Zobrazeno 1 - 7
of 7
pro vyhledávání: '"I. L. Padilla"'
Autor:
J. P. Filippini, A. E. Gambrel, A. S. Rahlin, E. Y. Young, P. A. R. Ade, M. Amiri, S. J. Benton, A. S. Bergman, R. Bihary, J. J. Bock, J. R. Bond, J. A. Bonetti, S. A. Bryan, H. C. Chiang, C. R. Contaldi, O. Doré, A. J. Duivenvoorden, H. K. Eriksen, M. Farhang, A. A. Fraisse, K. Freese, M. Galloway, N. N. Gandilo, K. Ganga, R. Gualtieri, J. E. Gudmundsson, M. Halpern, J. Hartley, M. Hasselfield, G. Hilton, W. Holmes, V. V. Hristov, Z. Huang, K. D. Irwin, W. C. Jones, A. Karakci, C. L. Kuo, Z. D. Kermish, J. S.- Y. Leung, S. Li, D. S. Y. Mak, P. V. Mason, K. Megerian, L. Moncelsi, T. A. Morford, J. M. Nagy, C. B. Netterfield, M. Nolta, R. O’Brient, B. Osherson, I. L. Padilla, B. Racine, C. Reintsema, J. E. Ruhl, M. C. Runyan, T. M. Ruud, J. A. Shariff, E. C. Shaw, C. Shiu, J. D. Soler, X. Song, A. Trangsrud, C. Tucker, R. S. Tucker, A. D. Turner, J. F. van der List, A. C. Weber, I. K. Wehus, S. Wen, D. V. Wiebe
Publikováno v:
19th International Workshop on Low Temperature Detectors
19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States
J.Low Temp.Phys.
19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States. pp.649-657, ⟨10.1007/s10909-022-02729-5⟩
19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States
J.Low Temp.Phys.
19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States. pp.649-657, ⟨10.1007/s10909-022-02729-5⟩
Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sensitive and non-intrusive method for monitoring variations in TES respon
Autor:
J. S.-Y. Leung, J. Hartley, J. M. Nagy, C. B. Netterfield, J. A. Shariff, P. A. R. Ade, M. Amiri, S. J. Benton, A. S. Bergman, R. Bihary, J. J. Bock, J. R. Bond, J. A. Bonetti, S. A. Bryan, H. C. Chiang, C. R. Contaldi, O. Doré, A. J. Duivenvoorden, H. K. Eriksen, M. Farhang, J. P. Filippini, A. A. Fraisse, K. Freese, M. Galloway, A. E. Gambrel, N. N. Gandilo, K. Ganga, R. Gualtieri, J. E. Gudmundsson, M. Halpern, M. Hasselfield, G. Hilton, W. Holmes, V. V. Hristov, Z. Huang, K. D. Irwin, W. C. Jones, A. Karakci, C. L. Kuo, Z. D. Kermish, S. Li, D. S. Y. Mak, P. V. Mason, K. Megerian, L. Moncelsi, T. A. Morford, M. Nolta, R. O’Brient, B. Osherson, I. L. Padilla, B. Racine, A. S. Rahlin, C. Reintsema, J. E. Ruhl, M. C. Runyan, T. M. Ruud, E. C. Shaw, C. Shiu, J. D. Soler, X. Song, A. Trangsrud, C. Tucker, R. S. Tucker, A. D. Turner, J. F. van der List, A. C. Weber, I. K. Wehus, S. Wen, D. V. Wiebe, E. Y. Young
Publikováno v:
Astrophys.J.
