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Title: The SPTpol Extended Cluster Survey

Abstract

We describe the observations and resultant galaxy cluster catalog from the 2770 deg2 SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev–Zel'dovich (SZ) effect and confirmed with a combination of archival and targeted follow-up data, making particular use of data from the Dark Energy Survey (DES). With incomplete follow-up we have confirmed as clusters 244 of 266 candidates at a detection significance ξ ≥ 5 and an additional 204 systems at 4 < ξ < 5. The confirmed sample has a median mass of $${M}_{500c}\sim 4.4\times {10}^{14}\,{M}_{\odot }\,{h}_{70}^{-1}$$ and a median redshift of z = 0.49, and we have identified 44 strong gravitational lenses in the sample thus far. Radio data are used to characterize contamination to the SZ signal; the median contamination for confirmed clusters is predicted to be ~1% of the SZ signal at the ξ > 4 threshold, and <4% of clusters have a predicted contamination >10% of their measured SZ flux. We associate SZ-selected clusters, from both SPT-ECS and the SPT-SZ survey, with clusters from the DES redMaPPer sample, and we find an offset distribution between the SZ center and central galaxy in general agreement with previous work, though with a larger fraction of clusters with significant offsets. Adopting a fixed Planck-like cosmology, we measure the optical richness–SZ mass ($$\lambda -M$$) relation and find it to be 28% shallower than that from a weak-lensing analysis of the DES data—a difference significant at the 4σ level—with the relations intersecting at λ = 60. The SPT-ECS cluster sample will be particularly useful for studying the evolution of massive clusters and, in combination with DES lensing observations and the SPT-SZ cluster sample, will be an important component of future cosmological analyses.

Authors:
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Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); Gordon and Betty Moore Foundation; USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
Contributing Org.:
DES Collaboration
OSTI Identifier:
1608577
Alternate Identifier(s):
OSTI ID: 1597079; OSTI ID: 1633071; OSTI ID: 1661220; OSTI ID: 1737601
Report Number(s):
arXiv:1910.04121; FERMILAB-PUB-19-513-AE; DES-2019-0442
Journal ID: ISSN 1538-4365
Grant/Contract Number:  
AC02-06CH11357; AC02-76SF00515; AC02-05CH11231; PLR-1248097; PHY-0114422; GBMF-947; HST-GO-15307.001; AC02-07CH11359; AST-0956135; AST-1716965; CSSI-1835865; 716762; R165SBKTMA; 693024; 50-OR-1610; 50-OR-1803; DP150103208; AST-1814719
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal. Supplement Series (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal. Supplement Series (Online); Journal Volume: 247; Journal Issue: 1; Journal ID: ISSN 1538-4365
Publisher:
American Astronomical Society/IOP
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; clusters; cosmology; general { large-scale structure of universe, gravitational lensing; observations - galaxies; strong

