Eintrag weiter verarbeiten
Verfügbar über Online-Ressource

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

Gespeichert in:

Bibliographische Detailangaben
Zeitschriftentitel: The Astrophysical Journal
Personen und Körperschaften: 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, Mitri, I. De, Piazzoli, B. D’Ettorre, Girolamo, T. Di, Sciascio, G. Di, 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.
In: The Astrophysical Journal, 842, 2017, 1, S. 31
Format: E-Article
Sprache: Unbestimmt
veröffentlicht:
American Astronomical Society
Schlagwörter:
Space and Planetary Science
Astronomy and Astrophysics
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
Mitri, I. De
Piazzoli, B. D’Ettorre
Girolamo, T. Di
Sciascio, G. Di
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.
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
Mitri, I. De
Piazzoli, B. D’Ettorre
Girolamo, T. Di
Sciascio, G. Di
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 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
Mitri, I. De
Piazzoli, B. D’Ettorre
Girolamo, T. Di
Sciascio, G. Di
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.
spellingShingle 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
Mitri, I. De
Piazzoli, B. D’Ettorre
Girolamo, T. Di
Sciascio, G. Di
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.
The Astrophysical Journal
Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode
Space and Planetary Science
Astronomy and Astrophysics
author_sort bartoli, b.
spelling 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 Mitri, I. De Piazzoli, B. D’Ettorre Girolamo, T. Di Sciascio, G. Di 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. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aa74bc <jats:title>Abstract</jats:title> <jats:p>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 (&gt;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 <jats:italic>θ</jats:italic> ≤ 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<jats:sup>−5</jats:sup> erg cm<jats:sup>−2</jats:sup> to ∼10<jats:sup>−1</jats:sup> erg cm<jats:sup>−2</jats:sup>. The <jats:italic>Fermi</jats:italic>-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by <jats:italic>Fermi</jats:italic>-LAT, is discussed in detail.</jats:p> Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode The Astrophysical Journal
doi_str_mv 10.3847/1538-4357/aa74bc
facet_avail Online
Free
finc_class_facet Physik
Technik
format ElectronicArticle
fullrecord blob:ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMzg0Ny8xNTM4LTQzNTcvYWE3NGJj
id ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMzg0Ny8xNTM4LTQzNTcvYWE3NGJj
institution DE-Gla1
DE-Zi4
DE-15
DE-Rs1
DE-Pl11
DE-105
DE-14
DE-Ch1
DE-L229
DE-D275
DE-Bn3
DE-Brt1
DE-Zwi2
DE-D161
imprint American Astronomical Society, 2017
imprint_str_mv American Astronomical Society, 2017
issn 0004-637X
1538-4357
issn_str_mv 0004-637X
1538-4357
language Undetermined
mega_collection American Astronomical Society (CrossRef)
match_str bartoli2017searchforgammarayburstswiththeargoybjdetectorinshowermode
publishDateSort 2017
publisher American Astronomical Society
recordtype ai
record_format ai
series The Astrophysical Journal
source_id 49
title Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode
title_unstemmed 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 Space and Planetary Science
Astronomy and Astrophysics
url http://dx.doi.org/10.3847/1538-4357/aa74bc
publishDate 2017
physical 31
description <jats:title>Abstract</jats:title> <jats:p>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 (&gt;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 <jats:italic>θ</jats:italic> ≤ 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<jats:sup>−5</jats:sup> erg cm<jats:sup>−2</jats:sup> to ∼10<jats:sup>−1</jats:sup> erg cm<jats:sup>−2</jats:sup>. The <jats:italic>Fermi</jats:italic>-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by <jats:italic>Fermi</jats:italic>-LAT, is discussed in detail.</jats:p>
container_issue 1
container_start_page 0
container_title The Astrophysical Journal
container_volume 842
format_de105 Article, E-Article
format_de14 Article, E-Article
format_de15 Article, E-Article
format_de520 Article, E-Article
format_de540 Article, E-Article
format_dech1 Article, E-Article
format_ded117 Article, E-Article
format_degla1 E-Article
format_del152 Buch
format_del189 Article, E-Article
format_dezi4 Article
format_dezwi2 Article, E-Article
format_finc Article, E-Article
format_nrw Article, E-Article
