cometadata/test-preprints-extracted-funding huggingface dataset:
This work was supported by Samsung Science and Technology Foundation (project no. SRFC-MA2201-03) and by the Ministry of Education of the Republic of Korea and the National Research Foundation of Korea (RS-2024-00343871). This work was supported by a KIAS Individual Grant (AP091501 to J.W.Y., CG035003 to C.H.) at Korea Institute for Advanced Study. We especially thank Tae Jun Yoon for his fruitful discussion.
MWT acknowledges support from the NASA ADAP program through the grant number 80NSSC23K0467. DPS acknowledges support from the National Science Foundation through the grant AST-2109066. AZ acknowledges support by Grant No. 2020750 from the United States-Israel Binational Science Foundation (BSF) and Grant No. 2109066 from the United States National Science Foundation (NSF); by the Ministry of Science &amp; Technology, Israel; and by the Israel Science Foundation Grant No. 864/23.
This work has been partially supported by the Spanish Ministry of Science and Innovation through the PID2022-139977NB-I00 project and TED2021-131310BI00 ('Bayes-Interpret'), and by the Autonomous Community of Madrid within the ELLIS Unit Madrid frame-
This work was also partially supported by the Dutch Research Council (NWO/OCW), as part of the Quantum Software Consortium programme (project number 024.003.03), and co-funded by the European Union (ERC CoG, BeMAIQuantum, 101124342). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them
Vicente P. Soloviev has been supported by the predoctoral grant FPI PRE2020-094828 from the Spanish Ministry of Science and Innovation.
We appreciate the valuable discussion and comments from the referee, which have greatly improved the manuscript. This work has been partially supported by MICINN (Spain), project PID2019-104397GB-I00, of the Spanish State Research Agency program AEI/10.13039/501100011033, by the Catalan Government, AGAUR project 2021-SGR00171, and by the program Unidad de Excelencia Mar´ ıa de Maeztu CEX2020-001058-M. M.K. has been supported by a Juan de la Cierva-incorporacion grant (IJC2020-042690-I).
The authors would like to thank Diego Pazó and Alessandro Torcini for useful feedback on this work. PC and JGO have received funding from the Future and Emerging Technologies Programme (FET) of the European Union's Horizon 2020 research and innovation programme (project NEUROTWIN, grant agreement No 101017716). JGO was also financially supported by the Spanish Ministry of Science and Innovation, the Spanish State Research Agency and FEDER (project reference PID2021-127311NB-I00), and by the ICREA Academia program. This work has done while PF was a student at the ETSETB, Universitat Politècnica de Catalunya.
This work was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation): KR5148/3-1 (project number 510395418), KR5148/5-1 (project number 542747151), and GRK 2839 (project number 468527017) to PK, and grant SCHI 1482/3-1 (project number 451810794) to AS.
This work benefited from useful conversations with Benjamin Chandran, Christopher Chen, Mihailo Martinovic, Romain Meyrand, and Evan Yerger. M.F.Z. and M.W.K. were supported by the National Aeronautics and Space Administration (NASA) under Grant No. 80NSSC24K0171 issued through the Heliophysics, Theory, Modeling and Simulation Program. Support for J.S. was provided by Rutherford Discovery Fellowship RDF-U001804 and Marsden Fund grant UOO1727, which are managed through the Royal Society Te Ap¯ arangi. K.G.K. was supported by NASA grant 80NSSC19K0912 from the Heliophysics Early Career Investigators Program. This work is part of the Frontera computing project at the Texas Advanced Computing Center under allocation number AST20010; it also made extensive use of the Perseus cluster at the PICSciEOIT TIGRESS High Performance Computing Center and Visualization Laboratory at Princeton University, as well as High Performance Computing resources sup-
ported by the University of Arizona Research Technologies department. The authors thank the Kavli Institute for Theoretical Physics (KITP) for its hospitality dur- ing the completion of this work; KITP is supported in part by the National Science Foundation under Award No. PHY-2309135.
