Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1

W. H. Allen; I. A. Bond; E. Budding; M. J. Conway; A. Daniel; K. B. Fenton; H. Fujii; Z. Fujii; N. Hayashida; K. Hibino; M. Honda; J. E. Humble; S. Kabe; K. Kasahara; T. Kifune; G. D. Lythe; A. Masaike; Y. Matsubara; K. Mitsui; Y. Miura; M. Mori; Y. Muraki; M. Nagano; T. Nakamura; M. Nishizawa; P. M. Norris; S. Ogio; T. O. Saito; M. Sakata; H. Sato; H. M. Shimizu; M. Spencer; J. R. Storey; T. Tanimori; M. Teshima; Shoji Torii; A. Wadsworth; Y. Watase; M. D. Woodhams; Y. Yamamoto; P. C M Yock; T. Yuda

Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1

W. H. Allen^*, I. A. Bond, E. Budding, M. J. Conway, A. Daniel, K. B. Fenton, H. Fujii, Z. Fujii, N. Hayashida, K. Hibino, M. Honda, J. E. Humble, S. Kabe, K. Kasahara, T. Kifune, G. D. Lythe, A. Masaike, Y. Matsubara, K. Mitsui, Y. MiuraM. Mori, Y. Muraki, M. Nagano, T. Nakamura, M. Nishizawa, P. M. Norris, S. Ogio, T. O. Saito, M. Sakata, H. Sato, H. M. Shimizu, M. Spencer, J. R. Storey, T. Tanimori, M. Teshima, Shoji Torii, A. Wadsworth, Y. Watase, M. D. Woodhams, Y. Yamamoto, P. C M Yock, T. Yuda

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研究成果: Article › 査読

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The active galaxy Centaurus A and the X-ray binary systems Vela X-1, Centaurus X-3, and Circinus X-1 were monitored for VHE gamma-ray emission above 1 TeV with the JANZOS Cerenkov facility during 1988 and 1989. No evidence was found for persistent or episodic emission from any of these objects. Subseqeunt upper limits on the integral fluxes of 2.2 × 10^-11, 2.8 × 10^-11, 4.0 × 10^-11, and 4.2 × 10^-11 cm^-2 s^-1, respectively, were obtained for these objects. These limits are consistent with results of observations made by other groups.

本文言語	English
ページ（範囲）	554-558
ページ数	5
ジャーナル	Astrophysical Journal
巻	405
号	2
出版ステータス	Published - 1993 3月 10
外部発表	はい

ASJC Scopus subject areas

宇宙惑星科学

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引用スタイル

Allen, W. H., Bond, I. A., Budding, E., Conway, M. J., Daniel, A., Fenton, K. B., Fujii, H., Fujii, Z., Hayashida, N., Hibino, K., Honda, M., Humble, J. E., Kabe, S., Kasahara, K., Kifune, T., Lythe, G. D., Masaike, A., Matsubara, Y., Mitsui, K., ... Yuda, T. (1993). Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1. Astrophysical Journal, 405(2), 554-558.

Allen, WH, Bond, IA, Budding, E, Conway, MJ, Daniel, A, Fenton, KB, Fujii, H, Fujii, Z, Hayashida, N, Hibino, K, Honda, M, Humble, JE, Kabe, S, Kasahara, K, Kifune, T, Lythe, GD, Masaike, A, Matsubara, Y, Mitsui, K, Miura, Y, Mori, M, Muraki, Y, Nagano, M, Nakamura, T, Nishizawa, M, Norris, PM, Ogio, S, Saito, TO, Sakata, M, Sato, H, Shimizu, HM, Spencer, M, Storey, JR, Tanimori, T, Teshima, M, Torii, S, Wadsworth, A, Watase, Y, Woodhams, MD, Yamamoto, Y, Yock, PCM & Yuda, T 1993, 'Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1', Astrophysical Journal, vol. 405, no. 2, pp. 554-558.

