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The ARGO-YBJ detector and high energy GRBs
Bacci, C; Bao, KZ; Barone, F; Bartoli, B; Bastieri, D; Bernardini, P; Buonomo, R; Bussino, S; Calloni, E; Cao, BY; Cardarelli, R; Catalanotti, S; Cavaliere, A; Cesaroni, F; Creti, P; Danzengluobu; Piazzoli, BD; De Vincenzi, M; Di Girolamo, T; Di Sciascio, G; Feng, ZY; Fu, Y; Gao, XY; Geng, QX; Guo, HW; He, HH; He, M; Huang, Q; Iacovacci, M; Iucci, N; Jai, HY; Kong, FM; Kuang, HH; Labaciren; Li, B; Li, JY; Liu, ZQ; Lu, H; Ma, XH; Mancarella, G; Mari, SM; Marsella, G; Martello, D; Mei, DM; Meng, XR; Milano, L; Morselli, A; Mu, J; Oliviero, M; Padovani, P; Panareo, M; Parisi, M; Pellizzoni, G; Peng, ZR; Pistilli, P; Santonico, R; Sartori, G; Sbarra, C; Severino, G; Shen, PR; Sparvoli, R; Stanescu, C; Su, J; Sun, LR; Sun, SC; Surdo, A; Tan, YH; Vernetto, S; Vietri, M; Wang, CR; Wang, H; Wang, HY; Wei, YN; Yang, HT; Yao, QK; Yu, GC; Yue, XD; Yuan, AF; Zhang, HM; Zhang, JL; Zhang, NJ; Zhang, TJ; Zhang, XY; Zhaxisangzhu; Zhaxiciren; Zhu, QQ; Kuang HH(况浩怀); Lu H(卢红); Ma XH(马欣华); Zhu QQ(朱清琪)
Corresponding AuthorCNR, Ist Cosmogeofis, I-10133 Turin, Italy ; Ist Nazl Fis Nucl, I-10125 Turin, Italy ; Ist Nazl Fis Nucl, I-80125 Naples, Italy ; Univ Roma Tre, Dipartimento Fis, Rome, Italy ; Zhengzhou Univ, Henan, Peoples R China ; Univ Naples, Dipartimento Fis, I-80138 Naples, Italy ; Ist Nazl Fis Nucl, Naples, Italy ; Ist Nazl Fis Nucl, Padua, Italy ; Univ Padua, Padua, Italy ; Ist Nazl Fis Nucl, I-73100 Lecce, Italy ; Univ Lecce, Dipartimento Fis, I-73100 Lecce, Italy ; Shandong Univ, Jinan 250100, Peoples R China ; Univ Rome Tor Vergata, Dipartimento Fis, Rome, Italy ; Ist Nazl Fis Nucl, Rome, Italy ; Tibet Univ, Lhassa, Peoples R China ; SW Jiaotong Univ, Chengdu, Peoples R China ; Yunnan Univ, Kunming 650091, Peoples R China ; IHEP, Beijing, Peoples R China ; Univ Basilicata, I-85100 Potenza, Italy ; Osservatorio Astron Capodimonte, I-80131 Naples, Italy
SubtypeArticle; Proceedings Paper
AbstractARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimized to study small size air showers. It consists of a layer of Resistive Plate Counters (RPCs) covering an area of similar to 6500 m(2) and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m a.s.l. ARGO-YBJ will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics in the range 10 GeV divided by 500 TeV. The sensitivity of ARGO-YBJ to detect high energy GRBs is presented.
Subject AreaAstronomy & Astrophysics
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000083156100092
ADS Bibcode1999A&AS..138..597B
ADS URLhttps://ui.adsabs.harvard.edu/abs/1999A&AS..138..597B
ADS CITATIONShttps://ui.adsabs.harvard.edu/abs/1999A&AS..138..597B/citations
Citation statistics
Cited Times:13[WOS]   [WOS Record]     [Related Records in WOS]
Cited Times:7 [INSPIRE]
Cited Times:8 [ADS]
Document Type期刊论文
First Author AffilicationInstitute of High Energy
Recommended Citation
GB/T 7714
Bacci, C,Bao, KZ,Barone, F,et al. The ARGO-YBJ detector and high energy GRBs[J]. ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES,1999,138(3):597-598.
APA Bacci, C.,Bao, KZ.,Barone, F.,Bartoli, B.,Bastieri, D.,...&朱清琪.(1999).The ARGO-YBJ detector and high energy GRBs.ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES,138(3),597-598.
MLA Bacci, C,et al."The ARGO-YBJ detector and high energy GRBs".ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES 138.3(1999):597-598.
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