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| 001 | 395488 | ||
| 005 | 20211110145214.0 | ||
| 020 | _ | _ | |a 978-3-945931-06-6 |
| 020 | _ | _ | |a 978-3-945931-06-6 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2009-03/Meyer_Manuel |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2017-12153 |
| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-PROC-2016-03 |
| 088 | _ | _ | |a DESY-PROC-2016-03 |2 DESY |
| 100 | 1 | _ | |a Meyer, Manuel |0 P:(DE-H253)PIP1089089 |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 Searches for Axionlike Particles Using $\gamma$-RayObservations |
| 260 | _ | _ | |a Hamburg |c 2017 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Meyer, Manuel "Searches for Axionlike Particles Using $\gamma$-RayObservations" 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 102-111 |
| 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 1513676029_7217 |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 Axionlike particles (ALPs) are a common prediction of theories beyond the Standard Model of particle physics that could explain the entirety of the cold dark matter. These particles could be detected through their mixing with photons in external electromagnetic fields. Here, we provide a short review over ALP searches that utilize astrophysical $\gamma$-ray observations. We summarize current bounds as well as future sensitivities and discuss the possibility that ALPs alter the $\gamma$-ray opacity of the Universe. |
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| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 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/395488/files/fulltext.pdf |y OpenAccess |
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| 910 | 1 | _ | |a Externes Institut |0 I:(DE-HGF)0 |k Extern |b 0 |6 P:(DE-H253)PIP1089089 |
| 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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