User Tools

Site Tools


swgo_rel_pub

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
swgo_rel_pub [2019/10/28 19:40]
swgowikiadmin [Contributions to the ASTRO2020 decadal survey]
swgo_rel_pub [2021/02/10 11:06] (current)
elisaprandini
Line 2: Line 2:
 ~~NOTOC~~ ~~NOTOC~~
  
----- 
 ==== Conference Proceedings ==== ==== Conference Proceedings ====
-  * //A next-generation ground-based wide field-of-view gamma-ray observatory in the southern hemisphere//,​ H. Schoorlemmer (on behalf of the SWGO collaboration),​ [[https://​pos.sissa.it/​358/​785/​pdf|PoS(ICRC2019)785]]+  * //A next-generation ground-based wide field-of-view gamma-ray observatory in the southern hemisphere//,​ H. Schoorlemmer (on behalf of the SWGO collaboration), Proceedings of ICRC 2019, [[https://​pos.sissa.it/​358/​785/​pdf|PoS(ICRC2019)785]] 
 +  * //The Southern Wide-Field Gamma-ray Observatory (SWGO)//, Proceedings of IWARA 2020 Virtual Conference, Ulisses Barres de Almeida (for the SWGO Collaboration),​ [[https://​arxiv.org/​abs/​2012.13740]]
  
  
------ +====== Related publications =====
-===== Related publications =====+==== SWGO-related papers (Cat3) ==== 
 +  * //Detection of VHE gamma-ray transients with monitoring facilities//,​ G. La Mura et al. MNRAS 497 (2020) 3, [[https://​arxiv.org/​abs/​2001.04503]] 
 ==== Science case white paper ==== ==== Science case white paper ====
  
-  * //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 ​=== +**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]] 
-  * //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**
-=== 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}}
Line 26: Line 28:
 ==== 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]]+  * //Characteristics of extensive air showers around the energy threshold for ground-particle-based γ-ray observatories//H. Schoorlemmer,​ J.A. Hinton, R. López-Coto. ​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]]
 +
 ==== Detector Design and Prototyping ==== ==== Detector Design and Prototyping ====
  
Line 35: Line 38:
   * //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]]
- 
- 
------- 
- 
-[[:​imprint|Imprint]] & 
-[[:​datenschutzhinweis|Datenschutzhinweis / Privacy Policy]] 
  
swgo_rel_pub.1572288054.txt.gz · Last modified: 2019/10/28 19:40 by swgowikiadmin