Search for rays from the supernova 1987A at energies greater than 100 TeV

I. A. Bond; E. Budding; M. J. Conway; K. B. Fenton; H. Fujii; Z. Fujii; H. Hasegawa; N. Hayashida; M. Honda; N. Hotta; J. E. Humble; S. Kabe; K. Kasahara; T. Kifune; A. Masaike; Y. Matsubara; K. Mitsui; Y. Miura; M. Mori; K. Murakami; Y. Muraki; M. Nagano; K. Nakamura; T. Nakamura; P. M. Norris; Y. Ohashi; A. Okada; To Saito; M. Sakata; H. Sato; S. Shibata; M. Shima; J. R. Storey; T. Tanimori; M. Teshima; Shoji Torii; K. Uchino; Y. Watase; M. D. Woodhams; Y. Yamamoto; P. C M Yock; T. Yuda

doi:10.1103/PhysRevLett.60.1110

Search for rays from the supernova 1987A at energies greater than 100 TeV

I. A. Bond^*, E. Budding, M. J. Conway, K. B. Fenton, H. Fujii, Z. Fujii, H. Hasegawa, N. Hayashida, M. Honda, N. Hotta, J. E. Humble, S. Kabe, K. Kasahara, T. Kifune, A. Masaike, Y. Matsubara, K. Mitsui, Y. Miura, M. Mori, K. MurakamiY. Muraki, M. Nagano, K. Nakamura, T. Nakamura, P. M. Norris, Y. Ohashi, A. Okada, To Saito, M. Sakata, H. Sato, S. Shibata, M. Shima, J. R. Storey, T. Tanimori, M. Teshima, Shoji Torii, K. Uchino, Y. Watase, M. D. Woodhams, Y. Yamamoto, P. C M Yock, T. Yuda

^*この研究の対応する著者

研究成果: Article › 査読

22 被引用数 (Scopus)

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We searched for ultrahigh-energy rays emitted by the supernova 1987A with a new cosmic-ray facility installed at the Black Birch Range in New Zealand. The observations from 13 October to 3 December 1987 suggest no clear clustering of events around the direction of the supernova. We conclude that an upper limit on the flux rays of energies greater than 100 TeV is 1.1×10-12 cm-2 s-1 (95% confidence limit) for a differential spectral index =2.0 and source distance d=50 kpc. This value gives an upper bound on the -ray luminosity of the supernova of 5.5×1038 erg s-1 for 1014, 1017 eV.

本文言語	English
ページ（範囲）	1110-1113
ページ数	4
ジャーナル	Physical Review Letters
巻	60
号	12
DOI	https://doi.org/10.1103/PhysRevLett.60.1110
出版ステータス	Published - 1988
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（全般）

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10.1103/PhysRevLett.60.1110

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Bond, I. A., Budding, E., Conway, M. J., Fenton, K. B., Fujii, H., Fujii, Z., Hasegawa, H., Hayashida, N., Honda, M., Hotta, N., Humble, J. E., Kabe, S., Kasahara, K., Kifune, T., Masaike, A., Matsubara, Y., Mitsui, K., Miura, Y., Mori, M., ... Yuda, T. (1988). Search for rays from the supernova 1987A at energies greater than 100 TeV. Physical Review Letters, 60(12), 1110-1113. https://doi.org/10.1103/PhysRevLett.60.1110

Bond, IA, Budding, E, Conway, MJ, Fenton, KB, Fujii, H, Fujii, Z, Hasegawa, H, Hayashida, N, Honda, M, Hotta, N, Humble, JE, Kabe, S, Kasahara, K, Kifune, T, Masaike, A, Matsubara, Y, Mitsui, K, Miura, Y, Mori, M, Murakami, K, Muraki, Y, Nagano, M, Nakamura, K, Nakamura, T, Norris, PM, Ohashi, Y, Okada, A, Saito, T, Sakata, M, Sato, H, Shibata, S, Shima, M, Storey, JR, Tanimori, T, Teshima, M, Torii, S, Uchino, K, Watase, Y, Woodhams, MD, Yamamoto, Y, Yock, PCM & Yuda, T 1988, 'Search for rays from the supernova 1987A at energies greater than 100 TeV', Physical Review Letters, vol. 60, no. 12, pp. 1110-1113. https://doi.org/10.1103/PhysRevLett.60.1110

