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Title: Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters

Abstract

Uncertainty in the mass-observable scaling relations is currently the limiting factor for galaxy cluster based cosmology. Weak gravitational lensing can provide a direct mass calibration and reduce the mass uncertainty. We present new ground-based weak lensing observations of 19 South Pole Telescope (SPT) selected clusters and combine them with previously reported space-based observations of 13 galaxy clusters to constrain the cluster mass scaling relations with the Sunyaev-Zel'dovich effect (SZE), the cluster gas mass $$M_\mathrm{gas}$$, and $$Y_\mathrm{X}$$, the product of $$M_\mathrm{gas}$$ and X-ray temperature. We extend a previously used framework for the analysis of scaling relations and cosmological constraints obtained from SPT-selected clusters to make use of weak lensing information. Here, we introduce a new approach to estimate the effective average redshift distribution of background galaxies and quantify a number of systematic errors affecting the weak lensing modelling. These errors include a calibration of the bias incurred by fitting a Navarro-Frenk-White profile to the reduced shear using $$N$$-body simulations. We blind the analysis to avoid confirmation bias. We are able to limit the systematic uncertainties to 6.4% in cluster mass (68% confidence). Our constraints on the mass-X-ray observable scaling relations parameters are consistent with those obtained by earlier studies, and our constraints for the mass-SZE scaling relation are consistent with the the simulation-based prior used in the most recent SPT-SZ cosmology analysis. We can now replace the external mass calibration priors used in previous SPT-SZ cosmology studies with a direct, internal calibration obtained on the same clusters.

Authors:
 [1];  [2];  [3];  [4]; ORCiD logo [5];  [1];  [6];  [7];  [8];  [9];  [2];  [10];  [8]; ORCiD logo [1];  [1];  [11];  [12];  [13];  [1];  [14] more »; ORCiD logo [15];  [16];  [8]; ORCiD logo [17];  [18]; ORCiD logo [17];  [19];  [20];  [21];  [1];  [22] « less
  1. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany
  2. Argonne National Laboratory, High-Energy Physics Division, 9700 S. Cass Avenue, Argonne, IL 60439, USA, Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA
  3. Argelander-Institut für Astronomie, Auf dem Hügel 71, D-53121 Bonn, Germany
  4. Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA
  5. Leiden Observatory, Leiden University, Niels Bohrweg 2, 2300 CA Leiden, the Netherlands
  6. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany, Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr., D-85748 Garching, Germany
  7. Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, USA, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
  8. Fermi National Accelerator Laboratory, Batavia, IL 60510-0500, USA
  9. Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA, Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110, USA, Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA
  10. Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA
  11. Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA, Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110, USA
  12. Department of Astronomy, University of Florida, Gainesville, FL 32611, USA
  13. Department of Physics, University of California, Berkeley, CA 94720, USA
  14. Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA
  15. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA, Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA
  16. Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
  17. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
  18. Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Science, University of Colorado, Boulder, CO 80309, USA, NASA Ames Research Center, Moffett Field, CA 94035, USA
  19. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany, INAF–Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
  20. LSST, 950 North Cherry Avenue, Tucson, AZ 85719, USA
  21. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
  22. Department of Physics, Harvard University, 17 Oxford Street, Cambridge, MA 02138, USA
Publication Date:
Research Org.:
Argonne National Lab. (ANL), Argonne, IL (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
SPT
OSTI Identifier:
1488616
Alternate Identifier(s):
OSTI ID: 1413679
Report Number(s):
arXiv:1711.05344; FERMILAB-PUB-17-557-AE
Journal ID: ISSN 0035-8711
Grant/Contract Number:  
AC02-06CH11357; AC02-07CH11359
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 483 Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United Kingdom
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; gravitational lensing: weak; galaxies: clusters: general; cosmology: observations

