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Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode

The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a “full coverage” (central carpet with an active area of ∼93%) air shower array dedicated to gamma-ray astronomy and cosmic-ray studies. The wide field of view (∼2 sr) and high duty cycle (>...

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Autores principales: Bartoli, B., Bernardini, P., Bi, X.J., Cao, Z., Catalanotti, S., Chen, S.Z., Chen, T.L., Cui, S.W., Dai, B.Z., D'Amone, A., Danzengluobu, De Mitri, I., Ettorre Piazzoli, B.D., Girolamo, T.Di, Di Sciascio, G., Feng, C.F., Feng, Zhaoyang, Feng, Zhenyong, Gao, W., Gou, Q.B., Guo, Y.Q., He, H.H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H.Y., Labaciren, Li, H.J., Liu, C., Liu, J., Liu, M.Y., Lu, H., Ma, L.L., Ma, X.H., Mancarella, G., Mari, S.M., Marsella, G., Mastroianni, S., Montini, P., Ning, C.C., Perrone, L., Pistilli, P., Salvini, P., Santonico, R., Shen, P.R., Sheng, X.D., Shi, F., Surdo, A., Tan, Y.H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C.Y., Wu, H.R., Xue, L., Yang, Q.Y., Yang, X.C., Yao, Z.G., Yuan, A.F., Zha, M., Zhang, H.M., Zhang, L., Zhang, X.Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X.X., Zhu, F.R., Zhu, Q.Q.
Lenguaje:eng
Publicado: 2017
Materias:
Acceso en línea:https://dx.doi.org/10.3847/1538-4357/aa74bc
http://cds.cern.ch/record/2260719
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author Bartoli, B.
Bernardini, P.
Bi, X.J.
Cao, Z.
Catalanotti, S.
Chen, S.Z.
Chen, T.L.
Cui, S.W.
Dai, B.Z.
D'Amone, A.
Danzengluobu
De Mitri, I.
Ettorre Piazzoli, B.D.
Girolamo, T.Di
Di Sciascio, G.
Feng, C.F.
Feng, Zhaoyang
Feng, Zhenyong
Gao, W.
Gou, Q.B.
Guo, Y.Q.
He, H.H.
Hu, Haibing
Hu, Hongbo
Iacovacci, M.
Iuppa, R.
Jia, H.Y.
Labaciren
Li, H.J.
Liu, C.
Liu, J.
Liu, M.Y.
Lu, H.
Ma, L.L.
Ma, X.H.
Mancarella, G.
Mari, S.M.
Marsella, G.
Mastroianni, S.
Montini, P.
Ning, C.C.
Perrone, L.
Pistilli, P.
Salvini, P.
Santonico, R.
Shen, P.R.
Sheng, X.D.
Shi, F.
Surdo, A.
Tan, Y.H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, H.
Wu, C.Y.
Wu, H.R.
Xue, L.
Yang, Q.Y.
Yang, X.C.
Yao, Z.G.
Yuan, A.F.
Zha, M.
Zhang, H.M.
Zhang, L.
Zhang, X.Y.
Zhang, Y.
Zhao, J.
Zhaxiciren
Zhaxisangzhu
Zhou, X.X.
Zhu, F.R.
Zhu, Q.Q.
author_facet Bartoli, B.
Bernardini, P.
Bi, X.J.
Cao, Z.
Catalanotti, S.
Chen, S.Z.
Chen, T.L.
Cui, S.W.
Dai, B.Z.
D'Amone, A.
Danzengluobu
De Mitri, I.
Ettorre Piazzoli, B.D.
Girolamo, T.Di
Di Sciascio, G.
Feng, C.F.
Feng, Zhaoyang
Feng, Zhenyong
Gao, W.
Gou, Q.B.
Guo, Y.Q.
He, H.H.
Hu, Haibing
Hu, Hongbo
Iacovacci, M.
Iuppa, R.
Jia, H.Y.
Labaciren
Li, H.J.
Liu, C.
Liu, J.
Liu, M.Y.
