CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam

S. K. Choi; C. J. Duell; J. Austermann; N. F. Cothard; J. Gao; R. G. Freundt; C. Groppi; T. Herter; J. Hubmayr; Z. B. Huber; B. Keller; Y. Li; P. Mauskopf; M. D. Niemack; T. Nikola; K. Rossi; A. Sinclair; G. J. Stacey; E. M. Vavagiakis; M. Vissers; C. Tucker; E. Weeks; J. Wheeler

doi:10.1007/s10909-022-02787-9

CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam

S. K. Choi, C. J. Duell, J. Austermann, N. F. Cothard, J. Gao, R. G. Freundt, C. Groppi, T. Herter, J. Hubmayr, Z. B. Huber, B. Keller, Y. Li, P. Mauskopf, M. D. Niemack, T. Nikola, K. Rossi, A. Sinclair, G. J. Stacey, E. M. Vavagiakis, M. VissersC. Tucker, E. Weeks, J. Wheeler

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

Abstract

The Prime-Cam receiver on the Fred Young Submillimeter Telescope for the CCAT-prime project aims to address important astrophysical and cosmological questions with sensitive broadband, polarimetric, and spectroscopic measurements. The primary frequency bands in development include 280, 350, and 850 GHz for the polarization-sensitive broadband channels and 210–420 GHz for the spectrometers. Microwave kinetic inductance detectors (MKIDs) are a natural choice of detector technology for the simplicity in multiplexed readout needed for large format arrays at these high frequencies. We present here the initial laboratory characterization of the feedhorn-coupled 280 GHz polarimetric MKID array and outline the plans for the subsequent MKID arrays and the development of the testbed to characterize them.

Original language	English (US)
Pages (from-to)	849-856
Number of pages	8
Journal	Journal of Low Temperature Physics
Volume	209
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-022-02787-9
State	Published - Dec 2022

Keywords

CCAT-prime
Cosmic microwave background
Epoch of reionization
FYST
Kinetic inductance detector
Prime-Cam

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
General Materials Science
Condensed Matter Physics

Access to Document

10.1007/s10909-022-02787-9

Cite this

Choi, S. K., Duell, C. J., Austermann, J., Cothard, N. F., Gao, J., Freundt, R. G., Groppi, C., Herter, T., Hubmayr, J., Huber, Z. B., Keller, B., Li, Y., Mauskopf, P., Niemack, M. D., Nikola, T., Rossi, K., Sinclair, A., Stacey, G. J., Vavagiakis, E. M., ... Wheeler, J. (2022). CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam. Journal of Low Temperature Physics, 209(5-6), 849-856. https://doi.org/10.1007/s10909-022-02787-9

Choi, SK, Duell, CJ, Austermann, J, Cothard, NF, Gao, J, Freundt, RG, Groppi, C, Herter, T, Hubmayr, J, Huber, ZB, Keller, B, Li, Y, Mauskopf, P, Niemack, MD, Nikola, T, Rossi, K, Sinclair, A, Stacey, GJ, Vavagiakis, EM, Vissers, M, Tucker, C, Weeks, E & Wheeler, J 2022, 'CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam', Journal of Low Temperature Physics, vol. 209, no. 5-6, pp. 849-856. https://doi.org/10.1007/s10909-022-02787-9

@article{7eec7eaa8b0142949e4be8cd75791b6a,

title = "CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam",

abstract = "The Prime-Cam receiver on the Fred Young Submillimeter Telescope for the CCAT-prime project aims to address important astrophysical and cosmological questions with sensitive broadband, polarimetric, and spectroscopic measurements. The primary frequency bands in development include 280, 350, and 850 GHz for the polarization-sensitive broadband channels and 210–420 GHz for the spectrometers. Microwave kinetic inductance detectors (MKIDs) are a natural choice of detector technology for the simplicity in multiplexed readout needed for large format arrays at these high frequencies. We present here the initial laboratory characterization of the feedhorn-coupled 280 GHz polarimetric MKID array and outline the plans for the subsequent MKID arrays and the development of the testbed to characterize them.",

