M. B. J. S. is supported by NSF grants AST-1920392 and AST1911074. We acknowledge the Las Campanas Observatory for the outstanding support during our observing runs, and to the Carnegie Observatories Time Allocation Committee for generous time allocations.
This study is supported under the RIE2020 Industry Alignment Fund - Industry Collaboration Projects (IAF-ICP) Funding Initiative, as well as cash and in-kind contribution from the industry partner(s). This research is partially supported by the National Research Foundation Singapore and DSO National Laboratories under the AI Singapore Programme (AISG Award No: AISG2-RP-2020-019), the NRF Investigatorship NRFNRFI06-2020-0001, the Ministry of Education, Singapore under its Academic Research Fund Tier 3 (MOET32020-0004). Any opinions, findings and conclusions or recommendations expressed in this material are those of the author(s) and do not reflect the views of the Ministry of Education, Singapore.
Volker Roeber acknowledges financial support from the I-SITE program Energy &amp; Environment Solutions (E2S), the Communauté d'Agglomération Pays Basque (CAPB), and the Communauté Région Nouvelle Aquitaine (CRNA) for the chair position HPC-Waves and support from the European Union's Horizon 2020 research and innovation programme under grant agreement no.
We thank Jan Bödewadt and Jurij Stell for technical support. We acknowledge funding from the Research Council of Norway under grant no. 239033/F20, and from Bergen Universitetsfond, MPB, JH, MS, MC, and RC wish to acknowledge from the Coasts in the Changing Earth System (PACES II) program of the Helmholtz Association, and support from the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation, project number 274762653, Collaborative Research Centre TRR 181 Energy Transfers in Atmosphere and Ocean ).