000408353 001__ 408353
000408353 005__ 20211110151244.0
000408353 010__ $$a
000408353 020__ $$a978-3-935702-83-6
000408353 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/redondo_javier
000408353 0247_ $$2ISSN$$a1435-8077
000408353 037__ $$aPUBDB-2018-02806
000408353 041__ $$aEnglish
000408353 0881_ $$aDESY-PROC-2013-04
000408353 088__ $$2DESY$$aDESY-PROC-2013-04
000408353 1001_ $$0P:(DE-H253)PIP1016726$$aDoebrich, Babette$$b0$$udesy
000408353 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408353 245__ $$aDark Matter - a light move
000408353 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408353 29510 $$aDöbrich, B. "Dark Matter - a light move" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408353 300__ $$a165-169
000408353 3367_ $$2ORCID$$aCONFERENCE_PAPER
000408353 3367_ $$033$$2EndNote$$aConference Paper
000408353 3367_ $$2BibTeX$$aINPROCEEDINGS
000408353 3367_ $$2DRIVER$$aconferenceObject
000408353 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000408353 3367_ $$2DataCite$$aOutput Types/Conference Paper
000408353 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1538476330_22172
000408353 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000408353 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000408353 520__ $$aThis proceedings contribution reports from the workshop Dark Matter - a light  move, held at DESY Hamburg in June 2013. Dark Matter particle candidates span a huge parameter range. In particular, well motivated candidates exist also in the sub-eV mass region, for example the axion. Whilst a plethora of setups searches for rather heavy Dark Matter particles, to this date only very few experiments aimed at direct detection of sub-eV Dark Matter exist. The aim of our workshop was to discuss if and how this could be changed in the near future.
000408353 536__ $$0G:(DE-HGF)POF3-899$$a899 - ohne Topic (POF3-899)$$cPOF3-899$$fPOF III$$x0
000408353 588__ $$aDataset connected to GVK
000408353 650_7 $$0(DE-588)4220935-3$$2gnd$$aHypothetisches Teilchen
000408353 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000408353 7001_ $$0P:(DE-HGF)0$$aRedondo, J.$$b1$$eCorresponding author
000408353 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
000408353 8564_ $$uhttps://bib-pubdb1.desy.de/record/408353/files/fulltext.pdf$$yOpenAccess
000408353 909CO $$ooai:bib-pubdb1.desy.de:408353$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000408353 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1016726$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000408353 9131_ $$0G:(DE-HGF)POF3-899$$1G:(DE-HGF)POF3-890$$2G:(DE-HGF)POF3-800$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bProgrammungebundene Forschung$$lohne Programm$$vohne Topic$$x0
000408353 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000408353 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000408353 9201_ $$0I:(DE-H253)L-20120731$$kL$$lBibliothek und Dokumentation$$x0
000408353 980__ $$acontrib
000408353 980__ $$aVDB
000408353 980__ $$aUNRESTRICTED
000408353 980__ $$areport
000408353 980__ $$acontb
000408353 980__ $$aI:(DE-H253)L-20120731
000408353 9801_ $$aFullTexts