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Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing

Fuente: arXiv

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Autores principales:	Ansarinejad, B., Raghunathan, S., Abbott, T. M. C., Ade, P. A. R., Aguena, M., Alves, O., Anderson, A. J., Andrade-Oliveira, F., Archipley, M., Balkenhol, L., Benabed, K., Bender, A. N., Benson, B. A., Bertin, E., Bianchini, F., Bleem, L. E., Bocquet, S., Bouchet, F. R., Brooks, D., Bryant, L., Burke, D. L., Camphuis, E., Carlstrom, J. E., Rosell, A. Carnero, Carretero, J., Castander, F. J., Cecil, T. W., Chang, C. L., Chaubal, P., Chichura, P. M., Chou, T. -L., Coerver, A., Costanzi, M., Crawford, T. M., Cukierman, A., da Costa, L. N., Daley, C., Davis, T. M., de Haan, T., Desai, S., De Vicente, J., Dibert, K. R., Dobbs, M. A., Doel, P., Doussot, A., Doux, C., Dutcher, D., Everett, W., Feng, C., Ferguson, K. R., Ferrero, I., Fichman, K., Foster, A., Frieman, J., Galli, S., Gambrel, A. E., García-Bellido, J., Gardner, R. W., Gaztanaga, E., Ge, F., Giannini, G., Goeckner-Wald, N., Grandis, S., Gruendl, R. A., Gualtieri, R., Guidi, F., Guns, S., Gutierrez, G., Halverson, N. W., Hinton, S. R., Hivon, E., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hood, J. C., Huang, N., James, D. J., Kéruzoré, F., Knox, L., Korman, M., Kuo, C. -L., Lee, A. T., Lee, S., Levy, K., Lowitz, A. E., Lu, C., Maniyar, A., Marshall, J. L., Mena-Fernández, J., Menanteau, F., Miquel, R., Millea, M., Mohr, J. J., Montgomery, J., Nakato, Y., Natoli, T., Noble, G. I., Novosad, V., Ogando, R. L. C., Omori, Y., Padin, S., Palmese, A., Pan, Z., Paschos, P., Pereira, M. E. S., Pieres, A., Malagón, A. A. Plazas, Prabhu, K., Quan, W., Rahlin, A., Rahimi, M., Reichardt, C. L., Reil, K., Romer, A. K., Rouble, M., Ruhl, J. E., Sanchez, E., Cid, D. Sanchez, Schiappucci, E., Sevilla-Noarbe, I., Smecher, G., Smith, M., Sobrin, J. A., Stark, A. A., Stephen, J., Suchyta, E., Suzuki, A., Swanson, M. E. C., Tandoi, C., Tarle, G., Thompson, K. L., Thorne, B., Trendafilova, C., Tucker, C., Umilta, C., Vieira, J. D., Wang, G., Weaverdyck, N., Whitehorn, N., Wiseman., P., Wu, W. L. K., Yefremenko, V., Young, M. R., Zebrowski, J. A.
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	Acceder al recurso
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_version_	1866916284668575744
author	Ansarinejad, B. Raghunathan, S. Abbott, T. M. C. Ade, P. A. R. Aguena, M. Alves, O. Anderson, A. J. Andrade-Oliveira, F. Archipley, M. Balkenhol, L. Benabed, K. Bender, A. N. Benson, B. A. Bertin, E. Bianchini, F. Bleem, L. E. Bocquet, S. Bouchet, F. R. Brooks, D. Bryant, L. Burke, D. L. Camphuis, E. Carlstrom, J. E. Rosell, A. Carnero Carretero, J. Castander, F. J. Cecil, T. W. Chang, C. L. Chaubal, P. Chichura, P. M. Chou, T. -L. Coerver, A. Costanzi, M. Crawford, T. M. Cukierman, A. da Costa, L. N. Daley, C. Davis, T. M. de Haan, T. Desai, S. De Vicente, J. Dibert, K. R. Dobbs, M. A. Doel, P. Doussot, A. Doux, C. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Ferrero, I. Fichman, K. Foster, A. Frieman, J. Galli, S. Gambrel, A. E. García-Bellido, J. Gardner, R. W. Gaztanaga, E. Ge, F. Giannini, G. Goeckner-Wald, N. Grandis, S. Gruendl, R. A. Gualtieri, R. Guidi, F. Guns, S. Gutierrez, G. Halverson, N. W. Hinton, S. R. Hivon, E. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hood, J. C. Huang, N. James, D. J. Kéruzoré, F. Knox, L. Korman, M. Kuo, C. -L. Lee, A. T. Lee, S. Levy, K. Lowitz, A. E. Lu, C. Maniyar, A. Marshall, J. L. Mena-Fernández, J. Menanteau, F. Miquel, R. Millea, M. Mohr, J. J. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Novosad, V. Ogando, R. L. C. Omori, Y. Padin, S. Palmese, A. Pan, Z. Paschos, P. Pereira, M. E. S. Pieres, A. Malagón, A. A. Plazas Prabhu, K. Quan, W. Rahlin, A. Rahimi, M. Reichardt, C. L. Reil, K. Romer, A. K. Rouble, M. Ruhl, J. E. Sanchez, E. Cid, D. Sanchez Schiappucci, E. Sevilla-Noarbe, I. Smecher, G. Smith, M. Sobrin, J. A. Stark, A. A. Stephen, J. Suchyta, E. Suzuki, A. Swanson, M. E. C. Tandoi, C. Tarle, G. Thompson, K. L. Thorne, B. Trendafilova, C. Tucker, C. Umilta, C. Vieira, J. D. Wang, G. Weaverdyck, N. Whitehorn, N. Wiseman., P. Wu, W. L. K. Yefremenko, V. Young, M. R. Zebrowski, J. A.
