Dr. Amanda S. Bergman Profile

Dr. Amanda S. Bergman

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Publications (2)

SPIE Journal Paper | 27 December 2024

In-flight performance of Spider’s 280-GHz receivers

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

JATIS, Vol. 10, Issue 04, 044012, (December 2024) https://doi.org/10.1117/12.10.1117/1.JATIS.10.4.044012

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Proceedings Article | 16 August 2024 Presentation + Paper

In-flight performance of SPIDER's 280 GHz receivers

E. Shaw, P. A. Ade, S. Akers, M. Amiri, J. Austermann, J. Beall, D. Becker, S. Benton, A. Bergman, J. Bock, J. Bond, S. Bryan, H. Chiang, C. Contaldi, R. Domagalski, O. Doré, S. Duff, A. Duivenvoorden, H. Ericksen, M. Farhang, J. Filippini, L. Fissel, A. Fraisse, K. Freese, M. Galloway, A. Gambrel, N. Gandilo, K. Ganga, S. Gibbs, S. Gourapura, A. Grigorian, R. Gualtieri, J. Gudmundsson, M. Halpern, J. Hartley, M. Hasselfield, G. Hilton, W. Holmes, V. Hristov, Z. Huang, J. Hubmayr, K. Irwin, W. Jones, A. Kahn, Z. Kermish, C. King, C. Kuo, A. Lennox, J. S.-Y. Leung, S. Li, T. Luu, P. Mason, J. May, K. Megerian, L. Moncelsi, T. Morford, J. Nagy, R. Nie, C. Netterfield, M. Nolta, B. Osherson, I. Padilla, A. Rahlin, S. Redmond, C. Reintsema, L. Romualdez, J. Ruhl, M. Runyan, J. Shariff, C. Shiu, J. Soler, X. Song, S. Tartakovsky, H. Thommesen, A. Trangsrud, C. Tucker, R. Tucker, A. Turner, J. Ullom, J. van der List, J. Van Lanen, M. Vissers, A. Weber, S. Wen, I. Wehus, D. Wiebe, E. Young

Proceedings Volume 13102, 1310204 (2024) https://doi.org/10.1117/12.3016837

KEYWORDS: Cosmic microwave background, Cosmology, Superconducting detectors, Sensors, Receivers, Optical filters, Physics, Calibration

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