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Institution

Stockholm University

EducationStockholm, Sweden
About: Stockholm University is a education organization based out in Stockholm, Sweden. It is known for research contribution in the topics: Population & Supernova. The organization has 21052 authors who have published 62567 publications receiving 2725859 citations. The organization is also known as: University of Stockholm & Stockholms universitet.


Papers
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Journal ArticleDOI
Peter Bohm1
TL;DR: In this paper, the authors describe a test involving five different approaches to estimating the demand for a public good in a setting which permitted a real collective choice and in which each subject was committed to actual payments when relevant.

413 citations

Journal ArticleDOI
TL;DR: The more recent systems constructed as models for the hydrogenase enzymes are reviewed, with a specific focus on the various strategies employed for incorporating of synthetic models into supramolecular frameworks and polypeptidic/protein scaffolds.

412 citations

Journal ArticleDOI
TL;DR: It is reported that nuclear factor erythroid-derived 2-related factor 1 (Nrf1), a transcription factor of the cap "n" collar basic leucine zipper family, but not the related Nrf2, is necessary for induced proteasome gene transcription in mouse embryonic fibroblasts (MEFs).

412 citations

Journal ArticleDOI
Elena Aprile1, Jelle Aalbers2, F. Agostini3, M. Alfonsi4, L. Althueser5, F. D. Amaro6, V. C. Antochi2, E. Angelino7, F. Arneodo8, D. Barge2, Laura Baudis9, Boris Bauermeister2, L. Bellagamba3, M. L. Benabderrahmane8, T. Berger10, P. A. Breur11, April S. Brown9, Ethan Brown10, S. Bruenner12, Giacomo Bruno8, Ran Budnik13, C. Capelli9, João Cardoso6, D. Cichon12, D. Coderre14, Auke-Pieter Colijn11, Jan Conrad2, Jean-Pierre Cussonneau15, M. P. Decowski11, P. de Perio1, A. Depoian16, P. Di Gangi3, A. Di Giovanni8, Sara Diglio15, A. Elykov14, G. Eurin12, J. Fei17, A. D. Ferella2, A. Fieguth5, W. Fulgione7, P. Gaemers11, A. Gallo Rosso, Michelle Galloway9, F. Gao1, M. Garbini3, L. Grandi18, Z. Greene1, C. Hasterok12, C. Hils4, E. Hogenbirk11, J. Howlett1, M. Iacovacci, R. Itay13, F. Joerg12, Shingo Kazama19, A. Kish9, Masanori Kobayashi1, G. Koltman13, A. Kopec16, H. Landsman13, R. F. Lang16, L. Levinson13, Qing Lin1, Sebastian Lindemann14, Manfred Lindner12, F. Lombardi17, F. Lombardi6, J. A. M. Lopes6, E. López Fune20, C. Macolino21, J. Mahlstedt2, A. Manfredini13, A. Manfredini9, Fabrizio Marignetti, T. Marrodán Undagoitia12, Julien Masbou15, S. Mastroianni, M. Messina8, K. Micheneau15, Kate C. Miller18, A. Molinario, K. Morå2, Y. Mosbacher13, M. Murra5, J. Naganoma22, Kaixuan Ni17, Uwe Oberlack4, K. Odgers10, J. Palacio15, Bart Pelssers2, R. Peres9, J. Pienaar18, V. Pizzella12, Guillaume Plante1, R. Podviianiuk, J. Qin16, H. Qiu13, D. Ramírez García14, S. Reichard9, B. Riedel18, A. Rocchetti14, N. Rupp12, J.M.F. dos Santos6, Gabriella Sartorelli3, N. Šarčević14, M. Scheibelhut4, S. Schindler4, J. Schreiner12, D. Schulte5, Marc Schumann14, L. Scotto Lavina20, M. Selvi3, P. Shagin22, E. Shockley18, Manuel Gameiro da Silva6, H. Simgen12, C. Therreau15, Dominique Thers15, F. Toschi14, Gian Carlo Trinchero7, C. Tunnell22, N. Upole18, M. Vargas5, G. Volta9, O. Wack12, Hongwei Wang23, Yuehuan Wei17, Ch. Weinheimer5, D. Wenz4, C. Wittweg5, J. Wulf9, J. Ye17, Yanxi Zhang1, T. Zhu1, J. P. Zopounidis20 
TL;DR: Constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment are reported, and no DM or CEvNS detection may be claimed because the authors cannot model all of their backgrounds.
Abstract: We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment. We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of (22±3) tonne day. Above ∼0.4 keVee, we observe 30 MeV/c2, and absorption of dark photons and axionlike particles for mχ within 0.186–1 keV/c2.

412 citations

Journal ArticleDOI
TL;DR: Asplund et al. as mentioned in this paper used spectral lines of all the indicators of the abundances present in the solar photospheric spectrum, from a discussion of the atomic and molecular data, and from an analysis of these lines based on a new 3D model of the solar outer layers, taking non-LTE effects into account when possible.
Abstract: We have very recently re-determined the abundances of nearly all the available chemical elements in the solar photosphere, from lithium to thorium (Asplund et al. Annu. Rev. Astron. Astrophys. 47, 481 (2009)). This new complete and homogeneous analysis results from a very careful selection of spectral lines of all the indicators of the abundances present in the solar photospheric spectrum, from a discussion of the atomic and molecular data, and from an analysis of these lines based on a new 3D model of the solar outer layers, taking non-LTE effects into account when possible. We present these new results, compare them with other recent solar data as well as with recent results for the solar neighborhood, and discuss some of their most important implications as well as some of the atomic data we still urgently need.

411 citations


Authors

Showing all 21326 results

NameH-indexPapersCitations
Hongjie Dai197570182579
Hyun-Chul Kim1764076183227
Richard S. Ellis169882136011
Stanley B. Prusiner16874597528
Anders Björklund16576984268
Yang Yang1642704144071
Tomas Hökfelt158103395979
Bengt Winblad1531240101064
Zhenwei Yang150956109344
Marvin Johnson1491827119520
Jan-Åke Gustafsson147105898804
Markus Ackermann14661071071
Hans-Olov Adami14590883473
Markku Kulmala142148785179
Kjell Fuxe142147989846
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023158
2022537
20213,664
20203,602
20193,347
20183,092