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.

引用

页数：8

共 35 条

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