Characterization of MKIDs for CMB Observation at 220 GHz With the South Pole Telescope-Reference-Cited by-同舟云学术

Characterization of MKIDs for CMB Observation at 220 GHz With the South Pole Telescope

Published:2023-08 Issue:5 Volume:33 Page:1-5
ISSN:1051-8223
Container-title:IEEE Transactions on Applied Superconductivity
language:
Short-container-title:IEEE Trans. Appl. Supercond.

Author:

Dibert K. R.¹^ORCID,Barry P. S.²,Anderson A. J.¹,Benson B. A.¹,Cecil T.³^ORCID,Chang C. L.¹,Fichman K. N.¹,Karkare K.¹,Li J.³^ORCID,Natoli T.¹,Pan Z.³^ORCID,Rouble M.⁴^ORCID,Shirokoff E.¹,Young M.⁵

Affiliation:

1. Department of Astronomy & Astrophysics, U. Chicago, Chicago, IL, USA

2. School of Physics, Astronomy, Cardiff University, Cardiff, U.K.

3. Argonne National Laboratory, Argonne, IL, USA

4. Department of Physics, McGill University, Montreal, Quebec, Canada

5. Kavli Institute for Cosmological Physics, U. Chicago, Chicago, IL, USA

Funder

DOE Graduate Instrumentation Research Award

National Science Foundation

Fermilab

Soft and Hybrid Nanotechnology Experimental

National Science Foundation's National Nanotechnology Coordinated Infrastructure

U.S. Department of Energy

Office of Science, Office of High Energy Physics

Publisher

Institute of Electrical and Electronics Engineers (IEEE)

Subject

Electrical and Electronic Engineering,Condensed Matter Physics,Electronic, Optical and Magnetic Materials

Link

https://ieeexplore.ieee.org/ielam/77/10024526/10056318-aam.pdf

Reference15 articles.

1. Photon-noise limited sensitivity in titanium nitride kinetic inductance detectors

2. Development of MKIDs for Measurement of the Cosmic Microwave Background with the South Pole Telescope

3. bicep2/KECK ARRAY. IV. OPTICAL CHARACTERIZATION AND PERFORMANCE OF THE bicep2 ANDKECK ARRAYEXPERIMENTS

4. SPT-3G+: mapping the high-frequency cosmic microwave background using kinetic inductance detectors