OO acknowledges partial financial support from CONICET (PIP 11220210100787CO) and Secyt-UNC (33620230100363CB), and the warm hospitality at FACENA-UNNE. AF and DAC acknowledge funding from CONICET (PUE22920170100089CO and PIP11220200100170), AF acknowledges partial financial support from ANPCyT (PICT2019-0654)
We would like to thank Simon D. M. White for useful discussions and advice. We also thank the anonymous referee for their helpful comments. We acknowledge the supports from the National Natural Science Foundation of China (Grant No. 11988101) and the K. C. Wong Education Foundation. SS acknowledges support from NSFC grant (No. 12273053), CAS Project for Young Scientists in Basic Research Grant (No. YSBR-062), and the science research grants from the China Manned Space Project with No. CMS-CSST-2021B03. AF is supported by a UKRI Future Leaders Fellowship (grant no MR/T042362/1). RJW acknowledges the supports by the Forrest Research Foundation and the European Research Council via ERC Consolidator Grant KETJU (no. 818930).
The authors thank Cole Miller and Jim Lattimer for useful discussions. V.G. acknowledges funding from the Southeastern Universities Research Association for the CRESST II/NASA Summer Internship at NASA/GSFC, during which part of this work was completed. D.R. acknowledges funding from the U.S. Department of Energy, Office of Science, Division of Nuclear Physics under Award Number(s) DE-SC0021177 and DE-SC0024388, and from the National Science Foundation (NSF) under Grants No. PHY-2011725, PHY-2020275, PHY-2116686, PHY-2407681, and AST-2108467. C.C. acknowledges support by NASA under award numbers 80GSFC21M0002 and 80NSSC20K0288. K.Y. acknowledges support from NSF Grant PHYS-2339969 and the Owens Family Foundation.
X. Yu, C. N. Luu, J. I. Moses, and J. Krissansen-Totton are supported by the NASA Habitable Worlds Program Grant 80NSSC24K0075. C. R. Glein and N. Truong acknowledge support from the Heising-Simons Foundation (grant 20234657). X. Yu is supported by the NASA Planetary Science Early Career Award 80NSSC23K1108 and by the HeisingSimons Foundation grant 2023-3936. S.-M.T. is supported by NASA through Exobiology Grant No. 80NSSC20K1437 and Interdisciplinary Consortia for Astrobiology Research (ICAR) Grant Nos. 80NSSC23K1399, 80NSSC21K0905, and 80NSSC23K1398. X. Zhang is supported by the National Science Foundation grant AST2307463 and the NASA Exoplanet Research grant 80NSSC22K0236. A. Aguichine is supported by NASA's Interdisciplinary Consortia for Astrobiology Research (ICAR) Grant No. 80NSSC21K0597. H.I. is supported by the European Union (ERC, DIVERSE, 101087755). This work also benefited from the Exoplanet Summer Programs in the Other Worlds Laboratory (OWL) at the University of California, Santa Cruz, a program funded by the Heising-Simons Foundation. We also acknowledge Dr. Ligia Fonseca Coelho for insightful discussions on the temperature range for microbial growth.
BH thanks Prof. Giovanni Ciccotti for the first discussion that sparked our interest in informed resetting protocols for enhanced sampling. BH acknowledges support by the Israel Science Foundation (grants No. 1037/22 and 1312/22) and the Pazy Foundation of the
IAEC-UPBC (grant No. 415-2023). This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Grant agreement No. 947731 to SR).
The authors thank useful discussion with Shuxuan Wang and Junnan Lu. Zhiwei Yin and Shaolong Wan acknowledge the support by NSFC Grant No. 11275180. Haoshu Li acknowledges the support from the China Postdoctoral Science Foundation 2023M743398. Zhongbo Yan acknowledges the support from the National Natural Science Foundation of China (Grant No. 12174455) and the Natural Science Foundation of Guangdong Province (Grant No. 2021B1515020026).
We thank the referee for multiple suggestions that improved the clarity and usefulness of this work. This work includes observations made with the NASA/ESA/CSA James Webb Space Telescope. The JWST data used in this paper can be found in MAST: 10.17909/7w5s-f430. 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, Inc., under NASA contract NAS 5-03127 for JWST. The observations are associated with JWST GO Cycle 1 programs 1549, 1584, and 1640. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). The authors acknowledge support from NASA/Space Telescope Science Institute grants: JWST-GO-01640, JWST-GO-01584, and JWST-GO-01549. G.A.B. gratefully acknowledges support from NASA grant 80NSSC24K0149.
