cometadata/test-preprints-extracted-funding huggingface dataset:
We thank Leandro Beraldo e Silva, Gregory Green, and the referees for valuable comments and suggestions, and Adrian Price-Whelan for providing an observational dataset used in several figures. EV is supported by an STFC Ernest Rutherford fellowship (ST/X004066/1). This work, as well as most of the referenced articles, has made use of data from the European Space Agency (ESA) mission Gaia (www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC). This work also used data from the Sloan Digital Sky Survey IV (www.sdss.org). Funding for SDSS-IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and numerous Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High Performance Computing at the University of Utah.
The authors are grateful to H. Ohgaki of the Institute of Advanced Energy, Kyoto University for making a large volume LaBr 3 :Ce detector available for the experiment. I.G., D.F. and M.K. acknowledge the support from the Extreme Light Infrastructure Nuclear Physics (ELINP) Phase II, a project cofinanced by the Romanian Government and the European Union through the European Regional Development Fund - the Competitiveness Operational Programme (1/07.07.2016, COP, ID 1334). I.G. and D.F. acknowledge the support from the Romanian Project PN-23-21-01-02. S.G. acknowledges financial support from F.R.S.-FNRS (Belgium). This work was supported by the F.R.S.- FNRS and FWO under the EOS Project Nr O022818F.
Research funding: Australian Research Council (Grant No. DP210101292), International Technology Center Indo-Pacific (ITC IPAC) via Army Research Office (Contract FA520923C0023), National Natural Science Foundation of China (Grants No. 12261131500, No. 12025402, and No. 12334016), Shen-
zhen Fundamental Research Projects (Grant No. JCYJ20241202123719025).
This work was supported in part by National Natural Science Foundation of China under Grant 62301251 and 62201463, in part by the Natural Science Foundation on Frontier Leading Technology Basic Research Project of Jiangsu under Grant BK20222001, in part by the open research fund of National Mobile Communications Research Laboratory, Southeast University (No. 2024D04), in part by the Aeronautical Science Foundation of China 2023Z071052007, and in part by the Young Elite Scientists Sponsorship Program by CAST 2023QNRC001. ( Corresponding author: Ziye Jia. )
JZ would like to thank Bao-chi Fu, Renata Krupczak, Guang-You Qin, Hendrik Roch, Xiang-Yu Wu for productive discussions. OGM would like to acknowledge productive discussions with Travis Dore, Wilke van der Schee and Govert Nijs. This work is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through the CRC-TR 211 'Strong-interaction matter under extreme conditions' project number 315477589 - TRR 211. OGM and SS also acknowledge support by the German Bundesministerium für Bildung und Forschung (BMBF) through Grant No. 05P21PBCAA. J.Z. is also supported in part by China Scholarship Council (CSC) under Grant No. 202306770009. Numerical simulations presented in this work were performed at the Paderborn Center for Parallel Computing ( PC 2 ).
We gratefully acknowledge financial support from the German Federal Ministry of Education and Research (BMBF) within the projects NEUROTEC 2 (16ME0399, 16ME0398K, 16ME0400) and NeuroSys (03ZU1106AA, 03ZU1106BA, 03ZU2106AE, 03ZU2106AA), from the European Union ' s Horizon Europe research and innovation program under the project ENERGIZE (101194458), and Deutsche Forschungsgemeinschaft (DFG) within the project SPP2262 MEMMEA, project no. 441918103 (MemrisTec).
