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5 results on '"Young, Edward Y."'

1. CMB-S4 Technology Book, First Edition

Author

Abitbol, Maximilian H., Ahmed, Zeeshan, Barron, Darcy, Thakur, Ritoban Basu, Bender, Amy N., Benson, Bradford A., Bischoff, Colin A., Bryan, Sean A., Carlstrom, John E., Chang, Clarence L., Chuss, David T., Crowley, Kevin T., Cukierman, Ari, de Haan, Tijmen, Dobbs, Matt, Essinger-Hileman, Tom, Filippini, Jeffrey P., Ganga, Ken, Gudmundsson, Jon E., Halverson, Nils W., Hanany, Shaul, Henderson, Shawn W., Hill, Charles A., Ho, Shuay-Pwu P., Hubmayr, Johannes, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Kernasovskiy, Sarah A., Kovac, John M., Kusaka, Akito, Lee, Adrian T., Maria, Salatino, Mauskopf, Philip, McMahon, Jeff J., Moncelsi, Lorenzo, Nadolski, Andrew W., Nagy, Johanna M., Niemack, Michael D., O'Brient, Roger C., Padin, Stephen, Parshley, Stephen C., Pryke, Clement, Roe, Natalie A., Rostem, Karwan, Ruhl, John, Simon, Sara M., Staggs, Suzanne T., Suzuki, Aritoki, Switzer, Eric R., Tajima, Osamu, Thompson, Keith L., Timbie, Peter, Tucker, Gregory S., Vieira, Joaquin D., Vieregg, Abigail G., Westbrook, Benjamin, Wollack, Edward J., Yoon, Ki Won, Young, Karl S., and Young, Edward Y.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible from the ground. The science goals and capabilities of CMB-S4 in illuminating cosmic inflation, measuring the sum of neutrino masses, searching for relativistic relics in the early universe, characterizing dark energy and dark matter, and mapping the matter distribution in the universe have been described in the CMB-S4 Science Book. This Technology Book is a companion volume to the Science Book. The ambitious science goals of CMB-S4, a "Stage-4" experiment, require a step forward in experimental capability from the current Stage=II experiments. To guide this process, we summarize the current state of CMB instrumentation technology, and identify R&D efforts necessary to advance it for use in CMB-S4. The book focuses on technical challenges in four broad areas: Telescope Design; Receiver Optics; Focal-Plane Optical Coupling; and Focal-Plane Sensor and Readout., Comment: 191 pages

Published
2017

2. Pointing control for the SPIDER balloon-borne telescope

Author

Shariff, Jamil A., Ade, Peter A. R., Amiri, Mandana, Benton, Steven J., Bock, Jamie J., Bond, J. Richard, Bryan, Sean A., Chiang, H. Cynthia, Contaldi, Carlo R., Crill, Brendan P., Doré, Olivier P., Farhang, Marzieh, Filippini, Jeffrey P., Fissel, Laura M., Fraisse, Aurelien A., Gambrel, Anne E., Gandilo, Natalie N., Golwala, Sunil R., Gudmundsson, Jon E., Halpern, Mark, Hasselfield, Matthew, Hilton, Gene C., Holmes, Warren A., Hristov, Viktor V., Irwin, Kent D., Jones, William C., Kermish, Zigmund D., Kuo, Chao-Lin, MacTavish, Carolyn J., Mason, Peter V., Megerian, Krikor G., Moncelsi, Lorenzo, Morford, Tracy A., Nagy, Johanna M., Netterfield, C. Barth, O'Brient, Roger, Rahlin, Alexandra S., Reintsema, Carl D., Ruhl, John E., Runyan, Marcus C., Soler, Juan D., Trangsrud, Amy, Tucker, Carole E., Tucker, Rebecca S., Turner, Anthony D., Weber, Alexis C., Wiebe, Donald V., and Young, Edward Y.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present the technology and control methods developed for the pointing system of the SPIDER experiment. SPIDER is a balloon-borne polarimeter designed to detect the imprint of primordial gravitational waves in the polarization of the Cosmic Microwave Background radiation. We describe the two main components of the telescope's azimuth drive: the reaction wheel and the motorized pivot. A 13 kHz PI control loop runs on a digital signal processor, with feedback from fibre optic rate gyroscopes. This system can control azimuthal speed with < 0.02 deg/s RMS error. To control elevation, SPIDER uses stepper-motor-driven linear actuators to rotate the cryostat, which houses the optical instruments, relative to the outer frame. With the velocity in each axis controlled in this way, higher-level control loops on the onboard flight computers can implement the pointing and scanning observation modes required for the experiment. We have accomplished the non-trivial task of scanning a 5000 lb payload sinusoidally in azimuth at a peak acceleration of 0.8 deg/s$^2$, and a peak speed of 6 deg/s. We can do so while reliably achieving sub-arcminute pointing control accuracy., Comment: 20 pages, 12 figures, Presented at SPIE Ground-based and Airborne Telescopes V, June 23, 2014. To be published in Proceedings of SPIE Volume 9145