Acknowledgements. JMS and MPC have been funded by Ministerio de Ciencia e Innovacion (Spain), projects PID2022-136585NB-C21 and PID2022-136585NB-C22, MCIN/AEI/10.13039/501100011033/FEDER, UE. BZ has been funded by the Young Elite Scientists Sponsorship Program by CAST (No. 2023QNRC001).
AST-2205628, and NASA grants 80NSSC23K0497 and 80NSSC23K1247. JS acknowledges support from the Packard Foundation. EA gratefully acknowledges support from the NASA Hubble Fellowship. JLS acknowledges support from NSF grant AST-1816100.
IM, LC, EA, KVS, PC, and CEH are grateful for support from NSF grants AST-1751874, AST-2107070, and
This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. 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, Inc., under NASA contract NAS 5-03127 for JWST. The specific observations analyzed can be accessed via 10.17909/vt74-kd84. These observations are associated with program #2078. Support for program #2078 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 5-03127.
We thank the anonymous reviewer for constructive comments that improved this manuscript. XJ thanks Yongda Zhu, Daichi Kashino, and Andrei Mesinger for informative discussions. FW acknowledges support from NSF Grant AST-2308258. RAM acknowledges support from the Swiss National Science Foundation (SNSF) through project grant 200020 207349. GDB was supported by the NSF through grant AST-1751404. SZ acknowledges support from the National Science Foundation of China (grant no. 12303011).
and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
All presented computations were performed on a PC-Cluster at the Center for Information Services and High Performance Computing (ZIH) at TU Dresden. The authors thus thank the ZIH for generous allocations of computer time. This work was supported by a postdoc fellowship of the German Academic Exchange Service (DAAD) to Karl A. Kalina. This support is gratefully acknowledged. Finally, the authors thank the German Research Foundation (DFG) for the support within the Research Training Group GRK 2868 D 3 -Project Number 493401063.
The authors are indebted to Marie-Aline Martin-Drumel for a machine-readable copy of her C 3 infrared spectrum covering the frequency range 1900 - 2100 cm -1 . This work used the DiRAC Data Intensive service (CSD3) at the University of Cambridge, managed by the University of Cambridge University Information Services and the DiRACDataIntensive service (DIaL2) at the University of Leicester, managed by the University of Leicester Research Computing Service on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). The DiRAC services at Cambridge and Leicester were funded by BEIS, UKRI and STFC capital funding and STFC operations grants. Computing facilities at University College London and the University of Oxford were also used. This work was supported by the STFC Project No. ST/Y001508/1 and by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme through Advance Grant number 883830. NFZ also acknowledges support by State Project IAP RAS No. FFUF2024-0016.
S.K., A.B.G., and R.R. acknowledge DST, India, for the financial support for the work done at the Elettra synchrotron source with proposal number 20165031. The authors thank Dr. S. N. Achary of the Chemistry Division, Bhabha Atomic Research Centre, for providing XRD data of LT-CuCN at ambient conditions. N.P.S. acknowledges support by DOE-SC (DESC0020340), DOE-NNSA (DE-NA0004153, CDAC), and NSF (DMR-2119308). N.P.S. acknowledges the support and encouragement of Prof. Russell J. Hemley.
We gratefully acknowledge Jack Raymond, Mohammad Amin, Trevor Lanting and Mark Johnson for their feedback and discussions. We gratefully acknowledge funding from the National Research Council (Canada) via Agreement AQC-002, Natural Sciences and Engineering Research Council (Canada), in particular, via Grants SAPPJ-2020-00032 and SAPPJ-2022-00020. This research was supported in part by Perimeter Institute for Theoretical Physics. Research at Perimeter Institute is
supported by the Government of Canada through the Department of Innovation, Science and Economic Development and by the Province of Ontario through the Ministry of Research, Innovation and Science. The University of Virginia acknowledges support from NSF 2212550 OAC Core: Smart Surrogates for High Performance Scientific Simulations and DE-SC0023452: FAIR Surrogate Benchmarks Supporting AI and Simulation Research. JQTM acknowledges a Mitacs Elevate Postdoctoral Fellowship (IT39533) with Perimeter Institute for Theoretical Physics.
