Zobrazeno 1 - 10
of 6 130
pro vyhledávání: '"Williams, S P"'
Autor:
Bowry, M., Tarasov, O. B., Berryman, J. S., Bader, V., Bazin, D., Chupp, T., Crawford, H. L., Gade, A., Lunderberg, E., Ratkiewicz, A., Recchia, F., Sherrill, B. M., Smalley, D., Stolz, A., Stroberg, S. R., Weisshaar, D., Williams, S., Wimmer, K., Yurkon, J.
Publikováno v:
Phys. Rev. C 108, 034604 (2023)
The availability of high-intensity, heavy-ion beams coupled to sensitive, large solid-angleacceptance spectrometers has enabled a detailed examination of the fission fragments produced in induced-fission reactions. The abrasion-fission process involv
Externí odkaz:
http://arxiv.org/abs/2401.18016
Autor:
Leardini, S., Sáa-Hernández, A., Kuźniak, M., González-Díaz, D., Azevedo, C. D. R., Lucas, F., Amedo, P., Cortez, A. F. V., Fernández-Posada, D., Mehl, B., Nieradka, G., de Oliveira, R., Peskov, V., Sworobowicz, T., Williams, S.
Publikováno v:
Front. Detect. Sci. Technol 2, 1373235 (2024)
The idea of implementing electroluminescence-based amplification through transparent multi-hole structures (FAT-GEMs) has been entertained for some time. Arguably, for such a technology to be attractive it should perform at least at a level comparabl
Externí odkaz:
http://arxiv.org/abs/2401.09905
Observations of type Ia supernova SN 2020nlb up to 600 days after explosion, and the distance to M85
Autor:
Williams, S. C., Kotak, R., Lundqvist, P., Mattila, S., Mazzali, P. A., Pastorello, A., Reguitti, A., Stritzinger, M. D., Fiore, A., Hook, I. M., Moran, S., Salmaso, I.
The type Ia supernova (SN Ia) SN 2020nlb was discovered in the Virgo Cluster galaxy M85 shortly after explosion. Here we present observations that include one of the earliest high-quality spectra and some of the earliest multi-colour photometry of a
Externí odkaz:
http://arxiv.org/abs/2401.08759
Autor:
Dumayne, J., Hook, I. M., Williams, S. C., Lowes, G. A., Head, D., Fritz, A., Graur, O., Holwerda, B., Humphrey, A., Milligan, A., Nicholl, M., Roukema, B. F., Wiseman, P.
The Rubin Observatory's 10-year Legacy Survey of Space and Time will observe near to 20 billion galaxies. For each galaxy the properties can be inferred. Approximately $10^5$ galaxies observed per year will contain Type Ia supernovae (SNe), allowing
Externí odkaz:
http://arxiv.org/abs/2308.04863
Autor:
Gracen L, Aikebuse M, Sarraf B, McPhail SM, Russell AW, O’Beirne J, Irvine KM, Williams S, Valery PC, Powell EE
Publikováno v:
Patient Preference and Adherence, Vol Volume 18, Pp 1845-1855 (2024)
Lucy Gracen,1 Melanie Aikebuse,2,3 Babak Sarraf,2– 4 Steven M McPhail,5 Anthony W Russell,6 James O’Beirne,7 Katharine M Irvine,8 Suzanne Williams,9 Patricia C Valery,4,* Elizabeth E Powell2– 4,* 1Department of Gastroenterology and Hepa
Externí odkaz:
https://doaj.org/article/10832f40cbf4427eb527e6f4fc09d346
Autor:
Williams S. Ebhota, Pavel Y. Tabakov
Publikováno v:
International Journal of Renewable Energy Development, Vol 13, Iss 3, Pp 508-520 (2024)
This study systematically evaluates Phototovoltaic (PV) system energy losses and performance quality across selected locations in sub-Saharan African (SSA). Utilising a computational model for a hypothetical 10 kWp crystalline silicon (c-Si) PV syste
Externí odkaz:
https://doaj.org/article/37911d7b3dc441179b62103d129db1d1