Citation Formats

Dietrich, J. P., Bocquet, S., Schrabback, T., Applegate, D., Hoekstra, H., Grandis, S., Mohr, J. J., Allen, S. W., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Capasso, R., Chiu, I., Crawford, T. M., Gonzalez, A. H., de Haan, T., Klein, M., von der Linden, A., Mantz, A. B., Marrone, D. P., McDonald, M., Raghunathan, S., Rapetti, D., Reichardt, C. L., Saro, A., Stalder, B., Stark, A., Stern, C., and Stubbs, C. Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters. United Kingdom: N. p., 2018. Web. doi:10.1093/mnras/sty3088.
Dietrich, J. P., Bocquet, S., Schrabback, T., Applegate, D., Hoekstra, H., Grandis, S., Mohr, J. J., Allen, S. W., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Capasso, R., Chiu, I., Crawford, T. M., Gonzalez, A. H., de Haan, T., Klein, M., von der Linden, A., Mantz, A. B., Marrone, D. P., McDonald, M., Raghunathan, S., Rapetti, D., Reichardt, C. L., Saro, A., Stalder, B., Stark, A., Stern, C., & Stubbs, C. Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters. United Kingdom. https://doi.org/10.1093/mnras/sty3088
Dietrich, J. P., Bocquet, S., Schrabback, T., Applegate, D., Hoekstra, H., Grandis, S., Mohr, J. J., Allen, S. W., Bayliss, M. B., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Capasso, R., Chiu, I., Crawford, T. M., Gonzalez, A. H., de Haan, T., Klein, M., von der Linden, A., Mantz, A. B., Marrone, D. P., McDonald, M., Raghunathan, S., Rapetti, D., Reichardt, C. L., Saro, A., Stalder, B., Stark, A., Stern, C., and Stubbs, C. Thu . "Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters". United Kingdom. https://doi.org/10.1093/mnras/sty3088.
@article{osti_1488616,
title = {Sunyaev–Zel’dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters},
author = {Dietrich, J. P. and Bocquet, S. and Schrabback, T. and Applegate, D. and Hoekstra, H. and Grandis, S. and Mohr, J. J. and Allen, S. W. and Bayliss, M. B. and Benson, B. A. and Bleem, L. E. and Brodwin, M. and Bulbul, E. and Capasso, R. and Chiu, I. and Crawford, T. M. and Gonzalez, A. H. and de Haan, T. and Klein, M. and von der Linden, A. and Mantz, A. B. and Marrone, D. P. and McDonald, M. and Raghunathan, S. and Rapetti, D. and Reichardt, C. L. and Saro, A. and Stalder, B. and Stark, A. and Stern, C. and Stubbs, C.},
abstractNote = {Uncertainty in the mass-observable scaling relations is currently the limiting factor for galaxy cluster based cosmology. Weak gravitational lensing can provide a direct mass calibration and reduce the mass uncertainty. We present new ground-based weak lensing observations of 19 South Pole Telescope (SPT) selected clusters and combine them with previously reported space-based observations of 13 galaxy clusters to constrain the cluster mass scaling relations with the Sunyaev-Zel'dovich effect (SZE), the cluster gas mass $M_\mathrm{gas}$, and $Y_\mathrm{X}$, the product of $M_\mathrm{gas}$ and X-ray temperature. We extend a previously used framework for the analysis of scaling relations and cosmological constraints obtained from SPT-selected clusters to make use of weak lensing information. Here, we introduce a new approach to estimate the effective average redshift distribution of background galaxies and quantify a number of systematic errors affecting the weak lensing modelling. These errors include a calibration of the bias incurred by fitting a Navarro-Frenk-White profile to the reduced shear using $N$-body simulations. We blind the analysis to avoid confirmation bias. We are able to limit the systematic uncertainties to 6.4% in cluster mass (68% confidence). Our constraints on the mass-X-ray observable scaling relations parameters are consistent with those obtained by earlier studies, and our constraints for the mass-SZE scaling relation are consistent with the the simulation-based prior used in the most recent SPT-SZ cosmology analysis. We can now replace the external mass calibration priors used in previous SPT-SZ cosmology studies with a direct, internal calibration obtained on the same clusters.},
doi = {10.1093/mnras/sty3088},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 483,
place = {United Kingdom},
year = {Thu Dec 20 00:00:00 EST 2018},
month = {Thu Dec 20 00:00:00 EST 2018}
}

Journal Article:
Free Publicly Available Full Text
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https://doi.org/10.1093/mnras/sty3088

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  • Hildebrandt, H.; Viola, M.; Heymans, C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 465, Issue 2
  • DOI: 10.1093/mnras/stw2805

Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA
journal, July 2013


JOINT ANALYSIS OF CLUSTER OBSERVATIONS. II. CHANDRA / XMM-NEWTON X-RAY AND WEAK LENSING SCALING RELATIONS FOR A SAMPLE OF 50 RICH CLUSTERS OF GALAXIES
journal, April 2013