This work is supported by the National Solar Observatory, the Office of Naval Research, and the NASA HSR and LWS Programs. JEL, MGL, PWS, LAT, and NDK acknowledge support from NASA grants NNH16ZDA001N-LWS 'Implementing and Evaluating a Vector-Magnetogram-Driven Magnetohydrodynamic Model of the Magnetic Field in the Low Solar Atmosphere', NNH21ZDA001N-LWS 'The Origin of the Photospheric Magnetic Field: Mapping Currents in the Chromosphere and Corona', and NNH17ZDA001NLWS 'Investigating Magnetic Flux Emergence with Modeling and Observations to Understand the Onset of Major Solar Eruptions'. MGL additionally acknowledges support from the Office of Naval Research. PWS and JEL additionally acknowledge support from the NASA Internal Science Funding Model (H-ISFM) program 'Magnetic Energy Buildup and Explosive Release in the Solar Atmosphere.' This research has made use of NASA's Astrophysics Data System. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19
This work was supported by the UK Royal Academy of Engineering under the Research Fellowship Scheme (RF/201718/17128). We acknowledge the Interdisciplinary Centre for Electron Microscopy (CIME) at EPFL for providing access to their electron microscopy facilities. Lastly, we thank Prof. Jean-Marc Triscone and Prof. Patrycja Paruch from the University of Geneva for their continued support during the realization of this work.
This work is partially supported by the National Natural Science Foundation of China under Grants No. 12175240, No. 12147153, No. 12305097, and No. 12305137, the Fundamental Research Funds for the Central Universities (Grant No. 23CX06037A), the Shandong Provincial Natural Science Foundation, China (Grant No. ZR2024QA096), and the Taishan Scholar Young Talent Program (tsqn202408091).
T.H., S.B., Y.M., T.K., K.K., M.O. and T.I. were supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI grant No. [22H01258, 23K22529], 23H05441, 21H04494, JP23K13153, [22H04939, 23K20035, 24H00004], 24K22894 and [21H04496, 23K03462] respectively. T.K. is grateful for support from the RIKEN Special Postdoctoral Researcher Program. K.I. acknowledges support under the grant PID2022-136827NB-C44 provided by MCIN/AEI/10.13039/501100011033 / FEDER, UE. M.S. was supported by the ALMA Japan Research Grant of NAOJ ALMA Project, NAOJ-ALMA-339.
This work was partly supported by the FCT Funda¸ c˜ ao para a Ciˆ encia e a Tecnologia, I.P., under Projects Nos. UIDB/04564/2020 ( https://doi.org/10.54499/UIDB/ 04564/2020 ), UIDP/04564/2020 ( https://doi.org/10. 54499/UIDP/04564/2020 ). O.O. also acknowledges financial support from grant 2022/05328-3, from S˜ ao Paulo Research Foundation (FAPESP). T. F. thanks the financial support from the Brazilian Institutions: National Council for Scientific and Technological Development CNPq (Grant No. 308486/2015-3), Improvement of Higher Education Personnel CAPES (Finance Code 001) and FAPESP (Grants No. 2017/05660-0 and 2019/07767-1). W. d. P. acknowledges the partial support of CNPQ under Grant No. 313030/2021-9 and the partial support of CAPES under Grant No. 88881.309870/201801. This work is a part of the project Instituto Nacional de Ciˆ encia e Tecnologia - F´ ısica Nuclear e Aplica¸ c˜ oes Proc. No. 464898/2014-5.
Support for program GO 2540 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 503127. Part of this research was carried out at the Jet Propul- sion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). A.I. acknowledges support from the National Aeronautics and Space Administration under grant No. 80NSSC18K0828. S.Z. acknowledges support by NASA through the NASA Hubble Fellowship grant #HSTHF2-51568 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.
the Spanish Virtual Observatory (https://svo.cab.inta-csic. es) project funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00. VOSA has been partially updated by using funding from the European Union's Horizon 2020 Research and Innovation Programme, under Grant Agreement nº 776403 (EXOPLANETS-A).
Thanks to Hailin Ma, Han Lu, Jiayi Guo, Rui Su for their support during this study.
This work was partially supported by the National Natural Science Foundation of China (Grant No. 82151318); Science and Technology Commission of Shanghai (Grant No. 22DZ2229004, 22JC1403603, 21Y11902500); the Key Research &amp; Development Project of Zhejiang Province (2024C03240); Scientific Development funds for Local Region from the Chinese Government in 2023 (Grant No. XZ202301YD0032C); Jilin Province science and technology development plan project (Grant No. 20230204094YY), 2022 'Chunhui Plan' cooperative scientific research project of the Ministry of Education.