Astrophys.J., 2022, 928 (2), pp.109. ⟨10.3847/1538-4357/ac562f⟩
Astrophys.J., 2022, 928 (2), pp.109. ⟨10.3847/1538-4357/ac562f⟩
Modern CMB analysis pipelines regularly employ complex time-domain filters, beam models, masking, and other techniques during the production of sky maps and their corresponding angular power spectra. However, these processes can generate couplings be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::044746471f9fe9c9c6269fdbb0e53aeb
Autor:
Jeffrey P. Filippini, Ingunn Kathrine Wehus, P. A. R. Ade, Peter Mason, Zigmund Kermish, Carlo R. Contaldi, X. Song, M. Galloway, Aurelien A. Fraisse, K. Ganga, I. L. Padilla, J. F. van der List, J. R. Bond, A. E. Gambrel, D. V. Wiebe, Michael R. Vissers, L. M. Fissel, Joel N. Ullom, Adriaan J. Duivenvoorden, Dan Becker, A. D. Turner, S. Akers, Steven J. Benton, Matthew Hasselfield, R. Gualtieri, Marzieh Farhang, J. J. Bock, S. Li, A. Trangsrud, M. R. Nolta, E. Y. Young, A. S. Bergman, O. Doré, Shyang Wen, M. C. Runyan, J. E. Ruhl, Warren Holmes, J. A. Beall, Calvin B. Netterfield, C. Tucker, H. C. Chiang, Carl D. Reintsema, A. C. Weber, C. Shiu, R. S. Tucker, Mandana Amiri, R. S. Domagalski, Susan Redmond, Lorenzo Moncelsi, Kent D. Irwin, K. G. Megerian, J. Austermann, Antoine Kahn, Johannes Hubmayr, J. M. Nagy, Sean Bryan, J. Hartley, Arpi Grigorian, W. C. Jones, Jon E. Gudmundsson, Shannon M. Duff, Natalie N. Gandilo, L. J. Romualdez, Viktor Hristov, Mark Halpern, R. Nie, Katherine Freese, A. Lennox, Gene C. Hilton, H. Thommesen, B. Osherson, E. C. Shaw, J. S.-Y. Leung, Jamil A. Shariff, H. K. Eriksen, Zhi-Feng Huang, T. A. Morford, Juan D. Soler, L. M. Mocanu, C. L. Kuo, Alexandra S. Rahlin, J. Van Lanen
Publikováno v:
SPIE ASTRONOMICAL TELESCOPES + INSTRUMENTATION
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2020
SPIE Astronomical Telescopes + Instrumentation 2020, Dec 2020, Online, United States. pp.114532F, ⟨10.1117/12.2562941⟩
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2020
SPIE Astronomical Telescopes + Instrumentation 2020, Dec 2020, Online, United States. pp.114532F, ⟨10.1117/12.2562941⟩
In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature in the cosm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c62c979d3a32daecfa5bd67d9affc191
http://hdl.handle.net/10044/1/85438
http://hdl.handle.net/10044/1/85438
Autor:
Johanna Nagy, Steven J. Benton, W. A. Holmes, Carlo R. Contaldi, Gene C. Hilton, Jeffrey P. Filippini, D. V. Wiebe, Amy Trangsrud, A. S. Rahlin, J. E. Ruhl, Marcus Runyan, Calvin B. Netterfield, J. J. Bock, E. Young, E. C. Shaw, A. D. Turner, Carole Tucker, J. Fu, Sean Bryan, J. Hartley, O. Doré, H. C. Chiang, R. S. Tucker, Mandana Amiri, Kent D. Irwin, Natalie N. Gandilo, T. A. Morford, Carl D. Reintsema, Peter Mason, A. C. Weber, Jon E. Gudmundsson, A. E. Gambrel, Aurelien A. Fraisse, B. Osherson, R. Gualtieri, K. G. Megerian, W. C. Jones, Matthew Hasselfield, Jamil A. Shariff, Mark Halpern, Viktor Hristov, R. V. Gramillano, I. L. Padilla, Juan D. Soler, Peter A. R. Ade, Lorenzo Moncelsi, Zigmund Kermish, J. R. Bond
Publikováno v:
18th International Workshop on Low Temperature Detectors
18th International Workshop on Low Temperature Detectors, Jul 2019, Milano, Italy
J.Low Temp.Phys.
18th International Workshop on Low Temperature Detectors, Jul 2019, Milano, Italy. pp.1127-1136, ⟨10.1007/s10909-020-02415-4⟩
18th International Workshop on Low Temperature Detectors, Jul 2019, Milano, Italy
J.Low Temp.Phys.
