The Design and Integrated Performance of SPT-3G

被引:58
作者
Sobrin, J. A. [1 ,2 ]
Anderson, A. J. [2 ,3 ]
Bender, A. N. [2 ,4 ]
Benson, B. A. [2 ,3 ,5 ]
Dutcher, D. [1 ,2 ]
Foster, A. [6 ]
Goeckner-Wald, N. [7 ,8 ,10 ]
Montgomery, J. [9 ]
Nadolski, A. [11 ]
Rahlin, A. [2 ,3 ]
Ade, P. A. R. [12 ]
Ahmed, Z. [8 ,10 ,13 ]
Anderes, E. [14 ]
Archipley, M. [11 ,15 ]
Austermann, J. E. [16 ]
Avva, J. S. [17 ]
Aylor, K. [18 ]
Balkenhol, L. [19 ]
Barry, P. S. [2 ,4 ]
Thakur, R. Basu [2 ,20 ]
Benabed, K. [21 ,22 ]
Bianchini, F. [7 ,8 ,10 ,19 ]
Bleem, L. E. [2 ,4 ]
Bouchet, F. R. [21 ,22 ]
Bryant, L. [23 ]
Byrum, K. [4 ]
Carlstrom, J. E. [1 ,2 ,4 ,5 ,23 ]
Carter, F. W. [2 ,4 ]
Cecil, T. W. [4 ]
Chang, C. L. [2 ,4 ,5 ]
Chaubal, P. [19 ]
Chen, G. [24 ]
Cho, H-M [13 ]
Chou, T-L [1 ,2 ]
Cliche, J-F [9 ]
Crawford, T. M. [2 ,5 ]
Cukierman, A. [7 ,8 ,10 ,13 ]
Daley, C. [11 ]
de Haan, T. [25 ]
Denison, E., V [16 ]
Dibert, K. [2 ,5 ]
Ding, J. [26 ]
Dobbs, M. A. [9 ,27 ]
Everett, W. [28 ]
Feng, C. [29 ]
Ferguson, K. R. [30 ]
Fu, J. [11 ]
Galli, S. [21 ,22 ]
Gambrel, A. E. [2 ]
Gardner, R. W. [23 ]
机构
[1] Univ Chicago, Dept Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA
[2] Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA
[3] Fermilab Natl Accelerator Lab, MS209,POB 500, Batavia, MS 60510 USA
[4] Argonne Natl Lab, High Energy Phys Div, 9700 South Cass Ave, Argonne, IL 60439 USA
[5] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA
[6] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA
[7] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[8] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
[9] McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada
[10] McGill Univ, McGill Space Inst, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada
[11] Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA
[12] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3YB, Wales
[13] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[14] Univ Calif Davis, Dept Stat, One Shields Ave, Davis, CA 95616 USA
[15] Natl Ctr Supercomp Applicat, Ctr AstroPhys Surveys, Urbana, IL 61801 USA
[16] NIST, Quantum Devices Grp, 325 Broadway Mailcode 817-03, Boulder, CO 80305 USA
[17] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[18] Univ Calif Davis, Dept Phys & Astron, One Shields Ave, Davis, CA 95616 USA
[19] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia
[20] CALTECH, 1200 East Calif Blvd, Pasadena, CA 91125 USA
[21] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France
[22] Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France
[23] Univ Chicago, Enrico Fermi Inst, 5640 South Ellis Ave, Chicago, IL 60637 USA
[24] Univ Chicago, 5640 South Ellis Ave, Chicago, IL 60637 USA
[25] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan
[26] Argonne Natl Lab, Mat Sci Div, 9700 South Cass Ave, Argonne, IL 60439 USA
[27] Canadian Inst Adv Res, CIFAR Program Grav & Extreme Universe, Toronto, ON M5G 1Z8, Canada
[28] Univ Colorado, Dept Astrophys & Planetary Sci, CASA, Boulder, CO 80309 USA
[29] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA
[30] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[31] Univ Colorado, Dept Phys, Boulder, CO 80309 USA
[32] Lawrence Berkeley Natl Lab, Phys Div, Berkeley, CA 94720 USA
[33] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA
[34] Three Speed Log Inc, Victoria, BC V8S 3Z5, Canada
[35] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[36] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[37] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[38] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
基金
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
ATACAMA COSMOLOGY TELESCOPE; POINT SOURCES; 500 DEG(2); POLARIZATION; CONSTRAINTS; TEMPERATURE; CATALOG; CMB;
D O I
10.3847/1538-4365/ac374f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
SPT-3G is the third survey receiver operating on the South Pole Telescope dedicated to high-resolution observations of the cosmic microwave background (CMB). Sensitive measurements of the temperature and polarization anisotropies of the CMB provide a powerful data set for constraining cosmology. Additionally, CMB surveys with arcminute-scale resolution are capable of detecting galaxy clusters, millimeter-wave bright galaxies, and a variety of transient phenomena. The SPT-3G instrument provides a significant improvement in mapping speed over its predecessors, SPT-SZ and SPTpol. The broadband optics design of the instrument achieves a 430 mm diameter image plane across observing bands of 95, 150, and 220 GHz, with 1.2 ' FWHM beam response at 150 GHz. In the receiver, this image plane is populated with 2690 dual-polarization, trichroic pixels (similar to 16,000 detectors) read out using a 68x digital frequency-domain multiplexing readout system. In 2018, SPT-3G began a multiyear survey of 1500 deg(2) of the southern sky. We summarize the unique optical, cryogenic, detector, and readout technologies employed in SPT-3G, and we report on the integrated performance of the instrument.
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页数:19
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