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In-Flight Performance of Spider's 280 GHz Receivers

Fuente: arXiv

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Autori principali:	Shaw, Elle C., Ade, P. A. R., Akers, S., Amiri, M., Austermann, J., Beall, J., Becker, D. T., Benton, S. J., Bergman, A. S., Bock, J. J., Bond, J. R., Bryan, S. A., Chiang, H. C., Contaldi, C. R., Domagalski, R. S., Doré, O., Duff, S. M., Duivenvoorden, A. J., Eriksen, H. K., Farhang, M., Filippini, J. P., Fissel, L. M., Fraisse, A. A., Freese, K., Galloway, M., Gambrel, A. E., Gandilo, N. N., Ganga, K., Gibbs, S. M., Gourapura, S., Grigorian, A., Gualtieri, R., Gudmundsson, J. E., Halpern, M., Hartley, J., Hasselfield, M., Hilton, G., Holmes, W., Hristov, V. V., Huang, Z., Hubmayr, J., Irwin, K. D., Jones, W. C., Kahn, A., Kermish, Z. D., King, C., Kuo, C. L., Lennox, A. R., Leung, J. S. -Y., Li, S., Luu, T. V., Mason, P. V., May, J., Megerian, K., Moncelsi, L., Morford, T. A., Nagy, J. M., Nie, R., Netterfield, C. B., Nolta, M., Osherson, B., Padilla, I. L., Rahlin, A. S., Redmond, S., Reintsema, C., Romualdez, L. J., Ruhl, J. E., Runyan, M. C., Shariff, J. A., Shiu, C., Soler, J. D., Song, X., Tartakovsky, S., Thommesen, H., Trangsrud, A., Tucker, C., Tucker, R. S., Turner, A. D., Ullom, J., van der List, J. F., Van Lanen, J., Vissers, M. R., Weber, A. C., Wehus, I. K., Wen, S., Wiebe, D. V., Young, E. Y.
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
Accesso online:	Acceder al recurso
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_version_	1866916903350435840
author	Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. Luu, T. V. Mason, P. V. May, J. Megerian, K. Moncelsi, L. Morford, T. A. Nagy, J. M. Nie, R. Netterfield, C. B. Nolta, M. Osherson, B. Padilla, I. L. Rahlin, A. S. Redmond, S. Reintsema, C. Romualdez, L. J. Ruhl, J. E. Runyan, M. C. Shariff, J. A. Shiu, C. Soler, J. D. Song, X. Tartakovsky, S. Thommesen, H. Trangsrud, A. Tucker, C. Tucker, R. S. Turner, A. D. Ullom, J. van der List, J. F. Van Lanen, J. Vissers, M. R. Weber, A. C. Wehus, I. K. Wen, S. Wiebe, D. V. Young, E. Y.
author_facet	Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. Luu, T. V. Mason, P. V. May, J. Megerian, K. Moncelsi, L. Morford, T. A. Nagy, J. M. Nie, R. Netterfield, C. B. Nolta, M. Osherson, B. Padilla, I. L. Rahlin, A. S. Redmond, S. Reintsema, C. Romualdez, L. J. Ruhl, J. E. Runyan, M. C. Shariff, J. A. Shiu, C. Soler, J. D. Song, X. Tartakovsky, S. Thommesen, H. Trangsrud, A. Tucker, C. Tucker, R. S. Turner, A. D. Ullom, J. van der List, J. F. Van Lanen, J. Vissers, M. R. Weber, A. C. Wehus, I. K. Wen, S. Wiebe, D. V. Young, E. Y.
contents	SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Balloon flights above the Antarctic continent. During its first flight in January 2015, SPIDER observed in the 95 GHz and 150 GHz frequency bands, setting constraints on the B-mode signature of primordial gravitational waves. Its second flight in the 2022-2023 season added new receivers at 280 GHz, each using an array of TESs coupled to the sky through feedhorns formed from stacks of silicon wafers. These receivers are optimized to produce deep maps of polarized Galactic dust emission over a large sky area, providing a unique data set with lasting value to the field. We describe the instrument's performance during SPIDER's second flight, focusing on the performance of the 280 GHz receivers. We include details on the flight, in-band optical loading at float, and an early analysis of detector noise.
format	Preprint
id	arxiv_https___arxiv_org_abs_2408_10444
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	In-Flight Performance of Spider's 280 GHz Receivers Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. Luu, T. V. Mason, P. V. May, J. Megerian, K. Moncelsi, L. Morford, T. A. Nagy, J. M. Nie, R. Netterfield, C. B. Nolta, M. Osherson, B. Padilla, I. L. Rahlin, A. S. Redmond, S. Reintsema, C. Romualdez, L. J. Ruhl, J. E. Runyan, M. C. Shariff, J. A. Shiu, C. Soler, J. D. Song, X. Tartakovsky, S. Thommesen, H. Trangsrud, A. Tucker, C. Tucker, R. S. Turner, A. D. Ullom, J. van der List, J. F. Van Lanen, J. Vissers, M. R. Weber, A. C. Wehus, I. K. Wen, S. Wiebe, D. V. Young, E. Y. Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Balloon flights above the Antarctic continent. During its first flight in January 2015, SPIDER observed in the 95 GHz and 150 GHz frequency bands, setting constraints on the B-mode signature of primordial gravitational waves. Its second flight in the 2022-2023 season added new receivers at 280 GHz, each using an array of TESs coupled to the sky through feedhorns formed from stacks of silicon wafers. These receivers are optimized to produce deep maps of polarized Galactic dust emission over a large sky area, providing a unique data set with lasting value to the field. We describe the instrument's performance during SPIDER's second flight, focusing on the performance of the 280 GHz receivers. We include details on the flight, in-band optical loading at float, and an early analysis of detector noise.
title	In-Flight Performance of Spider's 280 GHz Receivers
topic	Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2408.10444