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

研究成果: Article

22 引用 (Scopus)

抄録

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.

元の言語English
ページ(範囲)1110-1113
ページ数4
ジャーナルPhysical Review Letters
60
発行部数12
DOI
出版物ステータスPublished - 1988
外部発表Yes

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supernova 1987A
rays
supernovae
confidence limits
New Zealand
energy
cosmic rays
luminosity

ASJC Scopus subject areas

  • Physics and Astronomy(all)

これを引用

Bond, I. A., Budding, E., Conway, M. J., Fenton, K. B., Fujii, H., Fujii, Z., ... 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

Search for rays from the supernova 1987A at energies greater than 100 TeV. / 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.; Murakami, K.; Muraki, Y.; Nagano, M.; Nakamura, K.; Nakamura, T.; Norris, P. M.; Ohashi, Y.; Okada, A.; Saito, To; Sakata, M.; Sato, H.; Shibata, S.; Shima, M.; Storey, J. R.; Tanimori, T.; Teshima, M.; Torii, Shoji; Uchino, K.; Watase, Y.; Woodhams, M. D.; Yamamoto, Y.; Yock, P. C M; Yuda, T.

:: Physical Review Letters, 巻 60, 番号 12, 1988, p. 1110-1113.

研究成果: Article

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, 巻. 60, 番号 12, pp. 1110-1113. https://doi.org/10.1103/PhysRevLett.60.1110
Bond IA, Budding E, Conway MJ, Fenton KB, Fujii H, Fujii Z その他. Search for rays from the supernova 1987A at energies greater than 100 TeV. Physical Review Letters. 1988;60(12):1110-1113. https://doi.org/10.1103/PhysRevLett.60.1110
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. ; Murakami, K. ; Muraki, Y. ; Nagano, M. ; Nakamura, K. ; Nakamura, T. ; Norris, P. M. ; Ohashi, Y. ; Okada, A. ; Saito, To ; Sakata, M. ; Sato, H. ; Shibata, S. ; Shima, M. ; Storey, J. R. ; Tanimori, T. ; Teshima, M. ; Torii, Shoji ; Uchino, K. ; Watase, Y. ; Woodhams, M. D. ; Yamamoto, Y. ; Yock, P. C M ; Yuda, T. / Search for rays from the supernova 1987A at energies greater than 100 TeV. :: Physical Review Letters. 1988 ; 巻 60, 番号 12. pp. 1110-1113.
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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.",
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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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