Citation Formats

Bleem, L. E., Bocquet, S., Stalder, B., Gladders, M. D., Ade, P. A. R., Allen, S. W., Anderson, A. J., Annis, J., Ashby, M. L. N., Austermann, J. E., Avila, S., Avva, J. S., Bayliss, M., Beall, J. A., Bechtol, K., Bender, A. N., Benson, B. A., Bertin, E., Bianchini, F., Blake, C., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Carrasco Kind, M., Carretero, J., Chang, C. L., Chiang, H. C., Citron, R., Moran, C. Corbett, Costanzi, M., Crawford, T. M., Crites, A. T., da Costa, L. N., de Haan, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Eifler, T. F., Everett, W., Flaugher, B., Floyd, B., Frieman, J., Gallicchio, J., García-Bellido, J., George, E. M., Gerdes, D. W., Gilbert, A., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Halverson, N. W., Harrington, N., Henning, J. W., Heymans, C., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., James, D. J., Jeltema, T., Joudaki, S., Khullar, G., Klein, M., Knox, L., Kuropatkin, N., Lee, A. T., Li, D., Lidman, C., Lowitz, A., MacCrann, N., Mahler, G., Maia, M. A. G., Marshall, J. L., McDonald, M., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miquel, R., Mocanu, L. M., Mohr, J. J., Montgomery, J., Nadolski, A., Natoli, T., Nibarger, J. P., Noble, G., Novosad, V., Padin, S., Palmese, A., Parkinson, D., Patil, S., Paz-Chinchón, F., Plazas, A. A., Pryke, C., Ramachandra, N. S., Reichardt, C. L., Remolina González, J. D., Romer, A. K., Roodman, A., Ruhl, J. E., Rykoff, E. S., Saliwanchik, B. R., Sanchez, E., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Serrano, S., Sharon, K., Sievers, C., Smecher, G., Smith, M., Soares-Santos, M., Stark, A. A., Story, K. T., Suchyta, E., Tarle, G., Tucker, C., Vanderlinde, K., Veach, T., Vieira, J. D., Wang, G., Weller, J., Whitehorn, N., Wu, W. L. K., Yefremenko, V., and Zhang, Y. The SPTpol Extended Cluster Survey. United States: N. p., 2020. Web. doi:10.3847/1538-4365/ab6993.
Bleem, L. E., Bocquet, S., Stalder, B., Gladders, M. D., Ade, P. A. R., Allen, S. W., Anderson, A. J., Annis, J., Ashby, M. L. N., Austermann, J. E., Avila, S., Avva, J. S., Bayliss, M., Beall, J. A., Bechtol, K., Bender, A. N., Benson, B. A., Bertin, E., Bianchini, F., Blake, C., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Carrasco Kind, M., Carretero, J., Chang, C. L., Chiang, H. C., Citron, R., Moran, C. Corbett, Costanzi, M., Crawford, T. M., Crites, A. T., da Costa, L. N., de Haan, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Eifler, T. F., Everett, W., Flaugher, B., Floyd, B., Frieman, J., Gallicchio, J., García-Bellido, J., George, E. M., Gerdes, D. W., Gilbert, A., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Halverson, N. W., Harrington, N., Henning, J. W., Heymans, C., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., James, D. J., Jeltema, T., Joudaki, S., Khullar, G., Klein, M., Knox, L., Kuropatkin, N., Lee, A. T., Li, D., Lidman, C., Lowitz, A., MacCrann, N., Mahler, G., Maia, M. A. G., Marshall, J. L., McDonald, M., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miquel, R., Mocanu, L. M., Mohr, J. J., Montgomery, J., Nadolski, A., Natoli, T., Nibarger, J. P., Noble, G., Novosad, V., Padin, S., Palmese, A., Parkinson, D., Patil, S., Paz-Chinchón, F., Plazas, A. A., Pryke, C., Ramachandra, N. S., Reichardt, C. L., Remolina González, J. D., Romer, A. K., Roodman, A., Ruhl, J. E., Rykoff, E. S., Saliwanchik, B. R., Sanchez, E., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Serrano, S., Sharon, K., Sievers, C., Smecher, G., Smith, M., Soares-Santos, M., Stark, A. A., Story, K. T., Suchyta, E., Tarle, G., Tucker, C., Vanderlinde, K., Veach, T., Vieira, J. D., Wang, G., Weller, J., Whitehorn, N., Wu, W. L. K., Yefremenko, V., & Zhang, Y. The SPTpol Extended Cluster Survey. United States. doi:https://doi.org/10.3847/1538-4365/ab6993
