000600424 001__ 600424
000600424 005__ 20250715171428.0
000600424 0247_ $$2doi$$a10.22323/1.454.0055
000600424 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-07981
000600424 0247_ $$2altmetric$$aaltmetric:163849617
000600424 0247_ $$2openalex$$aopenalex:W4393902625
000600424 037__ $$aPUBDB-2023-07981
000600424 041__ $$aEnglish
000600424 082__ $$a530
000600424 1001_ $$0P:(DE-H253)PIP1089678$$aSchwemmbauer, Christina$$b0$$eCorresponding author
000600424 1112_ $$a1st General Meeting and 1st Training School of the COST Action COSMIC WISPers$$cBari and Lecce$$d2023-09-05 - 2023-09-14$$g(COSMICWISPers)$$wItaly
000600424 245__ $$aSimulations for direct dark matter searches using ALPS II’s TES detection system
000600424 260__ $$aTrieste$$bSISSA$$c2024
000600424 300__ $$a6
000600424 3367_ $$2ORCID$$aCONFERENCE_PAPER
000600424 3367_ $$033$$2EndNote$$aConference Paper
000600424 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000600424 3367_ $$2BibTeX$$aINPROCEEDINGS
000600424 3367_ $$2DRIVER$$aconferenceObject
000600424 3367_ $$2DataCite$$aOutput Types/Conference Paper
000600424 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1726055329_2596926
000600424 520__ $$aTransition Edge Sensors (TES) are superconducting microcalorimeters that can be used for single-photon detection with extremely low backgrounds. When they are within their superconducting transition region, small temperature fluctuations—like the energy deposited by single photons—lead to large resistance variations. These variations can be measured using Superconducting Quantum Interference Devices (SQUIDs). This technology is planned to be used as a single photon detector for later runs of the ALPS II experiment, a light-shining-through-walls experiment at DESY Hamburg, searching for Axion-Like Particles (ALPs), which are possible Dark Matter (DM)candidates. Due to the very low dark count rates in our setup, our TES system might be viable for direct DM searches at sub-MeV masses through electron-scattering of DM in the superconducting chip, as well. Simulations concerning background rejection and calibration methods demonstrate the needed sub-eV sensitivity already. 
000600424 536__ $$0G:(DE-HGF)POF4-611$$a611 - Fundamental Particles and Forces (POF4-611)$$cPOF4-611$$fPOF IV$$x0
000600424 536__ $$0G:(EU-Grant)948689$$aAxionDM - Searching for axion and axion-like-particle dark matter in the laboratory and with high-energy astrophysical observations (948689)$$c948689$$fERC-2020-STG$$x1
000600424 536__ $$0G:(GEPRIS)390833306$$aDFG project 390833306 - EXC 2121: Quantum Universe (390833306)$$c390833306$$x2
000600424 588__ $$aDataset connected to CrossRef Conference
000600424 693__ $$0EXP:(DE-H253)ALPS-20150101$$5EXP:(DE-H253)ALPS-20150101$$eAny Light Particle Search$$x0
000600424 7001_ $$0P:(DE-HGF)0$$aHochberg, Yonit$$b1
000600424 7001_ $$0P:(DE-HGF)0$$aIsleif, Katharina-Sophie$$b2
000600424 7001_ $$0P:(DE-H253)PIP1005478$$aJanuschek, Friederike$$b3
000600424 7001_ $$0P:(DE-HGF)0$$aLehmann, Benjamin V.$$b4
000600424 7001_ $$0P:(DE-H253)PIP1003168$$aLindner, Axel$$b5
000600424 7001_ $$0P:(DE-H253)PIP1089089$$aMeyer, Manuel$$b6
000600424 7001_ $$0P:(DE-H253)PIP1098835$$aOthman, Gulden$$b7
000600424 7001_ $$0P:(DE-H253)PIP1089473$$aRubiera Gimeno, José Alejandro$$b8
000600424 77318 $$2Crossref$$3proceedings-article$$a10.22323/1.454.0055$$bSissa Medialab$$d2024-04-03$$p055$$tProceedings of 1st General Meeting and 1st Training School of the COST Action COSMIC WSIPers — PoS(COSMICWISPers)$$y2024
000600424 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.454.0055$$p055$$tProceedings of Science / International School for Advanced Studies$$v(COSMICWISPers)$$x1824-8039$$y2024
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/CosmicWISPersTrainingSchool2023_Schwemmbauer.pdf$$yOpenAccess$$zStatID:(DE-HGF)0510
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/HTML-Approval_of_scientific_publication.html
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/PDF-Approval_of_scientific_publication.pdf
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/COSMICWISPers_055.pdf$$yRestricted$$zStatID:(DE-HGF)0599
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/COSMICWISPers_055.pdf?subformat=pdfa$$xpdfa$$yRestricted$$zStatID:(DE-HGF)0599
000600424 8564_ $$uhttps://bib-pubdb1.desy.de/record/600424/files/CosmicWISPersTrainingSchool2023_Schwemmbauer.pdf?subformat=pdfa$$xpdfa$$yOpenAccess$$zStatID:(DE-HGF)0510
000600424 909CO $$ooai:bib-pubdb1.desy.de:600424$$pdnbdelivery$$pec_fundedresources$$pVDB$$pdriver$$popen_access$$popenaire
000600424 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1089678$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000600424 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1005478$$aDeutsches Elektronen-Synchrotron$$b3$$kDESY
000600424 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1003168$$aDeutsches Elektronen-Synchrotron$$b5$$kDESY
000600424 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1089089$$aExternal Institute$$b6$$kExtern
000600424 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1098835$$aExternal Institute$$b7$$kExtern
000600424 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1089473$$aDeutsches Elektronen-Synchrotron$$b8$$kDESY
000600424 9131_ $$0G:(DE-HGF)POF4-611$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vFundamental Particles and Forces$$x0
000600424 9141_ $$y2024
000600424 915__ $$0LIC:(DE-HGF)CCBYNCND4$$2HGFVOC$$aCreative Commons Attribution-NonCommercial-NoDerivs CC BY-NC-ND 4.0
000600424 915__ $$0StatID:(DE-HGF)0501$$2StatID$$aDBCoverage$$bDOAJ Seal$$d2021-04-20T14:42:38Z
000600424 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ$$d2021-04-20T14:42:38Z
000600424 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000600424 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bDOAJ : Editorial review$$d2021-04-20T14:42:38Z
000600424 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2025-01-02
000600424 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2025-01-02
000600424 9201_ $$0I:(DE-H253)ALPS-20130318$$kALPS$$lAny Light Particle Search$$x0
000600424 980__ $$acontrib
000600424 980__ $$aVDB
000600424 980__ $$aUNRESTRICTED
000600424 980__ $$ajournal
000600424 980__ $$aI:(DE-H253)ALPS-20130318
000600424 9801_ $$aFullTexts