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title = "Search for rays from the supernova 1987A at energies greater than 100 TeV",

abstract = "We searched for ultrahigh-energy rays emitted by the supernova 1987A with a new cosmic-ray facility installed at the Black Birch Range in New Zealand. The observations from 13 October to 3 December 1987 suggest no clear clustering of events around the direction of the supernova. We conclude that an upper limit on the flux rays of energies greater than 100 TeV is 1.1×10-12 cm-2 s-1 (95% confidence limit) for a differential spectral index =2.0 and source distance d=50 kpc. This value gives an upper bound on the -ray luminosity of the supernova of 5.5×1038 erg s-1 for 1014, 1017 eV.",

author = "Bond, {I. A.} and E. Budding and Conway, {M. J.} and Fenton, {K. B.} and H. Fujii and Z. Fujii and H. Hasegawa and N. Hayashida and M. Honda and N. Hotta and Humble, {J. E.} and S. Kabe and K. Kasahara and T. Kifune and A. Masaike and Y. Matsubara and K. Mitsui and Y. Miura and M. Mori and K. Murakami and Y. Muraki and M. Nagano and K. Nakamura and T. Nakamura and Norris, {P. M.} and Y. Ohashi and A. Okada and To Saito and M. Sakata and H. Sato and S. Shibata and M. Shima and Storey, {J. R.} and T. Tanimori and M. Teshima and Shoji Torii and K. Uchino and Y. Watase and Woodhams, {M. D.} and Y. Yamamoto and Yock, {P. C M} and T. Yuda",

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T1 - Search for rays from the supernova 1987A at energies greater than 100 TeV

AU - Bond, I. A.

AU - Budding, E.

AU - Conway, M. J.

AU - Fenton, K. B.

AU - Fujii, H.

AU - Fujii, Z.

AU - Hasegawa, H.

AU - Hayashida, N.

AU - Honda, M.

AU - Hotta, N.

AU - Humble, J. E.

AU - Kabe, S.

AU - Kasahara, K.

AU - Kifune, T.

AU - Masaike, A.

AU - Matsubara, Y.

AU - Mitsui, K.

AU - Miura, Y.

AU - Mori, M.

AU - Murakami, K.

AU - Muraki, Y.

AU - Nagano, M.

AU - Nakamura, K.

AU - Nakamura, T.

AU - Norris, P. M.

AU - Ohashi, Y.

AU - Okada, A.

AU - Saito, To

AU - Sakata, M.

AU - Sato, H.

AU - Shibata, S.

AU - Shima, M.

AU - Storey, J. R.

AU - Tanimori, T.

AU - Teshima, M.

AU - Torii, Shoji

AU - Uchino, K.

AU - Watase, Y.

AU - Woodhams, M. D.

AU - Yamamoto, Y.

AU - Yock, P. C M

AU - Yuda, T.

PY - 1988

Y1 - 1988

N2 - We searched for ultrahigh-energy rays emitted by the supernova 1987A with a new cosmic-ray facility installed at the Black Birch Range in New Zealand. The observations from 13 October to 3 December 1987 suggest no clear clustering of events around the direction of the supernova. We conclude that an upper limit on the flux rays of energies greater than 100 TeV is 1.1×10-12 cm-2 s-1 (95% confidence limit) for a differential spectral index =2.0 and source distance d=50 kpc. This value gives an upper bound on the -ray luminosity of the supernova of 5.5×1038 erg s-1 for 1014, 1017 eV.

AB - We searched for ultrahigh-energy rays emitted by the supernova 1987A with a new cosmic-ray facility installed at the Black Birch Range in New Zealand. The observations from 13 October to 3 December 1987 suggest no clear clustering of events around the direction of the supernova. We conclude that an upper limit on the flux rays of energies greater than 100 TeV is 1.1×10-12 cm-2 s-1 (95% confidence limit) for a differential spectral index =2.0 and source distance d=50 kpc. This value gives an upper bound on the -ray luminosity of the supernova of 5.5×1038 erg s-1 for 1014, 1017 eV.

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Search for rays from the supernova 1987A at energies greater than 100 TeV

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