@article{cf7a8210e0554364997637a0aeca0ed3,

title = "Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1",

abstract = "The active galaxy Centaurus A and the X-ray binary systems Vela X-1, Centaurus X-3, and Circinus X-1 were monitored for VHE gamma-ray emission above 1 TeV with the JANZOS Cerenkov facility during 1988 and 1989. No evidence was found for persistent or episodic emission from any of these objects. Subseqeunt upper limits on the integral fluxes of 2.2 × 10-11, 2.8 × 10-11, 4.0 × 10-11, and 4.2 × 10-11 cm-2 s-1, respectively, were obtained for these objects. These limits are consistent with results of observations made by other groups.",

keywords = "Galaxies: individual (Centaurus A), Gamma rays: observations, Stars: individual (Vela X-1, Centaurus X-3, Circinus X-1), X-rays: galaxies, X-rays: stars",

author = "Allen, {W. H.} and Bond, {I. A.} and E. Budding and Conway, {M. J.} and A. Daniel and Fenton, {K. B.} and H. Fujii and Z. Fujii and N. Hayashida and K. Hibino and M. Honda and Humble, {J. E.} and S. Kabe and K. Kasahara and T. Kifune and Lythe, {G. D.} and A. Masaike and Y. Matsubara and K. Mitsui and Y. Miura and M. Mori and Y. Muraki and M. Nagano and T. Nakamura and M. Nishizawa and Norris, {P. M.} and S. Ogio and Saito, {T. O.} and M. Sakata and H. Sato and Shimizu, {H. M.} and M. Spencer and Storey, {J. R.} and T. Tanimori and M. Teshima and Shoji Torii and A. Wadsworth and Y. Watase and Woodhams, {M. D.} and Y. Yamamoto and Yock, {P. C M} and T. Yuda",

year = "1993",

month = mar,

day = "10",

language = "English",

volume = "405",

pages = "554--558",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "2",

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TY - JOUR

T1 - Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1

AU - Allen, W. H.

AU - Bond, I. A.

AU - Budding, E.

AU - Conway, M. J.

AU - Daniel, A.

AU - Fenton, K. B.

AU - Fujii, H.

AU - Fujii, Z.

AU - Hayashida, N.

AU - Hibino, K.

AU - Honda, M.

AU - Humble, J. E.

AU - Kabe, S.

AU - Kasahara, K.

AU - Kifune, T.

AU - Lythe, G. D.

AU - Masaike, A.

AU - Matsubara, Y.

AU - Mitsui, K.

AU - Miura, Y.

AU - Mori, M.

AU - Muraki, Y.

AU - Nagano, M.

AU - Nakamura, T.

AU - Nishizawa, M.

AU - Norris, P. M.

AU - Ogio, S.

AU - Saito, T. O.

AU - Sakata, M.

AU - Sato, H.

AU - Shimizu, H. M.

AU - Spencer, M.

AU - Storey, J. R.

AU - Tanimori, T.

AU - Teshima, M.

AU - Torii, Shoji

AU - Wadsworth, A.

AU - Watase, Y.

AU - Woodhams, M. D.

AU - Yamamoto, Y.

AU - Yock, P. C M

AU - Yuda, T.

PY - 1993/3/10

Y1 - 1993/3/10

N2 - The active galaxy Centaurus A and the X-ray binary systems Vela X-1, Centaurus X-3, and Circinus X-1 were monitored for VHE gamma-ray emission above 1 TeV with the JANZOS Cerenkov facility during 1988 and 1989. No evidence was found for persistent or episodic emission from any of these objects. Subseqeunt upper limits on the integral fluxes of 2.2 × 10-11, 2.8 × 10-11, 4.0 × 10-11, and 4.2 × 10-11 cm-2 s-1, respectively, were obtained for these objects. These limits are consistent with results of observations made by other groups.

AB - The active galaxy Centaurus A and the X-ray binary systems Vela X-1, Centaurus X-3, and Circinus X-1 were monitored for VHE gamma-ray emission above 1 TeV with the JANZOS Cerenkov facility during 1988 and 1989. No evidence was found for persistent or episodic emission from any of these objects. Subseqeunt upper limits on the integral fluxes of 2.2 × 10-11, 2.8 × 10-11, 4.0 × 10-11, and 4.2 × 10-11 cm-2 s-1, respectively, were obtained for these objects. These limits are consistent with results of observations made by other groups.

KW - Galaxies: individual (Centaurus A)

KW - Gamma rays: observations

KW - Stars: individual (Vela X-1, Centaurus X-3, Circinus X-1)

KW - X-rays: galaxies

KW - X-rays: stars

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M3 - Article

AN - SCOPUS:12044250184

VL - 405

SP - 554

EP - 558

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

Upper limits on TeV gamma-ray emission from centaurus A, vela X-1, centaurus X-3, and circinus X-1

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