Lu, H.
Ma, L.L.
Ma, X.H.
Mancarella, G.
Mari, S.M.
Marsella, G.
Mastroianni, S.
Montini, P.
Ning, C.C.
Perrone, L.
Pistilli, P.
Salvini, P.
Santonico, R.
Shen, P.R.
Sheng, X.D.
Shi, F.
Surdo, A.
Tan, Y.H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, H.
Wu, C.Y.
Wu, H.R.
Xue, L.
Yang, Q.Y.
Yang, X.C.
Yao, Z.G.
Yuan, A.F.
Zha, M.
Zhang, H.M.
Zhang, L.
Zhang, X.Y.
Zhang, Y.
Zhao, J.
Zhaxiciren
Zhaxisangzhu
Zhou, X.X.
Zhu, F.R.
Zhu, Q.Q.
author_sort Bartoli, B.
collection CERN
description The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a “full coverage” (central carpet with an active area of ∼93%) air shower array dedicated to gamma-ray astronomy and cosmic-ray studies. The wide field of view (∼2 sr) and high duty cycle (>86%), made ARGO-YBJ suitable to search for short and unexpected gamma-ray emissions like gamma-ray bursts (GRBs). Between 2007 November 6 and 2013 February 7, 156 satellite-triggered GRBs (24 of them with known redshift) occurred within the ARGO-YBJ field of view (zenith angle θ ≤ 45°). A search for possible emission associated with these GRBs has been made in the two energy ranges 10–100 GeV and 10–1000 GeV. No significant excess has been found in time coincidence with the satellite detections nor in a set of different time windows inside the interval of one hour after the bursts. Taking into account the EBL absorption, upper limits to the energy fluence at a 99% confidence level have been evaluated, with values ranging from ∼10(−)(5) erg cm(−)(2) to ∼10(−)(1) erg cm(−)(2). The Fermi-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by Fermi-LAT, is discussed in detail.
id cern-2260719
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
record_format invenio
spelling cern-22607192022-02-01T07:19:42Zdoi:10.3847/1538-4357/aa74bcdoi:10.3847/1538-4357/aa74bchttp://cds.cern.ch/record/2260719engBartoli, B.Bernardini, P.Bi, X.J.Cao, Z.Catalanotti, S.Chen, S.Z.Chen, T.L.Cui, S.W.Dai, B.Z.D'Amone, A.DanzengluobuDe Mitri, I.Ettorre Piazzoli, B.D.Girolamo, T.DiDi Sciascio, G.Feng, C.F.Feng, ZhaoyangFeng, ZhenyongGao, W.Gou, Q.B.Guo, Y.Q.He, H.H.Hu, HaibingHu, HongboIacovacci, M.Iuppa, R.Jia, H.Y.LabacirenLi, H.J.Liu, C.Liu, J.Liu, M.Y.Lu, H.Ma, L.L.Ma, X.H.Mancarella, G.Mari, S.M.Marsella, G.Mastroianni, S.Montini, P.Ning, C.C.Perrone, L.Pistilli, P.Salvini, P.Santonico, R.Shen, P.R.Sheng, X.D.Shi, F.Surdo, A.Tan, Y.H.Vallania, P.Vernetto, S.Vigorito, C.Wang, H.Wu, C.Y.Wu, H.R.Xue, L.Yang, Q.Y.Yang, X.C.Yao, Z.G.Yuan, A.F.Zha, M.Zhang, H.M.Zhang, L.Zhang, X.Y.Zhang, Y.Zhao, J.ZhaxicirenZhaxisangzhuZhou, X.X.Zhu, F.R.Zhu, Q.Q.Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Modehep-phParticle Physics - Phenomenologyastro-ph.HEAstrophysics and AstronomyThe ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a “full coverage” (central carpet with an active area of ∼93%) air shower array dedicated to gamma-ray astronomy and cosmic-ray studies. The wide field of view (∼2 sr) and high duty cycle (>86%), made ARGO-YBJ suitable to search for short and unexpected gamma-ray emissions like gamma-ray bursts (GRBs). Between 2007 November 6 and 2013 February 7, 156 satellite-triggered GRBs (24 of them with known redshift) occurred