Zobrazeno 1 - 10
of 361
pro vyhledávání: '"Doriese, W"'
Autor:
Okumura, T., Azuma, T., Bennett, D. A., Doriese, W. B., Durkin, M. S., Fowler, J. W., Gard, J. D., Hashimoto, T., Hayakawa, R., Ichinohe, Y., Indelicato, P., Isobe, T., Kanda, S., Kato, D., Katsuragawa, M., Kawamura, N., Kino, Y., Kominato, N., Miyake, Y., Morgan, K. M., Noda, H., O'Neil, G. C., Okada, S., Okutsu, K., Paul, N., Reintsema, C. D., Sato, T., Schmidt, D. R., Shimomura, K., Strasser, P., Swetz, D. S., Takahashi, T., Takeda, S., Takeshita, S., Tampo, M., Tatsuno, H., Tőkési, K., Tong, X. M., Toyama, Y., Ullom, J. N., Watanabe, S., Yamada, S., Yamashita, T.
Electronic $K$ x rays emitted by muonic Ar atoms in the gas phase were observed using a superconducting transition-edge-sensor microcalorimeter. The high-precision energy spectra provided a clear signature of the presence of muonic atoms accompanied
Externí odkaz:
http://arxiv.org/abs/2407.07977
Autor:
Vaccaro, D., de Wit, M., van der Kuur, J., Gottardi, L., Ravensberg, K., Taralli, E., Adams, J., Bandler, S. R., Chervenak, J. A., Doriese, W. B., Durkin, M., Reintsema, C., Sakai, K., Smith, S. J., Wakeham, N. A., Jackson, B., Khosropanah, P., Gao, J. R., Herder, J. W. A. den, Roelfsema, P.
SRON (Netherlands Institute for Space Research) is developing the Focal Plane Assembly (FPA) for Athena X-IFU, whose Demonstration Model (DM) will use for the first time a time domain multiplexing (TDM)-based readout system for the on-board transitio
Externí odkaz:
http://arxiv.org/abs/2403.02978
Autor:
Goldfinger, David C., Ahmed, Zeeshan, Barron, Darcy R., Doriese, W. Bertrand, Durkin, Malcolm, Filippini, Jeffrey P., Haller, Gunther, Henderson, Shawn W., Herbst, Ryan, Hubmayr, Johannes, Irwin, Kent, Reese, Ben, Sapozhnikov, Leonid, Thompson, Keith L., Ullom, Joel, Vissers, Michael R.
The CMB-S4 experiment is developing next-generation ground-based microwave telescopes to observe the Cosmic Microwave Background with unprecedented sensitivity. This will require an order of magnitude increase in the 100 mK detector count, which in t
Externí odkaz:
http://arxiv.org/abs/2311.04424
Autor:
Szypryt, Paul, Nakamura, Nathan, Becker, Daniel T., Bennett, Douglas A., Dagel, Amber L., Doriese, W. Bertrand, Fowler, Joseph W., Gard, Johnathon D., Harris, J. Zachariah, Hilton, Gene C., Imrek, Jozsef, Jimenez, Edward S., Larson, Kurt W., Levine, Zachary H., Mates, John A. B., McArthur, D., Miaja-Avila, Luis, Morgan, Kelsey M., O'Neil, Galen C., Ortiz, Nathan J., Pappas, Christine G., Schmidt, Daniel R., Thompson, Kyle R., Ullom, Joel N., Vale, Leila, Vissers, Michael R., Walker, Christopher, Weber, Joel C., Wessels, Abigail L., Wheeler, Jason W., Swetz, Daniel S.