18th International Workshop on Low Temperature Detectors, Jul 2019, Milano, Italy. pp.1127-1136, ⟨10.1007/s10909-020-02415-4⟩
Future mm-wave and sub-mm space missions will employ large arrays of multiplexed Transition Edge Sensor (TES) bolometers. Such instruments must contend with the high flux of cosmic rays beyond our atmosphere that induce "glitches" in bolometer data,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f6084f1735af870b69810c28f6ffae0
https://hal.archives-ouvertes.fr/hal-02497766
https://hal.archives-ouvertes.fr/hal-02497766
Autor:
Rolando Dünner, Joseph Eimer, Matthew Petroff, Lucas Parker, John Karakla, Kevin L. Denis, Tobias A. Marriage, Joseph Cleary, Dominik Gothe, Thomas Essinger-Hileman, Pedro Fluxá Rojas, Sumit Dahal, Karwan Rostem, Charles L. Bennett, Keisuke Osumi, Bastián Pradenas, David T. Chuss, Michael K. Brewer, Rahul Datta, Carolina Núñez, Manwei Chan, Edward J. Wollack, N. Miller, Rodrigo Reeves, Janet Weiland, Aamir Ali, I. L. Padilla, Jeffrey Iuliano, Duncan J. Watts, Ricardo Bustos, Zhilei Xu, Yunyang Li, Deniz Augusto Nunes Valle, J. W. Appel, Jullianna Couto, Kathleen Harrington
Publikováno v:
The Astrophysical Journal. 891:134
The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background (CMB) over 75% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220 GHz. CLASS measures
Autor:
Matthew Petroff, Joseph Eimer, Bingjie Wang, I. L. Padilla, Sumit Dahal, David T. Chuss, Tobias A. Marriage, Kathleen Harrington, Edward J. Wollack, Zhilei Xu, Charles L. Bennett, Thomas Essinger-Hileman, Lucas Parker, Duncan J. Watts, John W. Appel, Jeffrey Iuliano, Gary Hinshaw, Karwan Rostem, Nathan J. Miller, Aamir Ali
We analyze simulated maps of the Cosmology Large Angular Scale Surveyor (CLASS) experiment and recover a nearly cosmic-variance limited estimate of the reionization optical depth $\tau$. We use a power spectrum-based likelihood to simultaneously clea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::499a6c1ec0564e7af64fed2a5afc39a2
http://arxiv.org/abs/1801.01481
http://arxiv.org/abs/1801.01481
Design and characterization of the Cosmology Large Angular Scale Surveyor (CLASS) 93 GHz focal plane
Autor:
Johannes Hubmayr, Mark Halpern, Joseph Cleary, Kyle Helson, Thomas Essinger-Hileman, Aamir Ali, Janet Weiland, Lucas Parker, Nathan P Miller, Sumit Dahal, Carolina Núñez, Pedro Fluxa, John Karakla, Rolando Dünner, Qinan Wang, Kevin L. Denis, Joseph Eimer, Kathleen Harrington, Lingzhen Zeng, Duncan J. Watts, Felipe Colazo, Jeffery Iuliano, Manwei Chan, Deniz Augusto Nunes Valle, Kongpop U-Yen, Carl D. Reintsema, Jeff McMahon, Karwan Rostem, Gary Hinshaw, Edward J. Wollack, Tobias A. Marriage, Matthew Petroff, Charles L. Bennett, David T. Chuss, Bingjie Wang, J. W. Appel, Trevor Van Engelhoven, Ziang Yan, Michael K. Brewer, Bastián Pradenas, Ricardo Bustos, Rodrigo Reeves, Gene C. Hilton, Jullianna Couto, I. L. Padilla, Zhilei Xu, Marco Sagliocca, Gonzalo A. Palma
The Cosmology Large Angular Scale Surveyor (CLASS) aims to detect and characterize the primordial B-mode signal and make a sample-variance-limited measurement of the optical depth to reionization. CLASS is a ground-based, multi-frequency microwave po
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1327993009e0fe941ecd8b3986502d61