Bleem, L. E., Bocquet, S., Stalder, B., Gladders, M. D., Ade, P. A. R., Allen, S. W., Anderson, A. J., Annis, J., Ashby, M. L. N., Austermann, J. E., Avila, S., Avva, J. S., Bayliss, M., Beall, J. A., Bechtol, K., Bender, A. N., Benson, B. A., Bertin, E., Bianchini, F., Blake, C., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Carrasco Kind, M., Carretero, J., Chang, C. L., Chiang, H. C., Citron, R., Moran, C. Corbett, Costanzi, M., Crawford, T. M., Crites, A. T., da Costa, L. N., de Haan, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dobbs, M. A., Eifler, T. F., Everett, W., Flaugher, B., Floyd, B., Frieman, J., Gallicchio, J., García-Bellido, J., George, E. M., Gerdes, D. W., Gilbert, A., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Halverson, N. W., Harrington, N., Henning, J. W., Heymans, C., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hrubes, J. D., Huang, N., Hubmayr, J., Irwin, K. D., James, D. J., Jeltema, T., Joudaki, S., Khullar, G., Klein, M., Knox, L., Kuropatkin, N., Lee, A. T., Li, D., Lidman, C., Lowitz, A., MacCrann, N., Mahler, G., Maia, M. A. G., Marshall, J. L., McDonald, M., McMahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miquel, R., Mocanu, L. M., Mohr, J. J., Montgomery, J., Nadolski, A., Natoli, T., Nibarger, J. P., Noble, G., Novosad, V., Padin, S., Palmese, A., Parkinson, D., Patil, S., Paz-Chinchón, F., Plazas, A. A., Pryke, C., Ramachandra, N. S., Reichardt, C. L., Remolina González, J. D., Romer, A. K., Roodman, A., Ruhl, J. E., Rykoff, E. S., Saliwanchik, B. R., Sanchez, E., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Serrano, S., Sharon, K., Sievers, C., Smecher, G., Smith, M., Soares-Santos, M., Stark, A. A., Story, K. T., Suchyta, E., Tarle, G., Tucker, C., Vanderlinde, K., Veach, T., Vieira, J. D., Wang, G., Weller, J., Whitehorn, N., Wu, W. L. K., Yefremenko, V., and Zhang, Y. Sun . "The SPTpol Extended Cluster Survey". United States. doi:https://doi.org/10.3847/1538-4365/ab6993. https://www.osti.gov/servlets/purl/1608577.
@article{osti_1608577,
title = {The SPTpol Extended Cluster Survey},
author = {Bleem, L. E. and Bocquet, S. and Stalder, B. and Gladders, M. D. and Ade, P. A. R. and Allen, S. W. and Anderson, A. J. and Annis, J. and Ashby, M. L. N. and Austermann, J. E. and Avila, S. and Avva, J. S. and Bayliss, M. and Beall, J. A. and Bechtol, K. and Bender, A. N. and Benson, B. A. and Bertin, E. and Bianchini, F. and Blake, C. and Brodwin, M. and Brooks, D. and Buckley-Geer, E. and Burke, D. L. and Carlstrom, J. E. and Rosell, A. Carnero and Carrasco Kind, M. and Carretero, J. and Chang, C. L. and Chiang, H. C. and Citron, R. and Moran, C. Corbett and Costanzi, M. and Crawford, T. M. and Crites, A. T. and da Costa, L. N. and de Haan, T. and De Vicente, J. and Desai, S. and Diehl, H. T. and Dietrich, J. P. and Dobbs, M. A. and Eifler, T. F. and Everett, W. and Flaugher, B. and Floyd, B. and Frieman, J. and Gallicchio, J. and García-Bellido, J. and George, E. M. and Gerdes, D. W. and Gilbert, A. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gupta, N. and Gutierrez, G. and Halverson, N. W. and Harrington, N. and Henning, J. W. and Heymans, C. and Holder, G. P. and Hollowood, D. L. and Holzapfel, W. L. and Honscheid, K. and Hrubes, J. D. and Huang, N. and Hubmayr, J. and Irwin, K. D. and James, D. J. and Jeltema, T. and Joudaki, S. and Khullar, G. and Klein, M. and Knox, L. and Kuropatkin, N. and Lee, A. T. and Li, D. and Lidman, C. and Lowitz, A. and MacCrann, N. and Mahler, G. and Maia, M. A. G. and Marshall, J. L. and McDonald, M. and McMahon, J. J. and Melchior, P. and Menanteau, F. and Meyer, S. S. and Miquel, R. and Mocanu, L. M. and Mohr, J. J. and Montgomery, J. and Nadolski, A. and Natoli, T. and Nibarger, J. P. and Noble, G. and Novosad, V. and Padin, S. and Palmese, A. and Parkinson, D. and Patil, S. and Paz-Chinchón, F. and Plazas, A. A. and Pryke, C. and Ramachandra, N. S. and Reichardt, C. L. and Remolina González, J. D. and Romer, A. K. and Roodman, A. and Ruhl, J. E. and Rykoff, E. S. and Saliwanchik, B. R. and Sanchez, E. and Saro, A. and Sayre, J. T. and Schaffer, K. K. and Schrabback, T. and Serrano, S. and Sharon, K. and Sievers, C. and Smecher, G. and Smith, M. and Soares-Santos, M. and Stark, A. A. and Story, K. T. and Suchyta, E. and Tarle, G. and Tucker, C. and Vanderlinde, K. and Veach, T. and Vieira, J. D. and Wang, G. and Weller, J. and Whitehorn, N. and Wu, W. L. K. and Yefremenko, V. and Zhang, Y.},