- We thank G. DelZanna, V. J. Esposito and Aigen Li for helpful discussions. We especially thank P. J. Storey for kindly making available extended tables of H I emissivities. We thank the anonymous referee for a thoughtful and very helpful report that led to improvements in the paper. 1 2 3 - This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. 4 - The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, 5 6 - Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with GO 7 - program #3435. The authors acknowledge the PDRs4All Team for their publicly available data products from the Early Release Science Program #1288. We also used publicly available data for 8 9 - M17 from Cycle 1 GO Program 1591, PI L. Allamandola. Support for program GO #3435 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by 10 11 - the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. 12 - This research has made use of NASA's Astrophysics Data System, as well as ds9, a tool for data visualization supported by the Chandra X-ray Science Center (CXC) and the High Energy Astrophysics Science Archive Center (HEASARC) with support from the JWST Mission office at the Space Telescope Science Institute for 3D visualization. 13 14 15 16 - K.S., D.D., J.D.S., A.D.B., M.L.B., D.C., K.D.G., A.K.L., J.R.D., and B.F.W. acknowledge support from grant JWST-GO-03435. A.A. acknowledges support from the Swedish National Space Agency 17 18 - (SNSA) through the grant 2021-00108. R.S.K. acknowledges financial support from the European 19 - Research Council via the ERC Synergy Grant 'ECOGAL' (project ID 855130), from the German Excellence Strategy via the Heidelberg Cluster of Excellence (EXC 2181-390900948) 'STRUCTURES', 20 21 - and from the German Ministry for Economic Affairs and Climate Action in project 'MAINN' (fund22 - ing ID 50OO2206). R.S.K. is grateful for computing resources provided by the Ministry of Science, 23 - Research and the Arts (MWK) of the State of Baden-W¨ urttemberg through bwHPC and the German 24
- for data storage at SDS@hd funded through grants INST 35/1314-1 FUGG and INST 35/1503-1 26 - FUGG. 27
This work was funded by the Council for At-Risk Academics (Cara) within the Cara Fellowship Programme &amp; the British Academy within the British Academy/Cara/Leverhulme Researchers at Risk Research Support Grants Programme under grant number LTRSF/100141. J.L. thanks CNPq, FAPERJ, and INCT-FNA (Instituto Nacional de Ciˆ encia e Tecnologia -F´ ısica Nuclear e Aplica¸ c˜ oes) research project 464898/2014-5 for the partial financial support.
This work was supported by National Key R&amp;D Program of China grant (2024YFB3816000), Shenzhen Key Laboratory of Ubiquitous Data Enabling (No. ZDSYS20220527171406015), Shenzhen Science and Technology Program (JCYJ20220530143013030), Guangdong Innovative and Entrepreneurial Research Team Program (2021ZT09L197), National Natural Science Foundation of China (62104125, 62003188), Tsinghua Shenzhen International Graduate School-Shenzhen Pengrui Young Faculty Program of Shenzhen Pengrui Foundation (No. SZPR2023005) and Meituan. Shoujie Li and Jianle Xu contributed equally to this work. (Corresponding author: Xueqian Wang &amp; Wenbo Ding, wang.xq@sz.tsinghua.edu.cn &amp; ding.wenbo@sz.tsinghua.edu.cn)
We thank Gang Liang, Elchanan Mossel, and Bin Yu for discussions and encouragements. S.R. gratefully acknowledges the partial support of CIPRES (NSF ITR grant # NSF EF 03-31494), NSERC (Canada), FQRNT (Quebec, Canada), a Lo` eve Fellowship (UC Berkeley), and NSF grant DMS0528488. S.R. also thanks Martin Nowak and the Program for Evolutionary Dynamics at Harvard University, where part of this work was done. S.B. thanks David Aldous for interesting discussions.