Autor:
Pastorello, A., Valerin, G., Fraser, M., Reguitti, A., Elias-Rosa, N., Filippenko, A. V., Rojas-Bravo, C., Tartaglia, L., Reynolds, T. M., Valenti, S., Andrews, J. E., Ashall, C., Bostroem, K. A., Brink, T. G., Burke, J., Cai, Y. -Z., Cappellaro, E., Coulter, D. A., Dastidar, R., Davis, K. W., Dimitriadis, G., Fiore, A., Foley, R. J., Fugazza, D., Galbany, L., Gangopadhyay, A., Geier, S., Gutierrez, C. P., Haislip, J., Hiramatsu, D., Holmbo, S., Howell, D. A., Hsiao, E. Y., Hung, T., Jha, S. W., Kankare, E., Karamehmetoglu, E., Kilpatrick, C. D., Kotak, R., Kouprianov, V., Kravtsov, T., Kumar, S., Li, Z. -T., Lundquist, M. J., Lundqvist, P., Matilainen, K., Mazzali, P. A., McCully, C., Misra, K., Morales-Garoffolo, A., Moran, S., Morrell, N., Newsome, M., Gonzalez, E. Padilla, Pan, Y. -C., Pellegrino, C., Phillips, M. M., Pignata, G., Piro, A. L., Reichart, D. E., Rest, A., Salmaso, I., Sand, D. J., Siebert, M. R., Smartt, S. J., Smith, K. W., Srivastav, S., Stritzinger, M. D., Taggart, K., Tinyanont, S., Yan, S. -Y., Wang, L., Wang, X. -F., Williams, S. C., Wyatt, S., Zhang, T. -M., de Boer, T., Chambers, K., Gao, H., Magnier, E.
Publikováno v:
A&A 671, A158 (2023)
We present photometric and spectroscopic data on three extragalactic luminous red novae (LRNe): AT2018bwo, AT2021afy, and AT2021blu. AT2018bwo was discovered in NGC45 (at 6.8 Mpc) a few weeks after the outburst onset. During the monitoring period, th
Externí odkaz:
http://arxiv.org/abs/2208.02782
Autor:
Valerin, G., Pumo, M. L., Pastorello, A., Reguitti, A., Elias-Rosa, N., Gútierrez, C. P., Kankare, E., Fraser, M., Mazzali, P. A., Howell, D. A., Kotak, R., Galbany, L., Williams, S. C., Cai, Y. -Z., Salmaso, I., Pinter, V., Müller-Bravo, T. E., Burke, J., Gonzalez, E. Padilla, Hiramatsu, D., McCully, C., Newsome, M., Pellegrino, C.
Photometric and spectroscopic data for two Low Luminosity Type IIP Supernovae (LL SNe IIP) are presented. SN 2020cxd reaches a peak absolute magnitude $M_{r}$ = -13.90 $\pm$ 0.05 mag two days after explosion, subsequently settling on a plateau for $\
Externí odkaz:
http://arxiv.org/abs/2203.03988
Autor:
Kuźniak, M., González-Díaz, D., Amedo, P., Azevedo, C. D. R., Fernández-Posada, D. J., Kuźwa, M., Leardini, S., Leonhardt, A., Łęcki, T., Manzanillas, L., Muenstermann, D., Nieradka, G., de Oliveira, R., Pollmann, T. R., Hernández, A. Saá, Sworobowicz, T., Türkoğlu, C., Williams, S.
Publikováno v:
Eur. Phys. J. C 81, 609 (2021)
A new concept for the simultaneous detection of primary and secondary scintillation in time projection chambers is proposed. Its core element is a type of very-thick GEM structure supplied with transparent electrodes and machined from a polyethylene
Externí odkaz:
http://arxiv.org/abs/2106.03773
Autor:
Ulukutlu, B., Gasik, P., Waldmann, T., Fabbietti, L., Klemenz, T., Lautner, L., de Oliveira, R., Williams, S.
Publikováno v:
Nuclear Inst. and Methods in Physics Research, A 1019 (2021) 165829
In this work GEM and single-hole Thick GEM structures, composed of different coating materials, are studied. The used foils incorporate conductive layers made of copper, aluminium, molybdenum, stainless steel, tungsten and tantalum. The main focus of
Externí odkaz:
http://arxiv.org/abs/2104.12191