Zobrazeno 1 - 10
of 450
pro vyhledávání: '"Crowley, P. D."'
Autor:
Galitzki, Nicholas, Tsan, Tran, Spisak, Jake, Randall, Michael, Silva-Feaver, Max, Seibert, Joseph, Lashner, Jacob, Adachi, Shunsuke, Adkins, Sean M., Alford, Thomas, Arnold, Kam, Ashton, Peter C., Austermann, Jason E., Baccigalupi, Carlo, Bazarko, Andrew, Beall, James A., Bhimani, Sanah, Bixler, Bryce, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D., Crowley, Kevin T., Day-Weiss, Samuel, Dicker, Simon, Dow, Peter N., Duell, Cody J., Duff, Shannon M., Gerras, Remington G., Groh, John C., Gudmundsson, Jon E., Harrington, Kathleen, Hasegawa, Masaya, Healy, Erin, Henderson, Shawn W., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keating, Brian, Keller, Ben, Kiuchi, Kenji, Kofman, Anna M., Koopman, Brian J., Kusaka, Akito, Lee, Adrian T., Lew, Richard A., Lin, Lawrence T., Link, Michael J, Lucas, Tammy J., Lungu, Marius, Mangu, Aashrita, McMahon, Jeffrey J, Miller, Amber D., Moore, Jenna E., Morshed, Magdy, Nakata, Hironobu, Nati, Federico, Newburgh, Laura B., Nguyen, David V., Niemack, Michael D., Page, Lyman A., Sakaguri, Kana, Sakurai, Yuki, Rao, Mayuri Sathyanarayana, Saunders, Lauren J., Shroyer, Jordan E., Sugiyama, Junna, Tajima, Osamu, Takeuchi, Atsuto, Bua, Refilwe Tanah, Teply, Grant, Terasaki, Tomoki, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R, Walters, Liam, Wang, Yuhan, Xu, Zhilei, Yamada, Kyohei, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands betwee
Externí odkaz:
http://arxiv.org/abs/2405.05550
Autor:
Crowley, Kevin D., McLellan, Russell A., Dutta, Aveek, Shumiya, Nana, Place, Alexander P. M., Le, Xuan Hoang, Gang, Youqi, Madhavan, Trisha, Khedkar, Nishaad, Feng, Yiming Cady, Umbarkar, Esha A., Gui, Xin, Rodgers, Lila V. H., Jia, Yichen, Feldman, Mayer M., Lyon, Stephen A., Liu, Mingzhao, Cava, Robert J., Houck, Andrew A., de Leon, Nathalie P.
Superconducting qubits are a leading system for realizing large scale quantum processors, but overall gate fidelities suffer from coherence times limited by microwave dielectric loss. Recently discovered tantalum-based qubits exhibit record lifetimes
Externí odkaz:
http://arxiv.org/abs/2301.07848
Autor:
McLellan, Russell A., Dutta, Aveek, Zhou, Chenyu, Jia, Yichen, Weiland, Conan, Gui, Xin, Place, Alexander P. M., Crowley, Kevin D., Le, Xuan Hoang, Madhavan, Trisha, Gang, Youqi, Baker, Lukas, Head, Ashley R., Waluyo, Iradwikanari, Li, Ruoshui, Kisslinger, Kim, Hunt, Adrian, Jarrige, Ignace, Lyon, Stephen A., Barbour, Andi M., Cava, Robert J., Houck, Andrew A., Hulbert, Steven L., Liu, Mingzhao, Walter, Andrew L., de Leon, Nathalie P.
