Search Results - "Maestas, M.M."

A search for arrival direction clustering in the HiRes-I monocular data above 1019.5 eV by Abbasi, R.U., Abu-Zayyad, T., Amann, J.F., Archbold, G., Atkins, R., Bellido, J.A., Belov, K., Belz, J.W., BenZvi, S., Bergman, D.R., Burt, G.W., Cao, Z., Clay, R.W., Connolly, B., Dawson, B.R., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G.A., Hüntemeyer, P., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.C., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M., Sasaki, M., Schnetzer, S.R., Simpson, K.M., Sinnis, G., Smith, J.D., Snow, R., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A.

“…In the past few years, small scale anisotropy has become a primary focus in the search for source of ultra-high energy cosmic rays (UHECRs). The Akeno Giant…”
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Measurement of the flux of ultra high energy cosmic rays by the stereo technique by Abbasi, R.U., Abu-Zayyad, T., Al-Seady, M., Allen, M., Amann, J.F., Archbold, G., Belov, K., Belz, J.W., Bergman, D.R., Blake, S.A., Brusova, O.A., Burt, G.W., Cannon, C., Cao, Z., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G., Hüntemeyer, P., Ivanov, D., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.C., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M.D., Rodriguez, D., Sasaki, M., Schnetzer, S.R., Scott, L.M., Sinnis, G., Smith, J.D., Snow, R., Sokolsky, P., Springer, R.W., Stokes, B.T., Stratton, S.R., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Wiencke, L.R., Zech, A., Zhang, B.K., Zhang, X., Zhang, Y.

“…The High Resolution Fly’s Eye (HiRes) experiment has measured the flux of ultrahigh energy cosmic rays using the stereoscopic air fluorescence technique. The…”
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Search for correlations between HiRes stereo events and active galactic nuclei by Abbasi, R.U., Abu-Zayyad, T., Allen, M., Amman, J.F., Archbold, G., Belov, K., Belz, J.W., BenZvi, S.Y., Bergman, D.R., Blake, S.A., Boyer, J.H., Brusova, O.A., Burt, G.W., Cannon, C., Cao, Z., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G., Hüntemeyer, P., Ivanov, D., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Knapp, B.C., Loh, E.C., Maestas, M.M., Manago, N., Mannel, E.J., Marek, L.J., Martens, K., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M.D., Rodriguez, D., Sasaki, N., Schnetzer, S.R., Scott, L.M., Seman, M., Sinnis, G., Smith, J.D., Snow, R., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Stratton, S.R., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Wiencke, L.R., Zech, A., Zhang, X.

“…We have searched for correlations between the pointing directions of ultrahigh energy cosmic rays observed by the High Resolution Fly’s Eye experiment and…”
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Observation of the ankle and evidence for a high-energy break in the cosmic ray spectrum by Abbasi, R.U., Abu-Zayyad, T., Amman, J.F., Archbold, G., Atkins, R., Bellido, J.A., Belov, K., Belz, J.W., Ben Zvi, S.Y., Bergman, D.R., Burt, G.W., Cao, Z., Clay, R.W., Connolly, B.C., Deng, W., Dawson, B.R., Fedorova, Y., Findlay, J., Finley, C.B., Hanlon, W.F., Hoffman, C.M., Hughes, G.A., Holzscheiter, M.H., Hüntemeyer, P., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.G., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., O'Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M., Sasaki, M., Schnetzer, S.R., Simpson, K.M., Sinnis, G., Smith, J.D., Snow, R., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A.

“…We have measured the cosmic ray spectrum at energies above 1017eV using the two air fluorescence detectors of the High Resolution Fly's Eye experiment…”
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Measurement of pressure dependent fluorescence yield of air: Calibration factor for UHECR detectors by Belz, J.W., Burt, G.W., Cao, Z., Chang, F.Y., Chen, C.C., Chen, C.W., Chen, P., Field, C., Findlay, J., Hüntemeyer, P., Huang, M.A., Hwang, W.-Y.P., Iverson, R., Jones, B.F., Jui, C.C.H., Kirn, M., Lin, G.-L., Loh, E.C., Maestas, M.M., Manago, N., Martens, K., Matthews, J.N., Ng, J.S.T., Odian, A., Reil, K., Smith, J.D., Snow, R., Sokolsky, P., Springer, R.W., Thomas, J.R., Thomas, S.B., Thomson, G.B., Walz, D., Zech, A.

