Mr. Jared May Profile

Jared May

at Case Western Reserve Univ

SPIE Involvement:

Author

Publications (2)

SPIE Journal Paper | 27 December 2024

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

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

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

KEYWORDS: Sensors, Receivers, Tunable filters, Optical filters, Physics, Equipment, Sapphire, Calibration, Detector arrays, Quantum receivers

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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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