author_facet	Ansarinejad, B. Raghunathan, S. Abbott, T. M. C. Ade, P. A. R. Aguena, M. Alves, O. Anderson, A. J. Andrade-Oliveira, F. Archipley, M. Balkenhol, L. Benabed, K. Bender, A. N. Benson, B. A. Bertin, E. Bianchini, F. Bleem, L. E. Bocquet, S. Bouchet, F. R. Brooks, D. Bryant, L. Burke, D. L. Camphuis, E. Carlstrom, J. E. Rosell, A. Carnero Carretero, J. Castander, F. J. Cecil, T. W. Chang, C. L. Chaubal, P. Chichura, P. M. Chou, T. -L. Coerver, A. Costanzi, M. Crawford, T. M. Cukierman, A. da Costa, L. N. Daley, C. Davis, T. M. de Haan, T. Desai, S. De Vicente, J. Dibert, K. R. Dobbs, M. A. Doel, P. Doussot, A. Doux, C. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Ferrero, I. Fichman, K. Foster, A. Frieman, J. Galli, S. Gambrel, A. E. García-Bellido, J. Gardner, R. W. Gaztanaga, E. Ge, F. Giannini, G. Goeckner-Wald, N. Grandis, S. Gruendl, R. A. Gualtieri, R. Guidi, F. Guns, S. Gutierrez, G. Halverson, N. W. Hinton, S. R. Hivon, E. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hood, J. C. Huang, N. James, D. J. Kéruzoré, F. Knox, L. Korman, M. Kuo, C. -L. Lee, A. T. Lee, S. Levy, K. Lowitz, A. E. Lu, C. Maniyar, A. Marshall, J. L. Mena-Fernández, J. Menanteau, F. Miquel, R. Millea, M. Mohr, J. J. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Novosad, V. Ogando, R. L. C. Omori, Y. Padin, S. Palmese, A. Pan, Z. Paschos, P. Pereira, M. E. S. Pieres, A. Malagón, A. A. Plazas Prabhu, K. Quan, W. Rahlin, A. Rahimi, M. Reichardt, C. L. Reil, K. Romer, A. K. Rouble, M. Ruhl, J. E. Sanchez, E. Cid, D. Sanchez Schiappucci, E. Sevilla-Noarbe, I. Smecher, G. Smith, M. Sobrin, J. A. Stark, A. A. Stephen, J. Suchyta, E. Suzuki, A. Swanson, M. E. C. Tandoi, C. Tarle, G. Thompson, K. L. Thorne, B. Trendafilova, C. Tucker, C. Umilta, C. Vieira, J. D. Wang, G. Weaverdyck, N. Whitehorn, N. Wiseman., P. Wu, W. L. K. Yefremenko, V. Young, M. R. Zebrowski, J. A.
