Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Michael Crumrine"'
Autor:
James Cornelison, Clara Verges, P A. Ade, Zeeshan Ahmed, Mandana Amiri, Denis Barkats, Ritoban Basu Thakur, Dominic Beck, Colin A. Bischoff, James J. Bock, Victor Buza, James R. Cheshire, Jake Connors, Michael Crumrine, Ari Jozef Cukierman, Edward Denison, Marion Dierickx, Lionel Duband, Miranda Eiben, Sofia Fatigoni, Jeff P. Filippini, Christos Giannakopoulos, Neil Goeckner-Wald, David C. Goldfinger, James A. Grayson, Paul Grimes, Grantland Hall, George Halal, Mark Halpern, Emma Hand, Sam A. Harrison, Shawn Henderson, Sergi Hildebrandt, Gene C. Hilton, Johannes Hubmayr, Howard Hui, Kent D. Irwin, Jae Hwan Kang, Kirit S. Karkare, Sinan Kefeli, John Kovac, Chao-Lin Kuo, King Lau, Erik M. Leitch, Amber Lennox, Tongtian Liu, Karsten Look, K(oko). G. Megerian, Lorenzo Minutolo, Lorenzo Moncelsi, Yuka Nakato, Toshiya Namikawa, H. T. Nguyen, Roger O'brient, Steven Palladino, Matthew Petroff, Thomas Prouve, Clement Pryke, Benjamin Racine, Carl D. Reintsema, Maria Salatino, Alessandro Schillaci, Benjamin Schmitt, Baibhav Singari, Ahmed Soliman, Tyler St Germaine, Bryan Steinbach, Rashmi Sudiwala, Keith L. Thompson, Calvin Tsai, Carole Tucker, Anthony D. Turner, Caterina Umiltà, Abigail G. Vieregg, Albert Wandui, Alexis C. Weber, Don Wiebe, Justin Willmert, Wai Ling K. Wu, Hung-I Yang, Ki Won Yoon, Edward Young, Cyndia Yu, Lingzhen Zeng, Cheng Zhang, Silvia Zhang
Publikováno v:
HAL
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2022
SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.121901X, ⟨10.1117/12.2620212⟩
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2022
SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.121901X, ⟨10.1117/12.2620212⟩
The BICEP3 Polarimeter is a small aperture, refracting telescope, dedicated to the observation of the Cosmic Microwave Background (CMB) at 95GHz. It is designed to target degree angular scale polarization patterns, in particular the very-much-sought-
Autor:
Jakob Vanzyl, Caterina Umiltà, Anthony D. Turner, Carole Tucker, James E. Tolan, Keith L. Thompson, Grant P. Teply, Rashmi Sudiwala, Bryan Steinbach, Zachary K. Staniszewski, Tyler St Germaine, Chris D. Sheehy, Grantland Hall, Lionel Duband, Marion Dierickx, Michael Crumrine, Brendan Crill, James Cornelison, Jake Connors, Victor Buza, Immanuel Buder, Justus A. Brevik, Rachel Bowens-Rubin, Denis Barkats, Kate D. Alexander, Randol Aikin, Zeeshan Ahmed, P. A. R. Ade, Cheng Zhang, Ki Won Yoon, Hung-I. Yang, Wai Ling K. Wu, Chin Lin Wong, Justin Willmert, Don Wiebe, Alexis C. Weber, Albert Wandui, Abigail G. Vieregg, Robert Schwarz, Alessandro Schillaci, Steffen Richter, Benjamin Racine, Clement Pryke, Stephen Palladino, R. Walt Ogburn IV, Roger O'brient, H. T. Nguyen, C. B. Netterfield, Toshiya Namikawa, Lorenzo Moncelsi, K(oko). G. Megerian, Martin Lueker, Erik M. Leitch, King Lau, Nicole Larson, Chao-Lin Kuo, J. M. Kovac, Sarah A. Kernasovskiy, Sinan Kefeli, Brian G. Keating, Jonathan Kaufman, Ethan Karpel, Kirit S. Karkare, Jae Hwan Kang, Kent D. Irwin, Howard Hui, Gene C. Hilton, Sergi Hildebrandt, Sam A. Harrison, Mark Halpern, James A. Grayson, Stefan Fliescher, Jeff P. Filippini, Cora Dvorkin, Eric Bullock, James J. Bock, Colin A. Bischoff, Steve J. Benton, Ahmed Soliman
BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f56e7e21bcc8d1224fa0e60110502426
http://arxiv.org/abs/1808.00571
http://arxiv.org/abs/1808.00571
Autor:
Jae Hwan Kang, Cheng Zhang, Ki Won Yoon, Hung-I Yang, Wai Ling K. Wu, Chin Lin Wong, Justin Willmert, Don Wiebe, Alexis C. Weber, Albert Wandui, Abigail G. Vieregg, Caterina Umiltà, Anthony D. Turner, Carole Tucker, James E. Tolan, Keith L. Thompson, Grant P. Teply, Rashmi Sudiwala, Bryan Steinbach, Zachary K. Staniszewski, Tyler St Germaine, Ahmed Soliman, Chris D. Sheehy, Robert Schwarz, Alessandro Schillaci, Steffen Richter, Benjamin Racine, Clement Pryke, Stephen Palladino, R. W. Ogburn IV, Roger O'brient, Hien T. Nguyen, C. B. Netterfield, Toshiya Namikawa, Lorenzo Moncelsi, Koko G. Megerian, Martin Lueker, Erik M. Leitch, King Lau, Nicole Larsen, Chao-Lin Kuo, John M. Kovac, Sarah A. Kernasovskiy, Sinan Kefeli, Brian G. Keating, Jonathan Kaufman, Ethan Karpel, Kirit S. Karkare, Kent D. Irwin, Howard Hui, Gene C. Hilton, Sergi Hildebrandt, Sam A. Harrison, Mark Halpern, Grantland Hall, James A. Grayson, Stefan Fliescher, Jeff P. Filippini, Cora Dvorkin, Lionel Duband, Marion Dierickx, Michael Crumrine, Brendan Crill, James Cornelison, Jake Conners, Victor Buza, Eric Bullock, Immanuel Buder, Justus A. Brevik, Rachel Bowens-Rubin, Hans Boenish, James J. Bock, Colin A. Bischoff, Steve J. Benton, Denis Barkats, Kate D. Alexander, Randol Aikin, Zeeshan Ahmed, Peter A. Ade