keywords = "CCAT-prime, Cosmic microwave background, Epoch of reionization, FYST, Kinetic inductance detector, Prime-Cam",

author = "Choi, {S. K.} and Duell, {C. J.} and J. Austermann and Cothard, {N. F.} and J. Gao and Freundt, {R. G.} and C. Groppi and T. Herter and J. Hubmayr and Huber, {Z. B.} and B. Keller and Y. Li and P. Mauskopf and Niemack, {M. D.} and T. Nikola and K. Rossi and A. Sinclair and Stacey, {G. J.} and Vavagiakis, {E. M.} and M. Vissers and C. Tucker and E. Weeks and J. Wheeler",

note = "Publisher Copyright: {\textcopyright} 2022, The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature.",

year = "2022",

month = dec,

doi = "10.1007/s10909-022-02787-9",

language = "English (US)",

volume = "209",

pages = "849--856",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "5-6",

}

TY - JOUR

T1 - CCAT-Prime

T2 - Characterization of the First 280 GHz MKID Array for Prime-Cam

AU - Choi, S. K.

AU - Duell, C. J.

AU - Austermann, J.

AU - Cothard, N. F.

AU - Gao, J.

AU - Freundt, R. G.

AU - Groppi, C.

AU - Herter, T.

AU - Hubmayr, J.

AU - Huber, Z. B.

AU - Keller, B.

AU - Li, Y.

AU - Mauskopf, P.

AU - Niemack, M. D.

AU - Nikola, T.

AU - Rossi, K.

AU - Sinclair, A.

AU - Stacey, G. J.

AU - Vavagiakis, E. M.

AU - Vissers, M.

AU - Tucker, C.

AU - Weeks, E.

AU - Wheeler, J.

PY - 2022/12

Y1 - 2022/12

N2 - The Prime-Cam receiver on the Fred Young Submillimeter Telescope for the CCAT-prime project aims to address important astrophysical and cosmological questions with sensitive broadband, polarimetric, and spectroscopic measurements. The primary frequency bands in development include 280, 350, and 850 GHz for the polarization-sensitive broadband channels and 210–420 GHz for the spectrometers. Microwave kinetic inductance detectors (MKIDs) are a natural choice of detector technology for the simplicity in multiplexed readout needed for large format arrays at these high frequencies. We present here the initial laboratory characterization of the feedhorn-coupled 280 GHz polarimetric MKID array and outline the plans for the subsequent MKID arrays and the development of the testbed to characterize them.

AB - The Prime-Cam receiver on the Fred Young Submillimeter Telescope for the CCAT-prime project aims to address important astrophysical and cosmological questions with sensitive broadband, polarimetric, and spectroscopic measurements. The primary frequency bands in development include 280, 350, and 850 GHz for the polarization-sensitive broadband channels and 210–420 GHz for the spectrometers. Microwave kinetic inductance detectors (MKIDs) are a natural choice of detector technology for the simplicity in multiplexed readout needed for large format arrays at these high frequencies. We present here the initial laboratory characterization of the feedhorn-coupled 280 GHz polarimetric MKID array and outline the plans for the subsequent MKID arrays and the development of the testbed to characterize them.

KW - CCAT-prime

KW - Cosmic microwave background

KW - Epoch of reionization

KW - FYST

KW - Kinetic inductance detector

KW - Prime-Cam

UR - http://www.scopus.com/inward/record.url?scp=85136998498&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85136998498&partnerID=8YFLogxK

U2 - 10.1007/s10909-022-02787-9

DO - 10.1007/s10909-022-02787-9

M3 - Article

AN - SCOPUS:85136998498

SN - 0022-2291

VL - 209

SP - 849

EP - 856

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 5-6

ER -

CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this