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pro vyhledávání: '"Foley, M. A."'
Autor:
Xie, J., Peng, C., Joosten, S., Meziani, Z. -E., Camsonne, A., Jones, M., Malace, S., Kaczanowicz, E., Rehfuss, M., Sparveris, N., Paolone, M., Foley, M., Minot, M., Popecki, M., Zhao, Z. W.
The SoLID spectrometer's gas Cherenkov counters require photosensors that operate in a high luminosity and high background environment. The reference design features arrays of 9 or 16 tiled multi-anode photomultipliers (MaPMTs), distributed across 32
Externí odkaz:
http://arxiv.org/abs/2402.00947
Autor:
Angelico, E., Elagin, A., Frisch, H. J., Spieglan, E., Adams, B. W., Foley, M. R., Minot, M. J.
We have designed and prototyped the process steps for the batch production of large-area micro-channel-plate photomultipliers (MCP-PMT) using the "air-transfer" assembly process developed with single $LAPPD^{\text{TM}}$ modules. Results are presented
Externí odkaz:
http://arxiv.org/abs/2003.06491
Autor:
Lyashenko, A. V., Adams, B. W., Aviles, M., Cremer, T., Ertley, C. D., Foley, M. R., Minot, M. J., Popecki, M. A., Stochaj, M. E., Worstell, W. A., Elam, J. W., Mane, A. U., Siegmund, O. H. W., Frisch, H. J., Elagin, A. L., Angelico, E., Spieglan, E.
We report on performance results achieved for recently produced LAPPDs - largest comercially available planar geometry photodetectors based on microchannel plates. These results include electron gains of up to $10^{7}$, low dark noise rates ($\sim$10
Externí odkaz:
http://arxiv.org/abs/1909.10399
Publikováno v:
Materials Science and Engineering: A, 2016, Volume 672, Pages 247-256
Composite materials comprising a porous Ti2AlC matrix and Al 6061 alloy were fabricated by a current-activated pressure assisted melt infiltration process. Coarse, medium and fine meso-structures were prepared with Al alloy filled pores of differing
Externí odkaz:
http://arxiv.org/abs/1908.08757
Publikováno v:
Open Access Emergency Medicine, Vol Volume 15, Pp 37-45 (2023)
Marie-Frédéric Tremblay,1 Frédéric Leblanc,1 Étienne Laroche,1 Virginie Blanchette,2,3 Magali Brousseau-Foley1,2 1Centre intégré universitaire de santé et de services sociaux de la Mauricie et du Centre-du-Québec affiliated to Université de
Externí odkaz:
https://doaj.org/article/03654f8f94e84c8894989d802e77da7f
Akademický článek
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Autor:
Jones, D. O., Scolnic, D. M., Foley, R. J., Rest, A., Kessler, R., Challis, P. M., Chambers, K. C., Coulter, D. A., Dettman, K. G., Foley, M. M., Huber, M. E., Jha, S. W., Johnson, E., Kilpatrick, C. D., Kirshner, R. P., Manuel, J., Narayan, G., Pan, Y. -C., Riess, A. G., Schultz, A. S. B., Siebert, M. R., Berger, E., Chornock, R., Flewelling, H., Magnier, E. A., Smartt, S. J., Smith, K. W., Wainscoat, R. J., Waters, C., Willman, M.
Measurements of the dark energy equation-of-state parameter, $w$, have been limited by uncertainty in the selection effects and photometric calibration of $z<0.1$ Type Ia supernovae (SNe Ia). The Foundation Supernova Survey is designed to lower these
Externí odkaz:
http://arxiv.org/abs/1811.09286
Autor:
Jones, D. O., Riess, A. G., Scolnic, D. M., Pan, Y. -C., Johnson, E., Coulter, D. A., Dettman, K. G., Foley, M. M., Foley, R. J., Huber, M. E., Jha, S. W., Kilpatrick, C. D., Kirshner, R. P., Rest, A., Schultz, A. S. B., Siebert, M. R.
Recent analyses suggest that distance residuals measured from Type Ia supernovae (SNe Ia) are correlated with local host galaxy properties within a few kpc of the SN explosion. However, the well-established correlation with global host galaxy propert
Externí odkaz:
http://arxiv.org/abs/1805.05911
Autor:
Foley, Ryan J., Scolnic, Daniel, Rest, Armin, Jha, S. W., Pan, Y. -C., Riess, A. G., Challis, P., Chambers, K. C., Coulter, D. A., Dettman, K. G., Foley, M. M., Fox, O. D., Huber, M. E., Jones, D. O., Kilpatrick, C. D., Kirshner, R. P., Schultz, A. S. B., Siebert, M. R., Flewelling, H. A., Gibson, B., Magnier, E. A., Miller, J. A., Primak, N., Smartt, S. J., Smith, K. W., Wainscoat, R. J., Waters, C., Willman, M.
The Foundation Supernova Survey aims to provide a large, high-fidelity, homogeneous, and precisely-calibrated low-redshift Type Ia supernova (SN Ia) sample for cosmology. The calibration of the current low-redshift SN sample is the largest component
Externí odkaz:
http://arxiv.org/abs/1711.02474
Autor:
Scolnic, D. M., Jones, D. O., Rest, A., Pan, Y. C., Chornock, R., Foley, R. J., Huber, M. E., Kessler, R., Narayan, G., Riess, A. G., Rodney, S., Berger, E., Brout, D. J., Challis, P. J., Drout, M., Finkbeiner, D., Lunnan, R., Kirshner, R. P., Sanders, N. E., Schlafly, E., Smartt, S., Stubbs, C. W., Tonry, J., Wood-Vasey, W. M., Foley, M., Hand, J., Johnson, E., Burgett, W. S., Chambers, K. C., Draper, P. W., Hodapp, K. W., Kaiser, N., Kudritzki, R. P., Magnier, E. A., Metcalfe, N., Bresolin, F., Gall, E., Kotak, R., McCrum, M., Smith, K. W.
We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry and ca
Externí odkaz:
http://arxiv.org/abs/1710.00845