This work was supported by the Department of Energy grant DE-SC0021152. Additionally, D. L. was supported by Department of Energy grant DE-SC0023658 and National Science Foundation grant PHY-2310620, and A. B. and L. H. were supported by Department of Energy grant DE-SC0019139. G. P. acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - project number 460248186 (PUNCH4NFDI). A.S. acknowledges funding support from Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through grant 513989149, under the National Science Foundation grant PHY- 2209185 and from the Department of Energy Topical Collaboration 'Nuclear Theory for New Physics', award No. DESC0023663
- M.J.H. is supported by the Swedish Research Council (Veten1 - skapsrådet) and is Fellow of the Knut &amp; Alice Wallenberg 2 - Foundation. B.L.J. is thankful for support from the Euro3 - pean Space Agency (ESA). We thank the anonymous referee 4 - for careful reflections that have improved the quality of the 5 - manuscript, C. Simmonds for useful discussions on the ioniz6
Manuscript received November 16, 2024; revised December 29, 2024; accepted add date. Date of publication add date; date of current version add date. This work was supported by the Defense Advanced Research Project Agency Microsystems Technology Office (DARPA MTO) COFFEE TA1 project under Contract HR001122C0088 and developed in collaboration with RTX Missiles and Defense and Naval Research Lab (NRL). The review of this letter was arranged by Editor add name. (Corresponding authors: L. Colombo and M. Rinaldi.)
This work is supported by the National Natural Science Foundation of China under grant Nos. 12375135, 11447024, and 11505108. A.K.L. acknowledges the financial support from the China Scholarship Council. Y.L.Y. acknowledges the financial support from the Continuous-Support Basic Scientific Research Project in China Institute of Atomic Energy. L.Z. acknowledges the support from the Fundamental Research Funds for the Central Universities, China University of Geosciences (Wuhan) with No. G1323523064. W.C.Z. is supported by the Natural Science Basic Research Plan in Shaanxi Province of China (No. 2023-JCYB-012). H.Z. acknowledges the financial support from Key Laboratory of Quark and Lepton Physics in Central China Normal University under grant No. QLPL2024P01.
S.J.H. and E.T. thank the Engineering and Physical Sciences Research Council (EPSRC) for funding under grants EP/S021531/1, EP/M010619/1, EP/V001914/1 and EP/P009050/1, the National Physical Laboratory (NPL) UK and the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (Grant ERC-2016-STGEvoluTEM-715502). TEM access was supported by the Henry Royce Institute for Advanced Materials, funded through EPSRC grants EP/R00661X/1, EP/S019367/1, EP/P025021/1 and EP/P025498/1.
BASS is a key project of the Telescope Access Program (TAP), which has been funded by the National Astronomical Observatories of China, the Chinese Academy of Sciences (the Strategic Priority Research Program 'The Emergence of Cosmological Structures' Grant # XDB09000000), and the Special Fund for Astronomy from the Ministry of Finance. The BASS is also supported by the External Cooperation Program of Chinese Academy of Sciences (Grant # 114A11KYSB20160057), and Chinese National Natural Science Foundation (Grant # 12120101003, # 11433005).
Funding for the Sloan Digital Sky Survey V has been provided by the Alfred P. Sloan Foundation, the Heising-Simons Foundation, the National Science Foundation, and the Participating Institutions. SDSSacknowledges support and resources from the Center for HighPerformance Computing at the University of Utah. SDSS telescopes are located at Apache Point Observatory, funded by the Astrophysical Research Consortium and operated by New Mexico State University, and at Las Campanas Observatory, operated by the Carnegie Institution for Science. The SDSS web site is www.sdss.org .
MJJ acknowledge the support of a UKRI Frontiers Research Grant [EP/X026639/1], which was selected by the European Research Council, and the STFC consolidated grants [ST/S000488/1] and [ST/W000903/1]. MJJ and CLH also acknowledge support from the Oxford Hintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze Family Charitable Foundation.
The Photometric Redshifts for the Legacy Surveys (PRLS) catalog used in this paper was produced thanks to funding from the U.S.
We acknowledge the use of the ilifu cloud computing facility www.ilifu.ac.za, a partnership between the University of Cape Town, the University of the Western Cape, Stellenbosch University, Sol Plaatje University and the Cape Peninsula University of Technology. The Ilifu facility is supported by contributions from the InterUniversity Institute for Data Intensive Astronomy (IDIA - a partnership between the University of Cape Town, the University of Pretoria and the University of the Western Cape, the Computational Biology division at UCT and the Data Intensive Research Initiative of South Africa (DIRISA). The authors acknowledge the Centre for High Performance Computing (CHPC), South Africa, for providing computational resources to this research project.
