SPT-3G+: Mapping the High-Frequency Cosmic Microwave Background Using Kinetic Inductance Detectors

被引：4

作者：

Anderson, A. J. ^{[1
,2
,3
]}

Barry, P. ^{[4
]}

Bender, A. N. ^{[2
,3
,5
]}

Benson, B. A. ^{[1
,2
,3
]}

Bleem, L. E. ^{[2
,5
]}

Carlstrom, J. E. ^{[2
,3
,5
,6
,7
]}

Cecil, T. W. ^{[5
]}

Chang, C. L. ^{[2
,3
,5
]}

Crawford, T. M. ^{[2
,3
]}

Dibert, K. R. ^{[2
,3
]}

Dobbs, M. A. ^{[8
,9
,10
]}

Fichman, K. ^{[7
]}

Halverson, N. W. ^{[11
,12
]}

Holzapfel, W. L. ^{[13
]}

Hryciuk, A. ^{[7
]}

Karkare, K. S. ^{[2
,3
]}

Li, J. ^{[5
]}

Lisovenko, M. ^{[5
]}

Marrone, D. ^{[14
,15
]}

McMahon, J. ^{[2
,3
]}

Montgomery, J. ^{[8
,9
]}

Natoli, T. ^{[2
]}

Pan, Z. ^{[2
,5
]}

Raghunathan, S. ^{[16
]}

Reichardt, C. L. ^{[17
]}

Rouble, M. ^{[8
,9
]}

Shirokoff, E. ^{[2
,3
]}

Smecher, G. ^{[18
]}

Stark, A. A. ^{[19
]}

Vieira, J. D. ^{[16
,20
,21
]}

Young, M. R. ^{[1
,2
]}

机构：

[1] Fermilab Natl Accelerator Lab, MS209,POB 500, Batavia, IL 60510 USA

[2] Univ Chicago, Kayli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[3] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[4] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3YB, Wales

[5] Argonne Natl Lab, High Energy Phys Div, 9700 South Cass Ave, Lemont, IL 60439 USA

[6] Univ Chicago, Enrico Fermi Inst, 5640 South Ellis Ave, Chicago, IL 60637 USA

[7] Univ Chicago, Dept Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA

[8] McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada

[9] McGill Univ, McGill Space Inst, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada

[10] Canadian Inst Adv Res, CIFAR Program Grav & Extreme Universe, Toronto, ON M5G 1Z8, Canada

[11] Univ Colorado, Dept Astrophys & Planetary Sci, CASA, Boulder, CO 80309 USA

[12] Univ Colorado, Dept Phys, Boulder, CO 80309 USA

[13] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[14] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA

[15] Univ Arizona, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA

[16] Natl Ctr Supercomp Applicat, Ctr AstroPhys Surveys, Urbana, IL 61801 USA

[17] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia

[18] Three Speed Log Inc, Victoria, BC V8S 3Z5, Canada

[19] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[20] Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA

[21] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA

来源：

MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY XI | 2022年 / 12190卷

基金：

澳大利亚研究理事会; 美国国家科学基金会; 加拿大自然科学与工程研究理事会;

关键词：

cosmic microwave background; kinetic inductance detectors; South Pole Telescope; kinematic Suriyaev-Zel'dovich effect; CONSTRAINTS;

D O I：

10.1117/12.2629755

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the design and science goals of SPT-3G+, a new camera for the South Pole Telescope, which will consist of a dense array of 34 100 kinetic inductance detectors measuring the cosmic microwave background (CMB) at 220, 285 and 345 GHz. The SPT-3G+ dataset will enable new constraints on the process of reionization, including measurements of the patchy kinematic Sunyaev-Zeldovich effect and improved constraints on the optical depth due to reionization. At the same time, it will serve as a pathfinder for the detection of Rayleigh scattering, which could allow future CMB surveys to constrain cosmological parameters better than from the primary CMB alone. In addition, the combined, multi-band SPT-3G and SPT-3G+ survey data, will have several synergies that enhance the original SPT-3G survey, including: extending the redshift-reach of SZ cluster surveys to z > 2; understanding the relationship between magnetic fields and star formation in our Galaxy; improved characterization of the impact of dust on inflationary B-mode searches; and characterizing astrophysical transients at the boundary between mm and sub-mm wavelengths. Finally, the modular design of the SPT-3G+ camera allows it to serve as an on-sky demonstrator for new detector technologies employing microwave readout, such as the on-chip spectrometers that we expect to deploy during the SPT-3G+ survey. In this paper, we describe the science goals of the project and the key technology developments that enable its powerful yet compact design.

引用

页数：26

共 16 条

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