Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future

被引:14
|
作者
Chaubal, P. S. [1 ]
Reichardt, C. L. [1 ]
Gupta, N. [1 ,2 ]
Ansarinejad, B. [1 ]
Aylor, K. [3 ]
Balkenhol, L. [1 ]
Baxter, E. J. [4 ,5 ,6 ]
Bianchini, F. [7 ]
Benson, B. A. [5 ,6 ,8 ]
Bleem, L. E. [5 ,9 ]
Bocquet, S. [10 ]
Carlstrom, J. E. [5 ,6 ,9 ,11 ,12 ]
Chang, C. L. [5 ,6 ,9 ]
Crawford, T. M. [5 ,6 ]
Crites, A. T. [5 ,6 ,13 ]
de Haan, T. [14 ,15 ,16 ]
Dobbs, M. A. [14 ,15 ,17 ]
Everett, W. B. [18 ]
Floyd, B. [19 ]
George, E. M. [16 ,20 ]
Halverson, N. W. [18 ,21 ]
Holzapfel, W. L. [16 ]
Hrubes, J. D. [22 ]
Knox, L. [3 ]
Lee, A. T. [16 ,23 ]
Luong-Van, D. [22 ]
McMahon, J. J. [24 ]
Meyer, S. S. [5 ,6 ,11 ,12 ]
Mocanu, L. M. [5 ,6 ]
Mohr, J. J. [10 ,25 ,26 ]
Natoli, T. [5 ,11 ,27 ]
Padin, S. [5 ,6 ]
Pryke, C. [28 ]
Ruhl, J. E. [29 ]
Ruppin, F. [30 ]
Salvati, L. [31 ,32 ,33 ]
Saro, A. [31 ,32 ,34 ,35 ]
Schaffer, K. K. [5 ,12 ,36 ]
Shirokoff, E. [5 ,6 ,16 ]
Staniszewski, Z. [29 ,37 ]
Stark, A. A. [38 ]
Vieira, J. D. [39 ,40 ]
Williamson, R. [5 ,6 ]
机构
[1] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia
[2] CSIRO Astron & Space Sci, POB 1130, Bentley, WA 6102, Australia
[3] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[4] Univ Penn, Ctr Particle Cosmol, Dept Phys & Astron, Philadelphia, PA 19104 USA
[5] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[6] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[7] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[8] Fermilab Natl Accelerator Lab, MS209,POB 500, Batavia, IL 60510 USA
[9] Argonne Natl Lab, High Energy Phys Div, Argonne, IL 60439 USA
[10] Ludwig Maximilians Univ Munchen, Fac Phys, D-81679 Munich, Germany
[11] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[12] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[13] CALTECH, Pasadena, CA 91125 USA
[14] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[15] McGill Univ, McGill Space Inst, Montreal, PQ H3A 2T8, Canada
[16] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[17] Canadian Inst Adv Res, CIFAR Program Cosmol & Grav, Toronto, ON M5G 1Z8, Canada
[18] Univ Colorado, Ctr Astrophys & Space Astron, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA
[19] Univ Missouri, Dept Phys & Astron, 5110 Rockhill Rd, Kansas City, MO 64110 USA
[20] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[21] Univ Colorado, Dept Phys, Boulder, CO 80309 USA
[22] Univ Chicago, Chicago, IL 60637 USA
[23] Lawrence Berkeley Natl Lab, Phys Div, Berkeley, CA 94720 USA
[24] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[25] Excellence Cluster Universe, D-85748 Garching, Germany
[26] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[27] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[28] Univ Minnesota, Dept Phys, Minneapolis, MN 55455 USA
[29] Case Western Reserve Univ, Ctr Educ & Res Cosmol & Astrophys, Phys Dept, Cleveland, OH 44106 USA
[30] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[31] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy
[32] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34014 Trieste, Italy
[33] Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France
[34] Univ Trieste, Dept Phys, Astron Unit, Via Tiepolo 11, I-3413 Trieste, Italy
[35] INFN Sez Trieste, Trieste, Italy
[36] Sch Art Inst Chicago, Liberal Arts Dept, Chicago, IL 60603 USA
[37] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[38] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[39] Univ Illinois, Astron Dept, 1002 W Green St, Urbana, IL 61801 USA
[40] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA
来源
ASTROPHYSICAL JOURNAL | 2022年 / 931卷 / 02期
基金
澳大利亚研究理事会; 美国国家科学基金会;
关键词
MASS CALIBRATION; EFFICIENT; PARAMETERS; INFERENCE;
D O I
10.3847/1538-4357/ac6a55
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show the improvement to cosmological constraints from galaxy cluster surveys with the addition of cosmic microwave background (CMB)-cluster lensing data. We explore the cosmological implications of adding mass information from the 3.1 sigma detection of gravitational lensing of the CMB by galaxy clusters to the Sunyaev-Zel'dovich (SZ) selected galaxy cluster sample from the 2500 deg(2) SPT-SZ survey and targeted optical and X-ray follow-up data. In the ACDM model, the combination of the cluster sample with the Planck power spectrum measurements prefers sigma(8) (Omega(m)/0.3)(0.5) = 0.831 +/- 0.020. Adding the cluster data reduces the uncertainty on this quantity by a factor of 1.4, which is unchanged whether the 3.1 sigma CMB-cluster lensing measurement is included or not. We then forecast the impact of CMB-cluster lensing measurements with future cluster catalogs. Adding CMB-cluster lensing measurements to the SZ cluster catalog of the ongoing SPT-3G survey is expected to improve the expected constraint on the dark energy equation of state w by a factor of 1.3 to sigma(w) = 0.19. We find the largest improvements from CMB-cluster lensing measurements to be for sigma(8), where adding CMB-cluster lensing data to the cluster number counts reduces the expected uncertainty on sigma(8) by respective factors of 2.4 and 3.6 for SPT-3G and CMB-S4.
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页数:8
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