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pro vyhledávání: '"Young, Karl"'
Bayesian image restoration has had a long history of successful application but one of the limitations that has prevented more widespread use is that the methods are generally computationally intensive. The authors recently addressed this issue by de
Externí odkaz:
http://arxiv.org/abs/2306.00309
Bayesian image analysis has played a large role over the last 40+ years in solving problems in image noise-reduction, de-blurring, feature enhancement, and object detection. However, these problems can be complex and lead to computational difficultie
Externí odkaz:
http://arxiv.org/abs/2305.19481
Autor:
Wen, Qi, Fadeeva, Elena, Hanany, Shaul, Koch, Jürgen, Matsumura, Tomotake, Takaku, Ryota, Young, Karl
Publikováno v:
Optics & Laser Technology, Volume 142, October 2021, 107207
We use a 1030 nm laser with 7 ps pulse duration and average power up to 100 W to ablate pyramid-shape subwavelength structures (SWS) on alumina and sapphire. The SWS give an effective and cryogenically robust anti-reflection coating in the millimeter
Externí odkaz:
http://arxiv.org/abs/2103.06974
Akademický článek
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Autor:
Hanany, Shaul, Alvarez, Marcelo, Artis, Emmanuel, Ashton, Peter, Aumont, Jonathan, Aurlien, Ragnhild, Banerji, Ranajoy, Barreiro, R. Belen, Bartlett, James G., Basak, Soumen, Battaglia, Nick, Bock, Jamie, Boddy, Kimberly K., Bonato, Matteo, Borrill, Julian, Bouchet, François, Boulanger, François, Burkhart, Blakesley, Chluba, Jens, Chuss, David, Clark, Susan E., Cooperrider, Joelle, Crill, Brendan P., De Zotti, Gianfranco, Delabrouille, Jacques, Di Valentino, Eleonora, Didier, Joy, Doré, Olivier, Eriksen, Hans K., Errard, Josquin, Essinger-Hileman, Tom, Feeney, Stephen, Filippini, Jeffrey, Fissel, Laura, Flauger, Raphael, Fuskeland, Unni, Gluscevic, Vera, Gorski, Krzysztof M., Green, Dan, Hensley, Brandon, Herranz, Diego, Hill, J. Colin, Hivon, Eric, Hložek, Renée, Hubmayr, Johannes, Johnson, Bradley R., Jones, William, Jones, Terry, Knox, Lloyd, Kogut, Al, López-Caniego, Marcos, Lawrence, Charles, Lazarian, Alex, Li, Zack, Madhavacheril, Mathew, Melin, Jean-Baptiste, Meyers, Joel, Murray, Calum, Negrello, Mattia, Novak, Giles, O'Brient, Roger, Paine, Christopher, Pearson, Tim, Pogosian, Levon, Pryke, Clem, Puglisi, Giuseppe, Remazeilles, Mathieu, Rocha, Graca, Schmittfull, Marcel, Scott, Douglas, Shirron, Peter, Stephens, Ian, Sutin, Brian, Tomasi, Maurizio, Trangsrud, Amy, van Engelen, Alexander, Vansyngel, Flavien, Wehus, Ingunn K., Wen, Qi, Xu, Siyao, Young, Karl, Zonca, Andrea
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full-sky surveys of intensity and polarization with a final combined-ma
Externí odkaz:
http://arxiv.org/abs/1902.10541
Autor:
Sutin, Brian, Alvarez, Marcelo, Battaglia, Nicholas, Bock, Jamie, Bonato, Matteo, Borrill, Julian, Chuss, David T., Cooperrider, Joelle, Crill, Brendan, Delabrouille, Jacques, Devlin, Mark, Essinger-Hileman, Thomas, Fissel, Laura, Flauger, Raphael, Gorski, Krzysztof, Green, Daniel, Hanany, Shaul, Hubmayr, Johannes, Johnson, Bradley, Jones, William C., Knox, Lloyd, Kogut, Alan, Lawrence, Charles, McMahon, Jeff, Matsumura, Tomotake, Negrello, Mattia, O'Brient, Roger, Paine, Christopher, Pryke, Clement, Shirron, Peter, Trangsrud, Amy, Wen, Qi, Young, Karl, de Zotti, Gianfranco
The Probe of Inflation and Cosmic Origins (PICO) is a NASA-funded study of a Probe-class mission concept. The top-level science objectives are to probe the physics of the Big Bang by measuring or constraining the energy scale of inflation, probe fund
Externí odkaz:
http://arxiv.org/abs/1808.01368
Autor:
Young, Karl, Alvarez, Marcelo, Battaglia, Nicholas, Bock, Jamie, Borrill, Julian, Chuss, David, Crill, Brendan, Delabrouille, Jacques, Devlin, Mark, Fissel, Laura, Flauger, Raphael, Green, Daniel, Gorski, Kris, Hanany, Shaul, Hills, Richard, Hubmayr, Johannes, Johnson, Bradley, Jones, Bill, Knox, Lloyd, Kogut, Al, Lawrence, Charles, Matsumura, Tomotake, McGuire, Jim, McMahon, Jeff, O'Brient, Roger, Pryke, Clem, Sutin, Brian M., Tan, Xin Zhi, Trangsrud, Amy, Wen, Qi, de Zotti, Gianfranco
The Probe of Inflation and Cosmic Origins (PICO) is a probe-class mission concept currently under study by NASA. PICO will probe the physics of the Big Bang and the energy scale of inflation, constrain the sum of neutrino masses, measure the growth o
Externí odkaz:
http://arxiv.org/abs/1808.01369
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:
Aubin, François, Hanany, Shaul, Johnson, Bradley R., Lee, Adrian, Suzuki, Aritoki, Westbrook, Benjamin, Young, Karl
We present our work to develop and characterize low thermal conductance bolometers that are part of sinuous antenna multi-chroic pixels (SAMP). We use longer, thinner and meandered bolometer legs to achieve 9 pW/K thermal conductance bolometers. We a
Externí odkaz:
http://arxiv.org/abs/1802.03822