This work has been supported by the Strategic Priority Research Program of Chinese Academy of Sciences (Grant No. XDB34010000), the National Natural Science Foundation of China (Grant Nos. 12375127 and 11975237), the U.S. Department of Energy under Grant Nos. DE-SC0013847 (Vanderbilt University), DESC0013365, and DE-SC0023175 (Michigan State University). The computations in present work have been performed on the C3S2 computing center in Huzhou University and HPC cluster in Beijing PARATERA Tech Ltd.
This research was supported by the National Natural Science Foundation of China under Grants Nos. (12305002, 12274171, 12274174, T2225013, and 12174142,12034009), the National Key R&amp;D Program of China (Grant No. 2023YFA1406200), the Program for JLU Science and Technology Innovative Research Team. Part of the calculation was performed in the high-performance computing center of Jilin University.
We thank all members of the ETM collaboration for a most conducive cooperation. We would like to thank Lorenzo Barca, Marilena Panagiotou and Rainer Sommer for useful discussions and suggestions. We acknowledge computing time granted on Piz Daint at Centro Svizzero di Calcolo Scientifico (CSCS) via the project with id s1174, JUWELS Booster at the Jülich Supercomputing Centre (JSC) via the project with id pines, and Cyclone at the Cyprus institute (CYI) via the project with ids P061, P146 and pro22a10951. Y.L. is supported by the Excellence Hub project "Unraveling the 3D parton structure of the nucleon with lattice QCD (3D-nucleon)" id EXCELLENCE/0421/0043 co-financed by the European Regional Development Fund and the Republic of Cyprus through the Research and Innovation Foundation. F.P. acknowledges financial support by the Cyprus Research and Innovation foundation Excellence Hub project NiceQuarks under contract with number EXCELLENCE/0421/0195. C.A. and G. K. acknowledge partial support from the European Joint Doctorate AQTIVATE that received funding from the European Union's research and innovation programme under the Marie Sklodowska-Curie Doctoral Networks action under the Grant Agreement No 101072344. M.P. acknowledges support by the Sino-German collaborative research center CRC 110.
KG is supported by the Australian Research Council through the Discovery Early Career Researcher Award (DECRA) Fellowship (project number DE220100766) funded by the Australian Government. KG is supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013.
MB gratefully acknowledges support from the ANID BASAL project FB210003 and from the FONDECYT regular grant 1211000.
RSK acknowledges financial support from the European 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',
This work was supported by the French government through the France 2030 investment plan managed by the National Research Agency (ANR), as part of the Initiative of Excellence of Universite Cˆ ote d'Azur under reference number ANR-15-IDEX-01.
and from the German Ministry for Economic Affairs and Climate Action in project 'MAINN' (funding ID 50OO2206). RSK is grateful for computing resources provided by the Ministry of Science, Research and the Arts (MWK) of the State of Baden-W¨ urttemberg through bwHPC and the German Science Foundation (DFG) through grants INST 35/1134-1 FUGG and 35/1597-1 FUGG, and also for data storage at SDS@hd funded through grants INST 35/1314-1 FUGG and INST 35/1503-1 FUGG. RSK also thanks the HarvardSmithsonian Center for Astrophysics and the Radcliffe Institute for Advanced Studies for their hospitality during his sabbatical, and the 2024/25 Class of Radcliffe Fellows for a great community and highly interesting and stimulating discussions.
This work was supported by NSF-China (Grant Nos. 11904078 and 11575051), GRF (Grant Nos. 17310622 and 17303023) of Hong Kong, Hebei NSF (Grant Nos. A2021205020 and A2019205266), and Hebei 333 Talent Project (B20231005). JR was also funded by the project of the China Postdoctoral Science Foundation (Grant No. 2020M670683).
This work is supported by National Natural Science Foundation of China (NSFC 62371325, 62071314), Sichuan Science and Technology Program 2023YFG0263, 2023YFG0025, 2023NSFSC0497, and Opening Foundation of Agile and Intelligent Computing Key Laboratory of Sichuan Province. The associate editor coordinating the review of this manuscript and approving it for publication was ***. (* Corresponding author: Yan Wang )