Publikováno v:
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2018
SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082N, ⟨10.1117/12.2313854⟩
SPIE Astronomical Telescopes + Instrumentation 2018
SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082N, ⟨10.1117/12.2313854⟩
BICEP3 is a 520mm aperture on-axis refracting telescope observing the polarization of the cosmic microwave background (CMB) at 95GHz in search of the B-mode signal originating from inflationary gravitational waves. BICEP3's focal plane is populated w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b68e136e8d2ddae20f20d865187d8e47
https://hal.archives-ouvertes.fr/hal-01851180
https://hal.archives-ouvertes.fr/hal-01851180
Publikováno v:
Day 2 Wed, March 07, 2018.
Abstract The authors have been contacted by many people in the industry lately that are incorrectly utilizing big data to produce correlations that attempt to identify operational "sweet spots". This paper will show examples and address the need to a
Autor:
Sumita Pennathur, Jesper Kristensen, Mathias Bækbo Andersen, Andrew Michael Crumrine, Henrik Bruus, Kristian Lund Jensen
Publikováno v:
Lund Jensen, K, Kristensen, J T, Crumrine, A M, Andersen, M B, Bruus, H & Pennathur, S 2011, ' Hydronium-dominated ion transport in carbon-dioxide-saturated electrolytes at low salt concentrations in nanochannels ', Physical Review E, vol. 83, no. 5, pp. artikle number 056307 . https://doi.org/10.1103/PhysRevE.83.056307
Nanochannel ion transport is known to be governed by surface charge at low ionic concentrations. In this paper, we show that this surface charge is typically dominated by hydronium ions arising from dissolution of ambient atmospheric carbon dioxide.
Publikováno v:
2011 IEEE 24th International Conference on Micro Electro Mechanical Systems.
We demonstrate a nanofluidic-based carbon dioxide sensor through corroboration with our nanochannel hydronium-dominated ion transport model. We verify the predictive power of our model by comparing calculated and measured conductances of solutions wi
Autor:
David C. Goldfinger, Peter A. R. Ade, Zeeshan Ahmed, Mandana Amiri, Denis Barkats, Ritoban Basu Thakur, Dominic Beck, Colin A. Bischoff, James J. Bock, Victor Buza, James R. Cheshire, Jake Connors, James Cornelison, Michael Crumrine, Ari J. Cukierman, Edward V. Denison, Marion I. Dierickx, Lionel Duband, Miranda Eiben, Sofia Fatigoni, Jeff P. Filippini, Christos Giannakopoulos, Neil Goeckner-Wald, James A. Grayson, Paul K. Grimes, Grantland Hall, George Halal, Mark Halpern, Emma Hand, Sam A. Harrison, Shawn Henderson, Sergi R. Hildebrandt, Gene C. Hilton, Johannes Hubmayr, Howard Hui, Kent D. Irwin, Jae Hwan Kang, Kirit S. Karkare, Sinan Kefeli, John M. Kovac, Chao-Lin Kuo, King Lau, Erik M. Leitch, Amber Lennox, Tongtian Liu, Krikor G. Megerian, Lorenzo Minutolo, Lorenzo Moncelsi, Yuka Nakato, Toshiya Namikawa, Hien T. Nguyen, Roger O'Brient, Steven M. Palladino, Matthew Petroff, Thomas Prouvé, Clement L. Pryke, Benjamin Racine, Carl D. Reintsema, Maria Salatino, Alessandro Schillaci, Benjamin L. Schmitt, Baibhav Singari, Ahmed Soliman, Amanda G. Smith, Tyler St. Germaine, Bryan Steinbach, Rashmi V. Sudiwala, Keith L. Thompson, Calvin Tsai, Carole E. Tucker, Anthony D. Turner, Caterina Umiltà, Clara Verges, Abigail G. Vieregg, Albert K. Wandui, Alexis C. Weber, Don V. Wiebe, Justin Willmert, Wai Ling K. Wu, Hung-I Yang, Ki Won Yoon, Edward Young, Cyndia Yu, Lingzhen Zeng, Cheng Zhang, Silvia Zhang
Publikováno v:
HAL
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2022
SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.121901V, ⟨10.1117/12.2629490⟩
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2022
SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.121901V, ⟨10.1117/12.2629490⟩
Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is therefore cr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd2db57b72bbc9f35b11b91e2bf7d313
https://hal.archives-ouvertes.fr/hal-03764973
https://hal.archives-ouvertes.fr/hal-03764973