Weighing the giants– V. Galaxy cluster scaling relations
journal, September 2016

  • Mantz, Adam B.; Allen, Steven W.; Morris, R. Glenn
  • Monthly Notices of the Royal Astronomical Society, Vol. 463, Issue 4
  • DOI: 10.1093/mnras/stw2250

LoCuSS: THE SUNYAEV–ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION
journal, July 2012


THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < z < 1.2 SELECTED FROM THE SPT-SZ SURVEY
journal, August 2013


Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data
journal, May 2017

  • Melchior, P.; Gruen, D.; McClintock, T.
  • Monthly Notices of the Royal Astronomical Society, Vol. 469, Issue 4
  • DOI: 10.1093/mnras/stx1053

Clash: the Concentration-Mass Relation of Galaxy Clusters
journal, June 2015


A Universal Density Profile from Hierarchical Clustering
journal, December 1997

  • Navarro, Julio F.; Frenk, Carlos S.; White, Simon D. M.
  • The Astrophysical Journal, Vol. 490, Issue 2
  • DOI: 10.1086/304888

LoCuSS: CALIBRATING MASS-OBSERVABLE SCALING RELATIONS FOR CLUSTER COSMOLOGY WITH SUBARU WEAK-LENSING OBSERVATIONS
journal, September 2010


Planck 2013 results. XVI. Cosmological parameters
journal, October 2014


A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3
journal, March 2011


Optical Spectroscopy and Velocity Dispersions of Galaxy Clusters from the Spt-Sz Survey
journal, August 2014


Sharpening the Precision of the Sunyaev-Zel'Dovich Power Spectrum
journal, August 2009


Galaxy Clusters Discovered with a Sunyaev-Zel'Dovich Effect Survey
journal, July 2009


Clash: Weak-Lensing Shear-And-Magnification Analysis of 20 Galaxy Clusters
journal, October 2014


Galaxy Clusters Selected with the Sunyaev-Zel'Dovich Effect from 2008 South pole Telescope Observations
journal, September 2010


CHANDRA CLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION
journal, February 2009


A SUNYAEV-ZEL'DOVICH-SELECTED SAMPLE OF THE MOST MASSIVE GALAXY CLUSTERS IN THE 2500 deg 2 SOUTH POLE TELESCOPE SURVEY
journal, August 2011


Works referencing / citing this record:

Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
journal, September 2019

  • Wu, Hao-Yi; Weinberg, David H.; Salcedo, Andrés N.
  • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2
  • DOI: 10.1093/mnras/stz2617

Dark Energy Survey Year 1 results: validation of weak lensing cluster member contamination estimates from P(z) decomposition
journal, August 2019

  • Varga, T. N.; DeRose, J.; Gruen, D.
  • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
  • DOI: 10.1093/mnras/stz2185

Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – I. The richness–mass relation
journal, March 2019

  • Capasso, R.; Mohr, J. J.; Saro, A.
  • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 2
  • DOI: 10.1093/mnras/stz931

Weak lensing measurements of the APEX-SZ galaxy cluster sample
journal, June 2019

  • Klein, Matthias; Israel, Holger; Nagarajan, Aarti
  • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 2
  • DOI: 10.1093/mnras/stz1491

Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey
journal, April 2019

  • Miyatake, Hironao; Battaglia, Nicholas; Hilton, Matt
  • The Astrophysical Journal, Vol. 875, Issue 1
  • DOI: 10.3847/1538-4357/ab0af0

The Aemulus Project. II. Emulating the Halo Mass Function
journal, February 2019

  • McClintock, Thomas; Rozo, Eduardo; Becker, Matthew R.
  • The Astrophysical Journal, Vol. 872, Issue 1
  • DOI: 10.3847/1538-4357/aaf568

The redshift evolution of X-ray and Sunyaev–Zel’dovich scaling relations in the fable simulations
journal, August 2019

  • Henden, Nicholas A.; Puchwein, Ewald; Sijacki, Debora
  • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
  • DOI: 10.1093/mnras/stz2301

Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning
journal, October 2019

  • Green, Sheridan B.; Ntampaka, Michelle; Nagai, Daisuke
  • The Astrophysical Journal, Vol. 884, Issue 1
  • DOI: 10.3847/1538-4357/ab426f

Dark Energy Survey Year 1 results: the effect of intracluster light on photometric redshifts for weak gravitational lensing
journal, July 2019

  • Gruen, D.; Zhang, Y.; Palmese, A.
  • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 3
  • DOI: 10.1093/mnras/stz2036