Zobrazeno 1 - 10
of 13 860
pro vyhledávání: '"Delay R"'
Publikováno v:
Journal of Statistical Software, Vol 22, Iss 8 (2007)
Results of ecological models differ, to some extent, more from measured data than from empirical knowledge. Existing techniques for validation based on quantitative assessments sometimes cause an underestimation of the performance of models due to ti
Externí odkaz:
https://doaj.org/article/717891947c444d3497474168cc647c84
Akademický článek
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Publikováno v:
Journal of Statistical Software; Vol 22 (2007); 1-30
Journal of Statistical Software, Vol 22, Iss 8 (2007)
Journal of Statistical Software, Vol 22, Iss 8 (2007)
Results of ecological models differ, to some extent, more from measured data than from empirical knowledge. Existing techniques for validation based on quantitative assessments sometimes cause an underestimation of the performance of models due to ti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7eda4a1ac8e72ef2b2666841950d060
Publikováno v:
Insurance Insider. 9/19/2022, p1-1. 1p.
Autor:
Abdo, A. A., Abeysekara, A. U., Allen, B. T., Aune, T., Barber, A. S., Berley, D., Braun, J., Chen, C., Christopher, G. E., Delay, R. S., DeYoung, T., Dingus, B. L., Ellsworth, R. W., Fraija, N., González, M. M., Goodman, J. A., Hays, E., Hoffman, C. M., Hüntemeyer, P. H., Imran, A., Kolterman, B. E., Linnemann, J. T., Marinelli, A., McEnery, J. E., Morgan, T., Mincer, A. I., Nemethy, P., Patricelli, B., Pretz, J., Ryan, J. M., Parkinson, P. M. Saz, Schneider, M., Shoup, A., Sinnis, G., Smith, A. J., Vasileiou, V., Walker, G. P., Williams, D. A., Yodh, G. B.
TeV flaring activity with time scales as short as tens of minutes and an orphan TeV flare have been observed from the blazar Markarian 421 (Mrk 421). The TeV emission from Mrk 421 is believed to be produced by leptonic synchrotron self-Compton (SSC)
Externí odkaz:
http://arxiv.org/abs/1401.2161
Publikováno v:
International Journal of Social Psychiatry; Sep2023, Vol. 69 Issue 6, p1501-1509, 9p
Autor:
Abdo, A. A., Allen, B., Berley, D., Blaufuss, E., Casanova, S., Chen, C., Coyne, D. G., Delay, R. S., Dingus, B. L., Ellsworth, R. W., Fleysher, L., Fleysher, R., Gonzalez, M. M., Goodman, J. A., Hays, E., Hoffman, C. M., Kolterman, B. E., Kelley, L. A., Lansdell, C. P., Linnemann, J. T., McEnery, J. E., Mincer, A. I., Moskalenko, I. V., Nemethy, P., Noyes, D., Ryan, J. M., Samuelson, F. W., Parkinson, P. M. Saz, Schneider, M., Shoup, A., Sinnis, G., Smith, A. J., Strong, A. W., Sullivan, G. W., Vasileiou, V., Walker, G. P., Williams, D. A., Xu, X. W., Yodh, G. B.
Publikováno v:
Astrophys.J.658:L33-L36,2007
The diffuse gamma radiation arising from the interaction of cosmic ray particles with matter and radiation in the Galaxy is one of the few probes available to study the origin of the cosmic rays. Milagro is a water Cherenkov detector that continuousl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611691
Autor:
Atkins, R., Benbow, W., Berley, D., Chen, M. -L., Coyne, D. G., Delay, R. S., Dingus, B. L., Dorfan, D. E., Ellsworth, R. W., Evans, D., Falcone, A., Fleysher, L., Fleysher, R., Gisler, G., Goodman, J. A., Haines, T. J., Hoffman, C. M., Hugenberger, S., Kelley, L. A., Leonor, I., Macri, J., McConnell, M., McCullough, J. F., McEnery, J. E., Miller, R. S., Mincer, A. I., Morales, M. F., Nemethy, P., Ryan, J. M., Schneider, M., Shen, B., Shoup, A., Sinnis, G., Smith, A. J., Sullivan, G. W., Thompson, T. N., Tumer, O. T., Wang, K., Wascko, M. O., Westerhoff, S., Williams, D. A., Yang, T., Yodh, G. B.
Previous works have shown that water Cherenkov detectors have superior sensitivity to those of scintillation counters as applied to detecting extensive air showers (EAS). This is in large part due to their much higher sensitivity to EAS photons which
Externí odkaz:
http://arxiv.org/abs/astro-ph/9907214
Autor:
Atkins, R., Benbow, W., Berley, D., Chen, M. -L., Coyne, D. G., Delay, R. S., Dingus, B. L., Dorfan, D. E., Ellsworth, R. W., Evans, D., Falcone, A., Fleysher, L., Fleysher, R., Gisler, G., Goodman, J. A., Haines, T. J., Hoffman, C. M., Hugenberger, S., Kelley, L. A., Leonor, I., Macri, J., McConnell, M., McCullough, J. F., McEnery, J. E., Miller, R. S., Mincer, A. I., Morales, M. F., Nemethy, P., Ryan, J. M., Schneider, M., Shen, B., Shoup, A., Sinnis, G., Smith, A. J., Sullivan, G. W., Thompson, T. N., Tumer, O. T., Wang, K., Wascko, M. O., Westerhoff, S., Williams, D. A., Yang, T., Yodh, G. B.
The Milagro detector is an air shower array which uses the water Cherenkov technique and is capable of continuously monitoring the sky at energies near 1 TeV. The detector consists of 20000 metric tons of pure water instrumented with 723 photo-multip
Externí odkaz:
http://arxiv.org/abs/astro-ph/9906417
Autor:
Atkins, R., Benbow, W., Berley, D., Chen, M. -L., Coyne, D. G., Delay, R. S., Dingus, B. L., Dorfan, D. E., Ellsworth, R. W., Evans, D., Falcone, A., Fleysher, L., Fleysher, R., Gisler, G., Goodman, J. A., Haines, T. J., Hoffman, C. M., Hugenberger, S., Kelley, L. A., Leonor, I., Macri, J., McConnell, M., McCullough, J. F., McEnery, J. E., Miller, R. S., Mincer, A. I., Morales, M. F., Nemethy, P., Ryan, J. M., Schneider, M., Shen, B., Shoup, A., Sinnis, G., Smith, A. J., Sullivan, G. W., Thompson, T. N., Tumer, O. T., Wang, K., Wascko, M. O., Westerhoff, S., Williams, D. A., Yang, T., Yodh, G. B.
Milagrito, a prototype for the Milagro detector, operated for 15 months in 1997-8 and collected 8.9 billion events. It was the first extensive air shower (EAS) array sensitive to showers intiated by primaries with energy below 1 TeV. The shadows of t
Externí odkaz:
http://arxiv.org/abs/astro-ph/9906388