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| 001 | 315505 | ||
| 005 | 20211110140134.0 | ||
| 020 | _ | _ | |a 978-3-935702-59-1 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2014-03/dreyling-eschweiler_jan |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 024 | 7 | _ | |a arXiv:1409.6992 |2 arXiv |
| 024 | 7 | _ | |a inspire:1318810 |2 inspire |
| 037 | _ | _ | |a PUBDB-2016-05912 |
| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-14-165; arXiv:1409.6992 |
| 088 | 1 | _ | |a DESY-14-165 |
| 088 | _ | _ | |a DESY-14-165 |2 DESY |
| 088 | _ | _ | |a arXiv:1409.6992 |2 arXiv |
| 088 | _ | _ | |a DESY-14-165 |2 DESY |
| 100 | 1 | _ | |a Dreyling-Eschweiler, Jan |0 P:(DE-H253)PIP1006425 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 10th Patras Workshop on Axions, WIMPs and WISPs |c Geneva |d 2014-06-29 - 2014-07-04 |g AXION-WIMP 2014 |0 C14-06-29.1 |2 inspire |w Switzerland |
| 245 | _ | _ | |a First sensitivity limits of the ALPS TES detector |
| 260 | _ | _ | |a Hamburg |c 2014 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva |
| 300 | _ | _ | |a 63-66 |
| 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 Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1512395239_3384 |2 PUB:(DE-HGF) |
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| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 500 | _ | _ | |a 4 pages, 1 figure; proceedings of 10th Patras Workshop on Axions, WIMPs, and WISPs, Geneva, CERN, 29 June to 4 July 2014 |
| 520 | _ | _ | |a The Any Light Particle Search II (ALPS II) requires a sensitive detection of 1064~nm photons. Thus, a low dark count rate ($DC$) and a high detection efficiency ($DE$) is needed. ALPS has set up a transition-edge sensor (TES) detector system, namely the ALPS TES detector. It is found that thermal photons from room temperature surfaces are the main contribution of dark counts for 1064~nm photon signals. Furthermore, the current setup of the ALPS TES detector shows an improvement compared to using the ALPS I detector. |
| 536 | _ | _ | |a 514 - Theoretical Particle Physics (POF2-514) |0 G:(DE-HGF)POF2-514 |c POF2-514 |f POF II |x 0 |
| 588 | _ | _ | |a Dataset connected to INSPIRE |
| 650 | _ | 7 | |a photon: thermal |2 INSPIRE |
| 650 | _ | 7 | |a temperature: surface |2 INSPIRE |
| 650 | _ | 7 | |a ALPS |2 INSPIRE |
| 650 | _ | 7 | |a sensitivity |2 INSPIRE |
| 650 | _ | 7 | |a efficiency |2 INSPIRE |
| 650 | _ | 7 | |a photon: detector |2 INSPIRE |
| 650 | _ | 7 | |a detector: superconductivity |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-H253)ALPS-20150101 |5 EXP:(DE-H253)ALPS-20150101 |e Any Light Particle Search |x 0 |
| 700 | 1 | _ | |a ALPS-II Collaboration |0 P:(DE-HGF)0 |b 1 |e Collaboration author |
| 787 | 0 | _ | |a Tsesmelis, Emmanuel et. al. |d Verlag Deutsches Elektronen-Synchrotron |i isPartOf |0 PUBDB-2016-05897 |r DESY-PROC-2014-03 |t Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014 |
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