Published
2014
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3. In-flight performance of Spider’s 280-GHz receivers

Author

Shaw, Elle C., Ade, Peter A. R., Akers, Scott, Amiri, Mandana, Austermann, Jason, Beall, James, Becker, Daniel T., Benton, Steven J., Bergman, Amanda S., Bock, James J., Bond, John R., Bryan, Sean A., Chiang, H. Cynthia, Contaldi, Carlo R., Domagalski, Rachel S., Doré, Olivier, Duff, Shannon M., Duivenvoorden, Adri J., Eriksen, Hans K., Farhang, Marzeih, Filippini, Jeffrey P., Fissel, Laura M., Fraisse, Aurelien A., Freese, Katherine, Galloway, Mathew, Gambrel, Anne E., Gandilo, Natalie N., Ganga, Kenneth, Gibbs, Sho M., Gourapura, Suren, Grigorian, Arpi, Gualtieri, Ricardo, Gudmundsson, Jón E., Halpern, Mark, Hartley, John, Hasselfield, Matthew, Hilton, Gene, Holmes, Warren, Hristov, Viktor V., Huang, Zhiqi, Hubmayr, Johannes, Irwin, Kent D., Jones, William C., Kahn, Asad, Kermish, Zigmund D., King, Cesiley, Kuo, Calvin L., Lennox, Amber R., Leung, Jason S.-Y., Li, Steven, Luu, Thuy Vy T., Mason, Peter V., May, Jared, Megerian, Krikor, Moncelsi, Lorenzo, Morford, Thomas A., Nagy, Johanna M., Nie, Rong, Netterfield, Calvin B., Nolta, Michael, Osherson, Benjamin, Padilla, Ivan L., Rahlin, Alexandra S., Redmond, Susan, Reintsema, Carl, Romualdez, L. Javier, Ruhl, John E., Runyan, Marcus C., Shariff, Jamil A., Shiu, Corwin, Soler, Juan D., Song, Xue, Tartakovsky, Simon, Thommesen, Harald, Trangsrud, Amy, Tucker, Carole, Turner, Anthony D., Ullom, Joel, van der List, Joseph F., Van Lanen, Jeff, Vissers, Michael R., Weber, Alexis C., Wehus, Ingunn K., Wen, Shyang, Wiebe, Donald V., and Young, Edward Y.

Published
2025
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4. Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole

Author

Moncelsi, Lorenzo, primary, Ade, Peter A., additional, Ahmed, Zeeshan, additional, Amiri, Mandana, additional, Barkats, Denis, additional, Basu Thakur, Ritoban, additional, Bischoff, Colin A., additional, Bock, Jamie J., additional, Buza, Victor, additional, Cheshire, James R., additional, Connors, Jake, additional, Cornelison, James, additional, Crumrine, Michael, additional, Cukierman, Ari J., additional, Denison, Edward, additional, Dierickx, Marion, additional, Duband, Lionel, additional, Eiben, Miranda, additional, Fatigoni, Sofia, additional, Filippini, Jeffrey P., additional, Goeckner-Wald, Neil, additional, Goldfinger, David, additional, Grayson, James A., additional, Grimes, Paul, additional, Hall, Grantland, additional, Halpern, Mark, additional, Harrison, Samuel A., additional, Henderson, Shawn, additional, Hildebrandt, Sergi, additional, Hilton, Gene, additional, Hubmayr, Johannes, additional, Hui, Howard, additional, Irwin, Kent D., additional, Kang, Jae Hwan, additional, Karkare, Kirit S., additional, Kefeli, Sinan, additional, Kovac, John M., additional, Kuo, Chao-Lin, additional, Lau, Kenny, additional, Leitch, Erik M., additional, Megerian, Krikor G., additional, Minutolo, Lorenzo, additional, Nakato, Yuka, additional, Namikawa, Toshiya, additional, Nguyen, Hien T., additional, O'brient, Roger C., additional, Palladino, Steven, additional, Precup, Nathan, additional, Prouve, Thomas, additional, Pryke, Clement, additional, Racine, Benjamin, additional, Reintsema, Carl D., additional, Schillaci, Alessandro, additional, Schmitt, Benjamin, additional, Soliman, Ahmed, additional, St. Germaine, Tyler, additional, Steinbach, Bryan, additional, R.Sudiwala@astro.cf.ac.uk, Rashmi, additional, Thompson, Keith L., additional, Tucker, Carole, additional, Turner, Anthony D., additional, Umiltà, Caterina, additional, Vieregg, Abigail G., additional, Wandui, Albert, additional, Weber, Alexis C., additional, Wiebe, Don V., additional, Willmert, Justin, additional, Wu, Wai Ling K., additional, Yang, Hung-I E., additional, Yoon, Ki Won, additional, Young, Edward Y., additional, Yu, Cyndia, additional, Zeng, Lingzhen, additional, Zhang, Cheng, additional, and Zhang, Silvia, additional

Published
2020
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5. CMB-S4 Technology Book, First Edition

Author

Abitbol, Maximilian H., Ahmed, Zeeshan, Barron, Darcy, Thakur, Ritoban Basu, Bender, Amy N., Benson, Bradford A., Bischoff, Colin A., Bryan, Sean A., Carlstrom, John E., Chang, Clarence L., Chuss, David T., Crowley, Kevin T., Cukierman, Ari, de Haan, Tijmen, Dobbs, Matt, Essinger-Hileman, Tom, Filippini, Jeffrey P., Ganga, Ken, Gudmundsson, Jon E., Halverson, Nils W., Hanany, Shaul, Henderson, Shawn W., Hill, Charles A., Ho, Shuay-Pwu P., Hubmayr, Johannes, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Kernasovskiy, Sarah A., Kovac, John M., Kusaka, Akito, Lee, Adrian T., Maria, Salatino, Mauskopf, Philip, McMahon, Jeff J., Moncelsi, Lorenzo, Nadolski, Andrew W., Nagy, Johanna M., Niemack, Michael D., O'Brient, Roger C., Padin, Stephen, Parshley, Stephen C., Pryke, Clement, Roe, Natalie A., Rostem, Karwan, Ruhl, John, Simon, Sara M., Staggs, Suzanne T., Suzuki, Aritoki, Switzer, Eric R., Tajima, Osamu, Thompson, Keith L., Timbie, Peter, Tucker, Gregory S., Vieira, Joaquin D., Vieregg, Abigail G., Westbrook, Benjamin, Wollack, Edward J., Yoon, Ki Won, Young, Karl S., Young, Edward Y., AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CMB-S4, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
detector: technology, Astrophysics::Instrumentation and Methods for Astrophysics, electronics: readout, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), optics, detector: design, activity report
Abstract

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible from the ground. The science goals and capabilities of CMB-S4 in illuminating cosmic inflation, measuring the sum of neutrino masses, searching for relativistic relics in the early universe, characterizing dark energy and dark matter, and mapping the matter distribution in the universe have been described in the CMB-S4 Science Book. This Technology Book is a companion volume to the Science Book. The ambitious science goals of CMB-S4, a "Stage-4" experiment, require a step forward in experimental capability from the current Stage=II experiments. To guide this process, we summarize the current state of CMB instrumentation technology, and identify R&D efforts necessary to advance it for use in CMB-S4. The book focuses on technical challenges in four broad areas: Telescope Design; Receiver Optics; Focal-Plane Optical Coupling; and Focal-Plane Sensor and Readout., 191 pages

Published
2019

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