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| 001 | 395478 | ||
| 005 | 20211110145213.0 | ||
| 020 | _ | _ | |a 978-3-945931-06-6 |
| 020 | _ | _ | |a 978-3-945931-06-6 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2009-03/Naganoma_Junji |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2017-12143 |
| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-PROC-2016-03 |
| 088 | _ | _ | |a DESY-PROC-2016-03 |2 DESY |
| 100 | 1 | _ | |a Naganoma, Junji |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 12th Patras Workshop on Axions, WIMPs and WISPs |c Jeju Island |d 2016-06-20 - 2016-06-24 |g AXION-WIMP 2016 |0 C16-06-20.4 |2 inspire |w South Korea |
| 245 | _ | _ | |a Status of the XENON Experiments |
| 260 | _ | _ | |a Hamburg |c 2017 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Naganoma, Junji "Status of the XENON Experiments" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20 - 2016-06-24, Jeju Island |
| 300 | _ | _ | |a 53-56 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
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| 336 | 7 | _ | |a Report |0 PUB:(DE-HGF)29 |2 PUB:(DE-HGF) |m report |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1513261385_4670 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a Contribution to a book |0 PUB:(DE-HGF)7 |2 PUB:(DE-HGF) |m contb |
| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 520 | _ | _ | |a The XENON experiments search for weakly interacting massive particles (WIMPs) using dual-phase xenon time projection chambers. While the XENON100 experiment completed its science program, the next ton-scale experiment, XENON1T, is fully installed and moving towards science data-taking. The most recent results of the collaboration are presented: from XENON100 latest analysis on low mass WIMPs to XENON1T status and its projected sensitivity, that has been evaluated to reach a minimum cross section of $1.6\times10^{-47}$~cm$^2$ at a WIMP mass of 50~GeV$/c^2$ after 2~years exposure with 1~ton of fiducial volume. |
| 536 | _ | _ | |a 899 - ohne Topic (POF3-899) |0 G:(DE-HGF)POF3-899 |c POF3-899 |f POF III |x 0 |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a XENON Collaboration |0 P:(DE-HGF)0 |b 1 |e Collaboration author |
| 787 | 0 | _ | |a Kim, Younglm et. al. |d Verlag Deutsches Elektronen-Synchrotron |i isPartOf |0 PUBDB-2017-11637 |r DESY-PROC-2016-03 |t 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/395478/files/fulltext.pdf |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:395478 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a Rice University - Houston - USA |b 0 |
| 913 | 1 | _ | |a DE-HGF |b Programmungebundene Forschung |l ohne Programm |1 G:(DE-HGF)POF3-890 |0 G:(DE-HGF)POF3-899 |2 G:(DE-HGF)POF3-800 |v ohne Topic |x 0 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 914 | 1 | _ | |y 2017 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 4.0 |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |
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| 980 | 1 | _ | |a FullTexts |
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