6533b82efe1ef96bd12929aa
RESEARCH PRODUCT
The ARGO-YBJ Experiment Progresses and Future Extension
Aielli GBacci CBartoli BBernardini PBi XjBleve CBranchini PBudano ACalabrese Melcarne AkCamarri PCao ZCappa ACardarelli RCatalanotti SCattaneo CCelio PChen SzChen TlChen YCheng NCreti PCui SwDai BzD'ali Staiti GDanzengluobuDattoli MDe Mitri ID'ettorre Piazzoli BMario De VincenziDi Girolamo TDing XhDi Sciascio GFeng CfFeng Zhao YangFeng Zhen YongGaleazzi FGaleotti PGargana RGou QbGuo YqHe HhHu HaibingHu Hong BoHuang QIacovacci MIuppa RJames IJia HyLabacirenLi HjLi JyLi XxLiberti BLiguori GLiu CLiu CqLiu MyLiu JLu HMa XhMancarella GMarsella GMartello DMastroianni SMeng XrMontini PNing CcPagliaro APanareo MPerrone LPistilli PQu XbRossi ERuggieri FSaggese LSalvini PSantonico RShen PrSheng XdShi FStanescu CSurdo ATan YhVallania PVernetto SVigorito CWang BWang HWu CyWu HrXu BXue LYan YxYang QyYang XcYuan AfZha MZhang HmZhang Ji LongZhang Jian LiZhang LZhang PZhang XyZhang YZhaxisangzhuZhou XxZhu FrZhu QqZizzi G.Severino Angelo Maria BussinoStefano Maria Marisubject
PhotonGamma ray source cosmic ray origin detector arraymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationDetector arrayFOS: Physical sciencesCosmic rayAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)detector arrayUltra-high-energy cosmic rayeducationMathematical Physicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studyDetectorGamma ray sourceAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicscosmic ray originCosmic ray originAir showerSpace and Planetary ScienceSkyAstrophysics - High Energy Astrophysical Phenomenadescription
Gamma ray source detection above 30 TeV is an encouraging approach for finding galactic cosmic ray origins. All sky survey for gamma ray sources using wide field of view detector is essential for population accumulation for various types of sources above 100 GeV. To target the goals, the ARGO-YBJ experiment has been established. Significant progresses have been made in the experiment. A large air shower detector array in an area of 1 km2 is proposed to boost the sensitivity. Hybrid detections with multi-techniques will allow a good discrimination between different types of primary particles, including photons and protons, thus enable an energy spectrum measurement for individual species. Fluorescence light detector array will extend the spectrum measurement to 100 PeV and higher where the second knee is located. An energy scale determined by balloon experiments at 10 TeV will be propagated to ultra high energy cosmic ray experiments.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2010-06-22 |