_version_ 1792342938191134721
geogr_code not assigned
last_indexed 2024-03-01T16:43:46.298Z
geogr_code_person not assigned
openURL url_ver=Z39.88-2004&ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fvufind.svn.sourceforge.net%3Agenerator&rft.title=Search+for+Gamma-Ray+Bursts+with+the+ARGO-YBJ+Detector+in+Shower+Mode&rft.date=2017-06-10&genre=article&issn=1538-4357&volume=842&issue=1&pages=31&jtitle=The+Astrophysical+Journal&atitle=Search+for+Gamma-Ray+Bursts+with+the+ARGO-YBJ+Detector+in+Shower+Mode&aulast=Zhu&aufirst=Q.+Q.&rft_id=info%3Adoi%2F10.3847%2F1538-4357%2Faa74bc&rft.language%5B0%5D=und
SOLR
_version_ 1792342938191134721
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, Mitri, I. De, Piazzoli, B. D’Ettorre, Girolamo, T. Di, Sciascio, G. Di, 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, Mitri, I. De, Piazzoli, B. D’Ettorre, Girolamo, T. Di, Sciascio, G. Di, 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., 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, Mitri, I. De, Piazzoli, B. D’Ettorre, Girolamo, T. Di, Sciascio, G. Di, 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.
container_issue 1
container_start_page 0
container_title The Astrophysical Journal
container_volume 842
description <jats:title>Abstract</jats:title> <jats:p>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 (&gt;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 <jats:italic>θ</jats:italic> ≤ 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<jats:sup>−5</jats:sup> erg cm<jats:sup>−2</jats:sup> to ∼10<jats:sup>−1</jats:sup> erg cm<jats:sup>−2</jats:sup>. The <jats:italic>Fermi</jats:italic>-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by <jats:italic>Fermi</jats:italic>-LAT, is discussed in detail.</jats:p>
doi_str_mv 10.3847/1538-4357/aa74bc
facet_avail Online, Free
finc_class_facet Physik, Technik
format ElectronicArticle
format_de105 Article, E-Article
format_de14 Article, E-Article
format_de15 Article, E-Article
format_de520 Article, E-Article
format_de540 Article, E-Article
format_dech1 Article, E-Article
format_ded117 Article, E-Article
format_degla1 E-Article
format_del152 Buch
format_del189 Article, E-Article
format_dezi4 Article
format_dezwi2 Article, E-Article
format_finc Article, E-Article
format_nrw Article, E-Article
geogr_code not assigned
geogr_code_person not assigned
id ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMzg0Ny8xNTM4LTQzNTcvYWE3NGJj
imprint American Astronomical Society, 2017
imprint_str_mv American Astronomical Society, 2017
institution DE-Gla1, DE-Zi4, DE-15, DE-Rs1, DE-Pl11, DE-105, DE-14, DE-Ch1, DE-L229, DE-D275, DE-Bn3, DE-Brt1, DE-Zwi2, DE-D161
issn 0004-637X, 1538-4357
issn_str_mv 0004-637X, 1538-4357
language Undetermined
last_indexed 2024-03-01T16:43:46.298Z
match_str bartoli2017searchforgammarayburstswiththeargoybjdetectorinshowermode
mega_collection American Astronomical Society (CrossRef)
physical 31
publishDate 2017
publishDateSort 2017
publisher American Astronomical Society
record_format ai
recordtype ai
series The Astrophysical Journal
source_id 49
spelling 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 Mitri, I. De Piazzoli, B. D’Ettorre Girolamo, T. Di Sciascio, G. Di 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. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aa74bc <jats:title>Abstract</jats:title> <jats:p>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 (&gt;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 <jats:italic>θ</jats:italic> ≤ 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<jats:sup>−5</jats:sup> erg cm<jats:sup>−2</jats:sup> to ∼10<jats:sup>−1</jats:sup> erg cm<jats:sup>−2</jats:sup>. The <jats:italic>Fermi</jats:italic>-GBM burst GRB 090902B, with a high-energy photon of 33.4 GeV detected by <jats:italic>Fermi</jats:italic>-LAT, is discussed in detail.</jats:p> Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode The Astrophysical Journal
spellingShingle 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, Mitri, I. De, Piazzoli, B. D’Ettorre, Girolamo, T. Di, Sciascio, G. Di, 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., The Astrophysical Journal, Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode, Space and Planetary Science, Astronomy and Astrophysics
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
title_unstemmed Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode
topic Space and Planetary Science, Astronomy and Astrophysics
url http://dx.doi.org/10.3847/1538-4357/aa74bc