abstractNote = {We describe the observations and resultant galaxy cluster catalog from the 2770 deg2 SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev–Zel'dovich (SZ) effect and confirmed with a combination of archival and targeted follow-up data, making particular use of data from the Dark Energy Survey (DES). With incomplete follow-up we have confirmed as clusters 244 of 266 candidates at a detection significance ξ ≥ 5 and an additional 204 systems at 4 < ξ < 5. The confirmed sample has a median mass of ${M}_{500c}\sim 4.4\times {10}^{14}\,{M}_{\odot }\,{h}_{70}^{-1}$ and a median redshift of z = 0.49, and we have identified 44 strong gravitational lenses in the sample thus far. Radio data are used to characterize contamination to the SZ signal; the median contamination for confirmed clusters is predicted to be ~1% of the SZ signal at the ξ > 4 threshold, and <4% of clusters have a predicted contamination >10% of their measured SZ flux. We associate SZ-selected clusters, from both SPT-ECS and the SPT-SZ survey, with clusters from the DES redMaPPer sample, and we find an offset distribution between the SZ center and central galaxy in general agreement with previous work, though with a larger fraction of clusters with significant offsets. Adopting a fixed Planck-like cosmology, we measure the optical richness–SZ mass ($\lambda -M$) relation and find it to be 28% shallower than that from a weak-lensing analysis of the DES data—a difference significant at the 4σ level—with the relations intersecting at λ = 60. The SPT-ECS cluster sample will be particularly useful for studying the evolution of massive clusters and, in combination with DES lensing observations and the SPT-SZ cluster sample, will be an important component of future cosmological analyses.},
doi = {10.3847/1538-4365/ab6993},
journal = {The Astrophysical Journal. Supplement Series (Online)},
number = 1,
volume = 247,
place = {United States},
year = {2020},
month = {3}
}

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Deep Full-sky Coadds from Three Years of WISE and NEOWISE Observations
journal, September 2017


Absolute Spectral Energy Distributions for White Dwarfs
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Methods for cluster cosmology and application to the SDSS in preparation for DES Year 1 release
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A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data
journal, January 2018


Tracing cosmic evolution with clusters of galaxies
journal, April 2005


SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope
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Constraining the Redshift Evolution of First Radio Sources in rcs1 Galaxy Clusters
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The Wide-Field Infrared Survey Explorer (Wise): Mission Description and Initial On-Orbit Performance
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The APM Galaxy Survey -- V. Catalogues of galaxy clusters
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The observed growth of massive galaxy clusters - I. Statistical methods and cosmological constraints: Cluster growth: methods and cosmology
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Cluster richness–mass calibration with cosmic microwave background lensing
journal, October 2017


A Weak-Lensing and Near-Infrared Study of A3192: Disassembling a Richness Class 3 Abell Cluster
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amico galaxy clusters in KiDS-DR3: sample properties and selection function
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