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1by Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Bouma, S., Buitink, S., Carter, K., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Latif, U., Magnuson, M., Meures, T., Meyers, Z. S., Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.“... can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm...”
Published in The European Physical Journal C (2021)
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2by Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Bouma, S., Buitink, S., Carter, K., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Latif, U., Meures, T., Meyers, Z. S., Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Oeyen, Bob, Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, Dirk, Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Van Den Broeck, D. J., van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.“... can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm...”
Published in The European Physical Journal C (2022)
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3by Aguilar, J. A., Allison, P., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Beatty, J. J., Hallgren, A., Hallmann, Steffen, Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Bernhoff, H., Krebs, R., Lahmann, R., Latif, U., Magnuson, M., Meures, T., Meyers, Zachary Samuel, Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Besson, D., Oeyen, B., Pandya, H., Plaisier, Ilse, Pyras, Lilly, Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Bingefors, N., Toscano, S., Tosi, D., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, Christoph, Wissel, S., Young, R., Zink, A., Botner, O., Bouma, S., Buitink, S., Carter, K.“... can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm...”
Published in The European Physical Journal C (2022)
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4by Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Bouma, S., Buitink, S., Carter, K., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Latif, U., Meures, T., Meyers, Z. S., Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Van Den Broeck, D. J., van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.“... can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm...”
Published in The European Physical Journal C (2022)
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5by Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, Hans, Besson, D., Bingefors, Nils, Botner, Olga, Bouma, S., Buitink, S., Carter, K., Cataldo, M., Clark, B. A., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Glaser, Christian, Hallgren, Allan, Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Latif, U., Meures, T., Meyers, Z. S., Mulrey, K., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I, Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Tosi, D., Van den Broeck, D. J., van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.“... can be estimated. We show that this method can achieve an uncertainty of 13% on the logarithm...”
Published in The European Physical Journal C (2022)
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6by Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S. -H., Welling, C.“... cm -2 s -1 sr -1 for a decade wide logarithmic bin centered at a neutrino energy of 1018,eV, which...”
Published in Journal of Cosmology and Astroparticle Physics (2023)
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7by Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S. -H., Welling, C.“...^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered at a neutrino energy...”
Published 2019
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8by Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S.-H., Welling, C.“...^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered at a neutrino energy...”
Published 2019
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9by Anker, A., Barwick, S. W., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Bernhoff, H., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S.-H., Welling, C., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C.“...^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered at a neutrino energy...”
Published 2019
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10by Anker, A., Barwick, S. W., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Bernhoff, H., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S.-H., Welling, C., ARIANNA Collaboration, Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C.“...^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered at a neutrino energy...”
Published in Journal of Cosmology and Astroparticle Physics (2020)
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11by Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S. -H., Welling, C.“...^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered at a neutrino energy...”
Published in Journal of Cosmology and Astroparticle Physics (2019)
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12by Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S.-H., Welling, C.“...^2\Phi=1.7\times 10^{-6}\mathrm{GeV cm^{-2}s^{-1}sr^{-1}}$ for a decade wide logarithmic bin centered...”
Published 2020
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