“…In a test experiment at the Final Focus Test Beam of the Stanford Linear Accelerator Center, the fluorescence yield of 28.5 GeV electrons in air and nitrogen…”
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Studies of systematic uncertainties in the estimation of the monocular aperture of the HiRes experiment by Abbasi, R.U., Abu-Zayyad, T., Amman, J.F., Archbold, G., Belov, K., Belz, J.W., Ben Zvi, S.Y., Bergman, D.R., Blake, S.A., Brusova, O., Burt, G.W., Cao, Z., Connolly, B.C., Deng, W., Fedorova, Y., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Hughes, G.A., Holzscheiter, M.H., Hüntemeyer, P., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.C., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M., Rodriguez, D., Sasaki, M., Schnetzer, S.R., Scott, L.M., Sinnis, G., Smith, J.D., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A., Zhang, X.

“…We have studied several sources of systematic uncertainty in calculating the aperture of the High Resolution Fly’s Eye experiment (HiRes) in monocular mode,…”
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Search for point-like sources of cosmic rays with energies above 1018.5eV in the HiRes-I monocular data set by Abbasi, R.U., Abu-Zayyad, T., Amann, J.F., Archbold, G., Belov, K., Belz, J.W., BenZvi, S., Bergman, D.R., Blake, S.A., Cao, Z., Connolly, B.M., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G.A., Hüntemeyer, P., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.C., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Rodriguez, D., Roberts, M.D., Sasaki, M., Schnetzer, S.R., Scott, L.M., Sinnis, G., Smith, J.D., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A., Zhang, X.

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An alternative method to finding patterns in HiRes stereo data by Abbasi, R.U., Abu-Zayyad, T., Amman, J.F., Archbold, G.C., Belov, K., Blake, S.A., Belz, J.W., BenZvi, S., Bergman, D.R., Boyer, J.H., Burt, G.W., Cao, Z., Connolly, B.M., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G.A., Hüntemeyer, P., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Knapp, B.C., Loh, E.C., Maestas, M.M., Manago, N., Mannel, E.J., Marek, L.J., Martins, K., Matthews, J.A.J., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M., Rodriguez, D., Sasaki, M., Schnetzer, S., Scott, L.M., Seman, M., Sinnis, G., Smith, J.D., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Weincke, L.R., Zech, A., Zhang, X.

“…In this paper ultra-high energy cosmic rays UHECRs data observed by the HiRes fluorescence detector in stereo mode is analyzed to search for events in the sky…”
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Search for point-like sources of cosmic rays with energies above 10 18.5 eV in the HiRes-I monocular data set by Abbasi, R.U., Abu-Zayyad, T., Amann, J.F., Archbold, G., Belov, K., Belz, J.W., BenZvi, S., Bergman, D.R., Blake, S.A., Cao, Z., Connolly, B.M., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Gray, R.C., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G.A., Hüntemeyer, P., Jones, B.F., Jui, C.C.H., Kim, K., Kirn, M.A., Loh, E.C., Maestas, M.M., Manago, N., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., Moore, S.A., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Rodriguez, D., Roberts, M.D., Sasaki, M., Schnetzer, S.R., Scott, L.M., Sinnis, G., Smith, J.D., Sokolsky, P., Song, C., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A., Zhang, X.

“…We report the results of a search for point-like deviations from isotropy in the arrival directions of ultra-high energy cosmic rays in the northern…”
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A likelihood method for measuring the ultrahigh energy cosmic ray composition by Abbasi, R.U., Abu-Zayyad, T., Amman, J.F., Archbold, G.C., Belov, K., Blake, S.A., Belz, J.W., BenZvi, S., Bergman, D.R., Boyer, J.H., Burt, G.W., Cao, Z., Connolly, B.M., Deng, W., Fedorova, Y., Findlay, J., Finley, C.B., Hanlon, W.F., Hoffman, C.M., Holzscheiter, M.H., Hughes, G.A., Hüntemeyer, P., Jui, C.C.H., Kim, K., Kirn, M.A., Knapp, B.C., Loh, E.C., Maestas, M.M., Manago, N., Mannel, E.J., Marek, L.J., Martens, K., Matthews, J.A.J., Matthews, J.N., O’Neill, A., Painter, C.A., Perera, L., Reil, K., Riehle, R., Roberts, M., Rodriguez, D., Sasaki, M., Schnetzer, S., Seman, M., Sinnis, G., Smith, J.D., Snow, R., Sokolsky, P., Springer, R.W., Stokes, B.T., Thomas, J.R., Thomas, S.B., Thomson, G.B., Tupa, D., Westerhoff, S., Wiencke, L.R., Zech, A.

“…Air fluorescence detectors traditionally determine the dominant chemical composition of the ultrahigh energy cosmic ray flux by comparing the averaged slant…”
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