Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future
Abstract
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 factorsmore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- SPT Collaboration
- OSTI Identifier:
- 1871050
- Alternate Identifier(s):
- OSTI ID: 1839552; OSTI ID: 1923894; OSTI ID: 1960011
- Report Number(s):
- FERMILAB-PUB-21-729-PPD; arXiv:2111.07491
Journal ID: ISSN 0004-637X
- Grant/Contract Number:
- AC02- 06CH11357; AC02-07CH11359; AC02-05CH11231; AC02-06CH11357
- Resource Type:
- Published Article
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Name: The Astrophysical Journal Journal Volume: 931 Journal Issue: 2; Journal ID: ISSN 0004-637X
- Publisher:
- American Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; CMB; cluster lensing; cosmological parameters; cosmology:observations
Citation Formats
Chaubal, P. S., Reichardt, C. L., Gupta, N., Ansarinejad, B., Aylor, K., Balkenhol, L., Baxter, E. J., Bianchini, F., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Floyd, B., George, E. M., Halverson, N. W., Holzapfel, W. L., Hrubes, J. D., Knox, L., Lee, A. T., Luong-Van, D., McMahon, J. J., Meyer, S. S., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Pryke, C., Ruhl, J. E., Ruppin, F., Salvati, L., Saro, A., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Vieira, J. D., and Williamson, R. Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future. United States: N. p., 2022.
Web. doi:10.3847/1538-4357/ac6a55.
Chaubal, P. S., Reichardt, C. L., Gupta, N., Ansarinejad, B., Aylor, K., Balkenhol, L., Baxter, E. J., Bianchini, F., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Floyd, B., George, E. M., Halverson, N. W., Holzapfel, W. L., Hrubes, J. D., Knox, L., Lee, A. T., Luong-Van, D., McMahon, J. J., Meyer, S. S., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Pryke, C., Ruhl, J. E., Ruppin, F., Salvati, L., Saro, A., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Vieira, J. D., & Williamson, R. Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future. United States. https://doi.org/10.3847/1538-4357/ac6a55
Chaubal, P. S., Reichardt, C. L., Gupta, N., Ansarinejad, B., Aylor, K., Balkenhol, L., Baxter, E. J., Bianchini, F., Benson, B. A., Bleem, L. E., Bocquet, S., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., Floyd, B., George, E. M., Halverson, N. W., Holzapfel, W. L., Hrubes, J. D., Knox, L., Lee, A. T., Luong-Van, D., McMahon, J. J., Meyer, S. S., Mocanu, L. M., Mohr, J. J., Natoli, T., Padin, S., Pryke, C., Ruhl, J. E., Ruppin, F., Salvati, L., Saro, A., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Vieira, J. D., and Williamson, R. Fri .
"Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future". United States. https://doi.org/10.3847/1538-4357/ac6a55.
@article{osti_1871050,
title = {Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future},
author = {Chaubal, P. S. and Reichardt, C. L. and Gupta, N. and Ansarinejad, B. and Aylor, K. and Balkenhol, L. and Baxter, E. J. and Bianchini, F. and Benson, B. A. and Bleem, L. E. and Bocquet, S. and Carlstrom, J. E. and Chang, C. L. and Crawford, T. M. and Crites, A. T. and de Haan, T. and Dobbs, M. A. and Everett, W. B. and Floyd, B. and George, E. M. and Halverson, N. W. and Holzapfel, W. L. and Hrubes, J. D. and Knox, L. and Lee, A. T. and Luong-Van, D. and McMahon, J. J. and Meyer, S. S. and Mocanu, L. M. and Mohr, J. J. and Natoli, T. and Padin, S. and Pryke, C. and Ruhl, J. E. and Ruppin, F. and Salvati, L. and Saro, A. and Schaffer, K. K. and Shirokoff, E. and Staniszewski, Z. and Stark, A. A. and Vieira, J. D. and Williamson, R.},
abstractNote = {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.},
doi = {10.3847/1538-4357/ac6a55},
journal = {The Astrophysical Journal},
number = 2,
volume = 931,
place = {United States},
year = {Fri Jun 03 00:00:00 EDT 2022},
month = {Fri Jun 03 00:00:00 EDT 2022}
}
https://doi.org/10.3847/1538-4357/ac6a55
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