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| 001 | 295122 | ||
| 005 | 20211110133409.0 | ||
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| 088 | 1 | _ | |a DESY-PROC-2011-04 |
| 088 | _ | _ | |a DESY-PROC-2011-04 |2 DESY |
| 100 | 1 | _ | |a Moulin, Emmanuel |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 7th Patras Workshop on Axions, WIMPs and WISPs |g AXION-WIMP 2011 |c Mykonos |d 2011-06-27 - 2011-07-01 |w Greece |
| 245 | _ | _ | |a Prospects for dark matter searches with CTA |
| 260 | _ | _ | |c 2011 |b Deutsches Elektronen-Synchrotron, DESY |a Hamburg |
| 300 | _ | _ | |a 27-30 |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
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| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 520 | _ | _ | |a Dark matter particle annihilations are expected to occur in dense regions of the universe. Among the final annihilation products are very high energy gamma rays. The future array of Imaging Atmospheric Cherenkov Telescopes (IACTs), i.e. the Cherenkov Telescope Array (CTA), is a well-suited instrument to look further for particle dark matter annihilations in the 10 GeV - 100 TeV range. Here, I will present CTA prospective studies for targeted and wide-field survey searches. |
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| 773 | _ | _ | |a 10.3204/DESY-PROC-2011-04/moulin_emmanuel |
| 787 | 0 | _ | |a Schumann, Marc et.al. |d 2011 |i IsPartOf |0 PUBDB-2016-01039 |r DESY-PROC-2011-04 |t Proceedings, 7th Patras Workshop on Axions, WIMPs and WISPs |
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