Zobrazeno 1 - 10
of 67
pro vyhledávání: '"Smecher, Graeme"'
Autor:
Rouble, Maclean, Smecher, Graeme, Adamič, Michel, Anderson, Adam, Barry, Peter S., Dibert, Karia, Dobbs, Matt, Fichman, Kyra, Montgomery, Joshua
RF-ICE is a signal processing platform for the readout of large arrays of superconducting resonators. Designed for flexibility, the system's low digital latency and ability to independently and dynamically set the frequency and amplitude of probe ton
Externí odkaz:
http://arxiv.org/abs/2406.17175
Autor:
Montgomery, Joshua, Avelino, Wellington, Dobbs, Matt, Letang, Joseph, Rouble, Maclean, Savchyn, Sofiia, Smecher, Graeme
Publikováno v:
Proceedings Volume 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII; 131020R (2024)
The t0.technology Control and Readout System (CRS) is a modular microwave control and readout system for mm-wave and radio astronomy, THz imaging, noise radar, and superconducting qubit control. The configuration discussed in this work implements fir
Externí odkaz:
http://arxiv.org/abs/2406.16266
LiteBIRD is a space-borne experiment dedicated to detecting large-scale $B$-mode anisotropies in the linear polarization of the Cosmic Microwave Background (CMB) predicted by the theory of inflation. It is planned to be launched in the late 2020s to
Externí odkaz:
http://arxiv.org/abs/2209.12492
We consider the stability and performance of a discrete-time control loop used as a dynamic nuller in the presence of a relatively large time delay in its feedback path. Controllers of this form occur in mm-wave telescopes using frequency-multiplexed
Externí odkaz:
http://arxiv.org/abs/2207.11377
The next generation of space-based mm-wave telescopes, such as JAXA's LiteBIRD mission, require focal planes with thousands of detectors in order to achieve their science goals. Digital frequency-domain multiplexing (dfmux) techniques allow detector
Externí odkaz:
http://arxiv.org/abs/2207.11375
The next generation of space-based mm-wave telescopes, such as JAXA's LiteBIRD mission, require focal planes with thousands of detectors in order to achieve their science goals. Digital frequency-domain multiplexing (dfmux) techniques allow detector
Externí odkaz:
http://arxiv.org/abs/2207.11374
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Pan, Zhaodi, Ade, Peter, Ahmed, Zeeshan, Adam, Anderson, Austermann, Jason, Avva, Jessica, Thakur, Ritoban Basu, Amy, Bender, Benson, Bradford, Carlstrom, John, Carter, Faustin, Cecil, Thomas, Chang, Clarence, Cliche, Jean-Francois, Cukierman, Ariel, Denison, Edward, de Haan, Tijmen, Ding, Junjia, Dobbs, Matt, Dutcher, Daniel, Everett, Wendeline, Foster, Allen, Gannon, Renae, Gilbert, Adam, Groh, John, Halverson, Nils, Harke-Horsemann, Angelina, Harrington, Nicholas, Henning, Jaosn, Hilton, Gene, Holzapfel, William, Huang, Nicholas, Irwin, Kent, Jeong, Oliver, Jonas, Michalle, Khaire, Trupti, Kofman, Anna, Korman, Milo, Kubik, Donna, Kuhlmann, Steve, Kuo, Chaolin, Lee, Adrian, Lowitz, Amy, Meyer, Stephan, Michalik, Daniel, Montgomery, Joshua, Nadolski, Andrew, Natoli, Tyler, Nguyen, Hogan, Noble, Gavin, Novosad, Valentyn, Padin, Stephan, Pearson, John, Posada, Chrystian, Rahlin, Alexandra, Ruhl, John, Saunders, Lauren, Sayre, James, Shirley, Ian, Shirokoff, Erik, Smecher, Graeme, Sobrin, Joshua, Stark, Antony, Story, Kyle, Suzuki, Aritoki, Tang, Qingyang, Thompson, Keith, Tucker, Carole, Vale, Leila, Vanderlinde, Keith, Vieira, Joaquin, Wang, Gensheng, Whitehorn, Nathan, Yefremenko, Volodymyr, Yoon, Ki Won, Young, Matt
The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-edge sensor (TES) bolometers. Each multichroic pixel on a detector wafe
Externí odkaz:
http://arxiv.org/abs/1805.03219
Autor:
The EBEX Collaboration, Abitbol, Maximilian, Aboobaker, Asad M., Ade, Peter, Araujo, Derek, Aubin, François, Baccigalupi, Carlo, Bao, Chaoyun, Chapman, Daniel, Didier, Joy, Dobbs, Matt, Feeney, Stephen M., Geach, Christopher, Grainger, Will, Hanany, Shaul, Helson, Kyle, Hillbrand, Seth, Hilton, Gene, Hubmayr, Johannes, Irwin, Kent, Jaffe, Andrew, Johnson, Bradley, Jones, Terry, Klein, Jeff, Korotkov, Andrei, Lee, Adrian, Levinson, Lorne, Limon, Michele, MacDermid, Kevin, Miller, Amber D., Milligan, Michael, Raach, Kate, Reichborn-Kjennerud, Britt, Reintsema, Carl, Sagiv, Ilan, Smecher, Graeme, Tucker, Gregory S., Westbrook, Benjamin, Young, Karl, Zilic, Kyle
EBEX was a long-duration balloon-borne experiment to measure the polarization of the cosmic microwave background. The experiment had three frequency bands centered at 150, 250, and 410 GHz and was the first to use a kilo-pixel array of transition edg
Externí odkaz:
http://arxiv.org/abs/1803.01018
Autor:
Bandura, Kevin, Cliche, Jean-Francois, Dobbs, Matt, Gilbert, Adam, Ittah, David, Parra, Juan Mena, Smecher, Graeme
New generation radio interferometers encode signals from thousands of antenna feeds across large bandwidth. Channelizing and correlating this data requires networking capabilities that can handle unprecedented data rates with reasonable cost. The Can
Externí odkaz:
http://arxiv.org/abs/1608.04347