within the ARGO-YBJ field of view (zenith angle θ ≤ 45°). A search for possible emission associated with these GRBs has been made in the two energy ranges 10–100 GeV and 10–1000 GeV. No significant excess has been found in time coincidence with the satellite detections nor in a set of different time windows inside the interval of one hour after the bursts. Taking into account the EBL absorption, upper limits to the energy fluence at a 99% confidence level have been evaluated, with values ranging from ∼10(−)(5) erg cm(−)(2) to ∼10(−)(1) erg cm(−)(2). The Fermi-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by Fermi-LAT, is discussed in detail.The ARGO-YBJ detector, located at the Yangbajing Cosmic Ray Laboratory (4300 m a. s. l., Tibet, China), was a full coverage air shower array dedicated to gamma ray astronomy and cosmic ray studies. The wide field of view (~ 2 sr) and high duty cycle (> 86%), made ARGO-YBJ suitable to search for short and unexpected gamma ray emissions like gamma ray bursts (GRBs). Between 2007 November 6 and 2013 February 7, 156 satellite-triggered GRBs (24 of them with known redshift) occurred within the ARGO-YBJ field of view. A search for possible emission associated to these GRBs has been made in the two energy ranges 10-100 GeV and 10-1000 GeV. No significant excess has been found in time coincidence with the satellite detections nor in a time window of one hour after the bursts. Taking into account the EBL absorption, upper limits to the energy fluence at 99% of confidence level have been evaluated,with values ranging from ~ 10-5 erg cm-2 to ~10-1 erg cm-2.arXiv:1703.09284oai:cds.cern.ch:22607192017-03-23
spellingShingle hep-ph
Particle Physics - Phenomenology
astro-ph.HE
Astrophysics and Astronomy
Bartoli, B.
Bernardini, P.
Bi, X.J.
Cao, Z.
Catalanotti, S.
Chen, S.Z.
Chen, T.L.
Cui, S.W.
Dai, B.Z.
D'Amone, A.
Danzengluobu
De Mitri, I.
Ettorre Piazzoli, B.D.
Girolamo, T.Di
Di Sciascio, G.
Feng, C.F.
Feng, Zhaoyang
Feng, Zhenyong
Gao, W.
Gou, Q.B.
Guo, Y.Q.
He, H.H.
Hu, Haibing
Hu, Hongbo
Iacovacci, M.
Iuppa, R.
Jia, H.Y.
Labaciren
Li, H.J.
Liu, C.
Liu, J.
Liu, M.Y.
Lu, H.
Ma, L.L.
Ma, X.H.
Mancarella, G.
Mari, S.M.
Marsella, G.
Mastroianni, S.
Montini, P.
Ning, C.C.
Perrone, L.
Pistilli, P.
Salvini, P.
Santonico, R.
Shen, P.R.
Sheng, X.D.
Shi, F.
Surdo, A.
Tan, Y.H.
Vallania, P.
Vernetto, S.
Vigorito, C.
Wang, H.
Wu, C.Y.
Wu, H.R.
Xue, L.
Yang, Q.Y.
Yang, X.C.
Yao, Z.G.
Yuan, A.F.
Zha, M.
Zhang, H.M.
Zhang, L.
Zhang, X.Y.
Zhang, Y.
Zhao, J.
Zhaxiciren
Zhaxisangzhu
Zhou, X.X.
Zhu, F.R.
Zhu, Q.Q.
Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_full Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_fullStr Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_full_unstemmed Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_short Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_sort search for gamma ray bursts with the argo-ybj detector in shower mode
topic hep-ph
Particle Physics - Phenomenology
astro-ph.HE
Astrophysics and Astronomy
url https://dx.doi.org/10.3847/1538-4357/aa74bc
https://dx.doi.org/10.3847/1538-4357/aa74bc
http://cds.cern.ch/record/2260719
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