Over the past decades, superconducting qubits have emerged as one of the leading hardware platforms for realizing a quantum processor. Consequently, researchers have made significant effort to understand the loss channels that limit the coherence tim
Externí odkaz:
http://arxiv.org/abs/2301.04567
Autor:
Crowley, Kevin D., Dow, Peter, Shroyer, Jordan E., Groh, John C., Dober, Bradley, Spisak, Jacob, Galitzki, Nicholas, Bhandarkar, Tanay, Devlin, Mark J., Dicker, Simon, Gallardo, Patricio A., Harrington, Kathleen, Johnson, Bradley R., Johnson, Delwin, Kofman, Anna M., Kusaka, Akito, Lee, Adrian, Limon, Michele, Iuliano, Jeffrey, Nati, Federico, Orlowski-Scherer, John, Page, Lyman, Randall, Michael, Teply, Grant, Tsan, Tran, Wollack, Edward J., Xu, Zhilei, Zhu, Ningfeng
Publikováno v:
Review of Scientific Instruments 93, 055106 (2022)
We present the design and measured performance of a new carbon fiber strut design that is used in a cryogenically cooled truss for the Simons Observatory Small Aperture Telescope (SAT). The truss consists of two aluminum 6061 rings separated by 24 st
Externí odkaz:
http://arxiv.org/abs/2201.06094
Autor:
McCarrick, Heather, Healy, Erin, Ahmed, Zeeshan, Arnold, Kam, Atkins, Zachary, Austermann, Jason E., Bhandarkar, Tanay, Beall, Jim A., Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Crowley, Kevin D., Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dutcher, Daniel, Frisch, Josef C., Galitzki, Nicholas, Gralla, Megan B., Gudmundsson, Jon E., Henderson, Shawn W., Hilton, Gene C., Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Kofman, Anna M., Kusaka, Akito, Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Link, Michael J., Lucas, Tammy J., Lungu, Marius, Mates, J. A. B., McMahon, Jeffrey J., Niemack, Michael D., Orlowski-Scherer, John, Seibert, Joseph, Silva-Feaver, Maximiliano, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Terasaki, Tomoki, Ullom, Joel N., Vavagiakis, Eve M., Vale, Leila R., Van Lanen, Jeff, Vissers, Michael R., Wang, Yuhan, Wollack, Edward J., Xu, Zhilei, Young, Edward, Yu, Cyndia, Zheng, Kaiwen, Zhu, Ningfeng
Publikováno v:
2021 ApJ 922 38
Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever lar
Externí odkaz:
http://arxiv.org/abs/2106.14797
Autor:
Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Beall, J. A., Bhandarkar, Tanay, Bond, J. Richard, Chesmore, Grace E., Chinone, Yuji, Choi, Steve K., Connors, Jake A., Coppi, Gabriele, Cothard, Nicholas F., Crowley, Kevin D., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Gudmundsson, Jon E., Haridas, Saianeesh K., Harrington, Kathleen, Hervias-Caimapo, Carlos, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Kaneko, Daisuke, Kofman, Anna M., Koopman, Brian J., Lashner, Jack, Limon, Michele, Link, Michael J., Lucas, Tammy J., Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Orlowski-Scherer, John, Piccirillo, Lucio, Sarmiento, Karen Perez, Schaan, Emmanuel, Silva-Feaver, Maximiliano, Sonka, Rita, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Terasaki, Tomoki, Thornton, Robert, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Whipps, Zachary, Wollack, Edward J., Zannoni, Mario, Zhu, Ningfeng, Zonca, Andrea
Publikováno v:
Research Notes AAS, 5, 100 (2021)
The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at $\sim$5200m altitude -- comprises three Small Aperture Telescopes (SATs) and
Externí odkaz:
http://arxiv.org/abs/2104.09511
Autor:
Kiuchi, Kenji, Adachi, Shunsuke, Ali, Aamir M., Arnold, Kam, Ashton, Peter, Austermann, Jason E., Bazako, Andrew, Beall, James A., Chinone, Yuji, Coppi, Gabriele, Crowley, Kevin D., Crowley, Kevin T., Dicker, Simon, Dober, Bradley, Duff, Shannon M., Fabbian, Giulio, Galitzki, Nicholas, Golec, Joseph E., Gudmundsson, Jon E., Harrington, Kathleen, Hasegawa, Masaya, Hattori, Makoto, Hill, Charles A., Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Johnson, Bradley R., Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Kusaka, Akito, Lashner, Jack, Lee, Adrian T., Matsuda, Frederick, McCarrick, Heather, Murata, Masaaki, Nati, Federico, Nishinomiya, Yume, Page, Lyman, Rao, Mayuri Sathyanarayana, Reichardt, Christian L., Sakaguri, Kana, Sakurai, Yuki, Seibert, Joseph, Spisak, Jacob, Tajima, Osamu, Teply, Grant P., Terasaki, Tomoki, Tsan, Tran, Walker, Samantha, Wollack, Edward J., Xu, Zhilei, Yamada, Kyohei, Zannoni, Mario, Zhu, Ningfeng
Publikováno v:
Proc. SPIE 11445, Ground-based and Airborne Telescopes VIII, 114457L (18 December 2020)
The Simons Observatory (SO) is a cosmic microwave background (CMB) experiment from the Atacama Desert in Chile comprising three small-aperture telescopes (SATs) and one large-aperture telescope (LAT). In total, SO will field over 60,000 transition-ed
Externí odkaz:
http://arxiv.org/abs/2101.11917
Autor:
Abitbol, Maximilian H., Alonso, David, Simon, Sara M., Lashner, Jack, Crowley, Kevin T., Ali, Aamir M., Azzoni, Susanna, Baccigalupi, Carlo, Barron, Darcy, Brown, Michael L., Calabrese, Erminia, Carron, Julien, Chinone, Yuji, Chluba, Jens, Coppi, Gabriele, Crowley, Kevin D., Devlin, Mark, Dunkley, Jo, Errard, Josquin, Fanfani, Valentina, Galitzki, Nicholas, Gerbino, Martina, Hill, J. Colin, Johnson, Bradley R., Jost, Baptiste, Keating, Brian, Krachmalnicoff, Nicoletta, Kusaka, Akito, Lee, Adrian T., Louis, Thibaut, Madhavacheril, Mathew S., McCarrick, Heather, McMahon, Jeffrey, Meerburg, P. Daniel, Nati, Federico, Nishino, Haruki, Page, Lyman A., Poletti, Davide, Puglisi, Giuseppe, Randall, Michael J., Rotti, Aditya, Spisak, Jacob, Suzuki, Aritoki, Teply, Grant P., Vergès, Clara, Wollack, Edward J., Xu, Zhilei, Zannoni, Mario
We quantify the calibration requirements for systematic uncertainties for next-generation ground-based observatories targeting the large-angle $B$-mode polarization of the Cosmic Microwave Background, with a focus on the Simons Observatory (SO). We e
Externí odkaz:
http://arxiv.org/abs/2011.02449
Autor:
Ali, Aamir M., Adachi, Shunsuke, Arnold, Kam, Ashton, Peter, Bazarko, Andrew, Chinone, Yuji, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D, Crowley, Kevin T, Devlin, Mark, Dicker, Simon, Duff, Shannon, Ellis, Chris, Galitzki, Nicholas, Goeckner-Wald, Neil, Harrington, Kathleen, Healy, Erin, Hill, Charles A, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Keating, Brian, Kiuchi, Kenji, Kusaka, Akito, Lee, Adrian T, Ludlam, Michael, Mangu, Aashrita, Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Nishino, Haruki, Orlowski-Scherer, John, Rao, Mayuri Sathyanarayana, Raum, Christopher, Sakurai, Yuki, Salatino, Maria, Sasse, Trevor, Seibert, Joseph, Sierra, Carlos, Silva-Feaver, Maximiliano, Spisak, Jacob, Simon, Sara M, Staggs, Suzanne, Tajima, Osamu, Teply, Grant, Tsan, Tran, Wollack, Edward, Westbrook, Bejamin, Xu, Zhilei, Zannoni, Mario, Zhu, Ningfeng
The Simons Observatory (SO) is an upcoming cosmic microwave background (CMB) experiment located on Cerro Toco, Chile, that will map the microwave sky in temperature and polarization in six frequency bands spanning 27 to 285 GHz. SO will consist of on
Externí odkaz:
http://arxiv.org/abs/2001.07848
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.