Publikováno v:
IEEE Transactions on Applied Superconductivity, vol. 33, no. 5, pp. 1-5, Aug. 2023, Art no. 2100705
We report on the 1,000-element transition-edge sensor (TES) x-ray spectrometer implementation of the TOMographic Circuit Analysis Tool (TOMCAT). TOMCAT combines a high spatial resolution scanning electron microscope (SEM) with a highly efficient and
Externí odkaz:
http://arxiv.org/abs/2212.12073
Autor:
Nakamura, Nathan, Szypryt, Paul, Dagel, Amber L., Alpert, Bradley K., Bennett, Douglas A., Doriese, W. Bertrand, Durkin, Malcolm, Fowler, Joseph W., Fox, Dylan T., Gard, Johnathon D., Goodner, Ryan N., Harris, J. Zachariah, Hilton, Gene C., Jimenez, Edward S., Kernen, Burke L., Larson, Kurt W., Levine, Zachary H., McArthur, Daniel, Morgan, Kelsey M., O'Neil, Galen C., Ortiz, Nathan J., Pappas, Christine G., Reintsema, Carl D., Schmidt, Daniel R., Schultz, Peter A., Thompson, Kyle R., Ullom, Joel N., Vale, Leila, Vaughan, Courtenay T., Walker, Christopher, Weber, Joel C., Wheeler, Jason W., Swetz, Daniel S.
X-ray nanotomography is a powerful tool for the characterization of nanoscale materials and structures, but is difficult to implement due to competing requirements on X-ray flux and spot size. Due to this constraint, state-of-the-art nanotomography i
Externí odkaz:
http://arxiv.org/abs/2212.10591
Autor:
Szypryt, Paul, Bennett, Douglas A., Boone, William J., Dagel, Amber L., Dalton, Gabriella, Doriese, W. Bertrand, Fowler, Joseph W., Garboczi, Edward J., Gard, Johnathon D., Hilton, Gene C., Imrek, Jozsef, Jimenez, Edward S., Kotsubo, Vincent Y., Larson, Kurt, Levine, Zachary H., Mates, John A. B., McArthur, Daniel, Morgan, Kelsey M., Nakamura, Nathan, O'Neil, Galen C., Ortiz, Nathan J., Pappas, Christine G., Reintsema, Carl D., Schmidt, Daniel R., Swetz, Daniel S., Thompson, Kyle R., Ullom, Joel N., Walker, Christopher, Weber, Joel C., Wessels, Abigail L., Wheeler, Jason W.
Publikováno v:
in IEEE Transactions on Applied Superconductivity, vol. 31, no. 5, pp. 1-5, Aug. 2021, Art no. 2100405
Feature sizes in integrated circuits have decreased substantially over time, and it has become increasingly difficult to three-dimensionally image these complex circuits after fabrication. This can be important for process development, defect analysi
Externí odkaz:
http://arxiv.org/abs/2212.07460
Autor:
Kraft, Ralph, Markevitch, Maxim, Kilbourne, Caroline, Adams, Joseph S., Akamatsu, Hiroki, Ayromlou, Mohammadreza, Bandler, Simon R., Barbera, Marco, Bennett, Douglas A., Bhardwaj, Anil, Biffi, Veronica, Bodewits, Dennis, Bogdan, Akos, Bonamente, Massimiliano, Borgani, Stefano, Branduardi-Raymont, Graziella, Bregman, Joel N., Burchett, Joseph N., Cann, Jenna, Carter, Jenny, Chakraborty, Priyanka, Churazov, Eugene, Crain, Robert A., Cumbee, Renata, Dave, Romeel, DiPirro, Michael, Dolag, Klaus, Doriese, W. Bertrand, Drake, Jeremy, Dunn, William, Eckart, Megan, Eckert, Dominique, Ettori, Stefano, Forman, William, Galeazzi, Massimiliano, Gall, Amy, Gatuzz, Efrain, Hell, Natalie, Hodges-Kluck, Edmund, Jackman, Caitriona, Jahromi, Amir, Jennings, Fred, Jones, Christine, Kaaret, Philip, Kavanagh, Patrick J., Kelley, Richard L., Khabibullin, Ildar, Kim, Chang-Goo, Koutroumpa, Dimitra, Kovacs, Orsolya, Kuntz, K. D., Lau, Erwin, Lee, Shiu-Hang, Leutenegger, Maurice, Lin, Sheng-Chieh, Lisse, Carey, Cicero, Ugo