swgo_rel_pub
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swgo_rel_pub [2019/10/16 10:58] swgowikiadmin [Detector Design and Prototyping] |
swgo_rel_pub [2020/04/28 14:35] fwerner [Detector Design and Prototyping] |
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| * //Science Case for a Wide Field-of-View Very-High-Energy Gamma-Ray Observatory in the Southern Hemisphere//, SGSO-alliance, [[https://arxiv.org/abs/1902.08429|arXiv:1902.08429]] | * //Science Case for a Wide Field-of-View Very-High-Energy Gamma-Ray Observatory in the Southern Hemisphere//, SGSO-alliance, [[https://arxiv.org/abs/1902.08429|arXiv:1902.08429]] | ||
| ==== Contributions to the ASTRO2020 decadal survey ==== | ==== Contributions to the ASTRO2020 decadal survey ==== | ||
| + | === Instrument === | ||
| + | |||
| + | * //The Southern Wide-Field Gamma-Ray Observatory (SWGO): A Next-Generation Ground-Based Survey Instrument for VHE Gamma-Ray Astronomy //. Petra Huentemeyer //et al//., [[https://arxiv.org/abs/1907.07737|arXiv:1907.07737]] | ||
| + | === Science cases === | ||
| * //All-Sky time domain astrophysics with Very High Energy Gamma raysmisphere, //K. Satalecka + F. Schüssler et al., {{:decadalsurveyastro2020_transientssgso.pdf|DecadalSurveyASTRO2020_TransientsSGSO.pdf}} | * //All-Sky time domain astrophysics with Very High Energy Gamma raysmisphere, //K. Satalecka + F. Schüssler et al., {{:decadalsurveyastro2020_transientssgso.pdf|DecadalSurveyASTRO2020_TransientsSGSO.pdf}} | ||
| * //Searching for Sources of TeV Particle Dark Matter in the Southern Hemisphere//, A. Albert et al., \\ {{:albertandream.pdf|DecadalSurveyASTRO2020_DM_Sources.pdf}} | * //Searching for Sources of TeV Particle Dark Matter in the Southern Hemisphere//, A. Albert et al., \\ {{:albertandream.pdf|DecadalSurveyASTRO2020_DM_Sources.pdf}} | ||
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| ==== General considerations ==== | ==== General considerations ==== | ||
| - | * H. Schoorlemmer, J.A. Hinton, R. López-Coto.“Characteristics of extensive air showers around the energy threshold for ground-particle-based γ-ray observatories”, Eur. Phys. J. C (2019) 79: 427. doi:[[https://doi.org/10.1140/epjc/s10052-019- 6942-x|https://doi.org/10.1140/epjc/s10052-019- 6942-x]] | + | * H. Schoorlemmer, J.A. Hinton, R. López-Coto.“Characteristics of extensive air showers around the energy threshold for ground-particle-based γ-ray observatories”, Eur. Phys. J. C (2019) 79: 427. doi:[[https://doi.org/10.1140/epjc/s10052-019-6942-x|https://doi.org/10.1140/epjc/s10052-019-6942-x]] |
| * //Baseline Design for a Next Generation Wide-Field-of-View Very-High-Energy Gamma Ray Observatory//, H. Schoorlemmer, R. Lopez-Coto and J. Hinton,[[https://pos.sissa.it/301/819/|PoS(ICRC2017)819]] | * //Baseline Design for a Next Generation Wide-Field-of-View Very-High-Energy Gamma Ray Observatory//, H. Schoorlemmer, R. Lopez-Coto and J. Hinton,[[https://pos.sissa.it/301/819/|PoS(ICRC2017)819]] | ||
| * //On the scientific motivation for a wide field-of-view TeV gamma-ray observatory in the Southern Hemisphere//, M. Mostafa, S. BenZvi, H. Schoorlemmer, F. Schüssler on behalf of the HAWC Collaboration,[[https://pos.sissa.it/301/851/|PoS(ICRC2017)851]] | * //On the scientific motivation for a wide field-of-view TeV gamma-ray observatory in the Southern Hemisphere//, M. Mostafa, S. BenZvi, H. Schoorlemmer, F. Schüssler on behalf of the HAWC Collaboration,[[https://pos.sissa.it/301/851/|PoS(ICRC2017)851]] | ||
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| * //The overview of the ALPACA Experiment//, M. Ohnishi,[[https://pos.sissa.it/301/827/|PoS(ICRC2017)827]] | * //The overview of the ALPACA Experiment//, M. Ohnishi,[[https://pos.sissa.it/301/827/|PoS(ICRC2017)827]] | ||
| * //Simulation study for the proposed wide field-of-view gamma-ray detector array ALTO//, S. Thoudam, Y. Becherini and M. Punch,[[https://pos.sissa.it/301/780/|PoS(ICRC2017)780]] | * //Simulation study for the proposed wide field-of-view gamma-ray detector array ALTO//, S. Thoudam, Y. Becherini and M. Punch,[[https://pos.sissa.it/301/780/|PoS(ICRC2017)780]] | ||
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| - | [[:imprint|Imprint]] & | ||
| - | [[:datenschutzhinweis|Datenschutzhinweis / Privacy Policy]] | ||
swgo_rel_pub.txt · Last modified: 2023/04/14 14:24 by hinton
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