Lo, Lovisari, Lorenzo, McCammon, Dan, McEntee, Sean, Mernier, Francois, Miller, Eric D., Nagai, Daisuke, Negro, Michela, Nelson, Dylan, Ness, Jan-Uwe, Nulsen, Paul, Ogorzalek, Anna, Oppenheimer, Benjamin D., Oskinova, Lidia, Patnaude, Daniel, Pfeifle, Ryan W., Pillepich, Annalisa, Plucinsky, Paul, Pooley, David, Porter, Frederick S., Randall, Scott, Rasia, Elena, Raymond, John, Ruszkowski, Mateusz, Sakai, Kazuhiro, Sarkar, Arnab, Sasaki, Manami, Sato, Kosuke, Schellenberger, Gerrit, Schaye, Joop, Simionescu, Aurora, Smith, Stephen J., Steiner, James F., Stern, Jonathan, Su, Yuanyuan, Sun, Ming, Tremblay, Grant, Truong, Nhut, Tutt, James, Ursino, Eugenio, Veilleux, Sylvain, Vikhlinin, Alexey, Vladutescu-Zopp, Stephan, Vogelsberger, Mark, Walker, Stephen A., Weaver, Kimberly, Weigt, Dale M., Werk, Jessica, Werner, Norbert, Wolk, Scott J., Zhang, Congyao, Zhang, William W., Zhuravleva, Irina, ZuHone, John
The Line Emission Mapper (LEM) is an X-ray Probe for the 2030s that will answer the outstanding questions of the Universe's structure formation. It will also provide transformative new observing capabilities for every area of astrophysics, and to hel
Externí odkaz:
http://arxiv.org/abs/2211.09827
Arrays of low-temperature microcalorimeters provide a promising technology for X-ray astrophysics: the imaging spectrometer. A camera with at least several thousand pixels, each of which has an energy-resolving power ($E/\Delta E\urss{FWHM}$) of a fe
Externí odkaz:
http://arxiv.org/abs/2209.05621
Autor:
Castellani, Florent, Beaumont, Sophie, Pajot, François, Roudil, Gilles, Adams, Joseph, Bandler, Simon, Chervenak, James, Daniel, Christophe, Denison, Edward V, Doriese, W Bertrand, Dupieux, Michel, Durkin, Malcolm, Geoffray, Hervé, Hilton, Gene C, Murat, David, Parot, Yann, Peille, Philippe, Prêle, Damien, Ravera, Laurent, Reintsema, Carl D, Sakai, Kazuhiro, Stevens, Robert W, Ullom, Joel N, Vale, Leila R, Wakeham, Nicholas
The X-IFU (X-ray Integral Field Unit) onboard the large ESA mission Athena (Advanced Telescope for High ENergy Astrophysics), planned to be launched in the mid 2030s, will be a cryogenic X-ray imaging spectrometer operating at 55 mK. It will provide
Externí odkaz:
http://arxiv.org/abs/2209.04151
Autor:
Barron, D. R., Ahmed, Z., Aguilar, J., Anderson, A. J., Baker, C. F., Barry, P. S., Beall, J. A., Bender, A. N., Benson, B. A., Besuner, R. W., Cecil, T. W., Chang, C. L., Chapman, S. C., Chesmore, G. E., Derylo, G., Doriese, W. B., Duff, S. M., Elleflot, T., Filippini, J. P., Flaugher, B., Gomez, J. G., Grimes, P. K., Gualtieri, R., Gullett, I., Haller, G., Henderson, S. W., Henke, D., Herbst, R., Huber, A. I., Hubmayr, J., Jonas, M., Joseph, J., King, C. L., Kovac, J. M., Kubik, D., Lisovenko, M., McMahon, J. J., Moncelsi, L., Nagy, J. M., Osherson, B., Reese, B., Ruhl, J. E., Sapozhnikov, L., Schillaci, A., Simon, S. M., Suzuki, A., Wang, G., Westbrook, B., Yefremenko, V., Zhang, J.
We present the conceptual design of the modular detector and readout system for the Cosmic Microwave Background Stage 4 (CMB-S4) ground-based survey experiment. CMB-S4 will map the cosmic microwave background (CMB) and the millimeter-wave sky to unpr
Externí odkaz:
http://arxiv.org/abs/2208.02284