contents	We measure the stacked lensing signal in the direction of galaxy clusters in the Dark Energy Survey Year 3 (DES Y3) redMaPPer sample, using cosmic microwave background (CMB) temperature data from SPT-3G, the third-generation CMB camera on the South Pole Telescope (SPT). We estimate the lensing signal using temperature maps constructed from the initial 2 years of data from the SPT-3G 'Main' survey, covering 1500 deg$^2$ of the Southern sky. We then use this signal as a proxy for the mean cluster mass of the DES sample. In this work, we employ three versions of the redMaPPer catalogue: a Flux-Limited sample containing 8865 clusters, a Volume-Limited sample with 5391 clusters, and a Volume&Redshift-Limited sample with 4450 clusters. For the three samples, we find the mean cluster masses to be ${M}_{200{\rm{m}}}=1.66\pm0.13$ [stat.]$\pm0.03$ [sys.], $1.97\pm0.18$ [stat.]$\pm0.05$ [sys.], and $2.11\pm0.20$ [stat.]$\pm0.05$ [sys.]$\times{10}^{14}\ {\rm{M}}_{\odot }$, respectively. This is a factor of $\sim2$ improvement relative to the precision of measurements with previous generations of SPT surveys and the most constraining cluster mass measurements using CMB cluster lensing to date. Overall, we find no significant tensions between our results and masses given by redMaPPer mass-richness scaling relations of previous works, which were calibrated using CMB cluster lensing, optical weak lensing, and velocity dispersion measurements from various combinations of DES, SDSS and Planck data. We then divide our sample into 3 redshift and 3 richness bins, finding no significant tensions with optical weak-lensing calibrated masses in these bins. We forecast a $5.7\%$ constraint on the mean cluster mass of the DES Y3 sample with the complete SPT-3G surveys when using both temperature and polarization data and including an additional $\sim1400$ deg$^2$ of observations from the 'Extended' SPT-3G survey.
format	Preprint
id	arxiv_https___arxiv_org_abs_2404_02153
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing Ansarinejad, B. Raghunathan, S. Abbott, T. M. C. Ade, P. A. R. Aguena, M. Alves, O. Anderson, A. J. Andrade-Oliveira, F. Archipley, M. Balkenhol, L. Benabed, K. Bender, A. N. Benson, B. A. Bertin, E. Bianchini, F. Bleem, L. E. Bocquet, S. Bouchet, F. R. Brooks, D. Bryant, L. Burke, D. L. Camphuis, E. Carlstrom, J. E. Rosell, A. Carnero Carretero, J. Castander, F. J. Cecil, T. W. Chang, C. L. Chaubal, P. Chichura, P. M. Chou, T. -L. Coerver, A. Costanzi, M. Crawford, T. M. Cukierman, A. da Costa, L. N. Daley, C. Davis, T. M. de Haan, T. Desai, S. De Vicente, J. Dibert, K. R. Dobbs, M. A. Doel, P. Doussot, A. Doux, C. Dutcher, D. Everett, W. Feng, C. Ferguson, K. R. Ferrero, I. Fichman, K. Foster, A. Frieman, J. Galli, S. Gambrel, A. E. García-Bellido, J. Gardner, R. W. Gaztanaga, E. Ge, F. Giannini, G. Goeckner-Wald, N. Grandis, S. Gruendl, R. A. Gualtieri, R. Guidi, F. Guns, S. Gutierrez, G. Halverson, N. W. Hinton, S. R. Hivon, E. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hood, J. C. Huang, N. James, D. J. Kéruzoré, F. Knox, L. Korman, M. Kuo, C. -L. Lee, A. T. Lee, S. Levy, K. Lowitz, A. E. Lu, C. Maniyar, A. Marshall, J. L. Mena-Fernández, J. Menanteau, F. Miquel, R. Millea, M. Mohr, J. J. Montgomery, J. Nakato, Y. Natoli, T. Noble, G. I. Novosad, V. Ogando, R. L. C. Omori, Y. Padin, S. Palmese, A. Pan, Z. Paschos, P. Pereira, M. E. S. Pieres, A. Malagón, A. A. Plazas Prabhu, K. Quan, W. Rahlin, A. Rahimi, M. Reichardt, C. L. Reil, K. Romer, A. K. Rouble, M. Ruhl, J. E. Sanchez, E. Cid, D. Sanchez Schiappucci, E. Sevilla-Noarbe, I. Smecher, G. Smith, M. Sobrin, J. A. Stark, A. A. Stephen, J. Suchyta, E. Suzuki, A. Swanson, M. E. C. Tandoi, C. Tarle, G. Thompson, K. L. Thorne, B. Trendafilova, C. Tucker, C. Umilta, C. Vieira, J. D. Wang, G. Weaverdyck, N. Whitehorn, N. Wiseman., P. Wu, W. L. K. Yefremenko, V. Young, M. R. Zebrowski, J. A. Cosmology and Nongalactic Astrophysics We measure the stacked lensing signal in the direction of galaxy clusters in the Dark Energy Survey Year 3 (DES Y3) redMaPPer sample, using cosmic microwave background (CMB) temperature data from SPT-3G, the third-generation CMB camera on the South Pole Telescope (SPT). We estimate the lensing signal using temperature maps constructed from the initial 2 years of data from the SPT-3G 'Main' survey, covering 1500 deg$^2$ of the Southern sky. We then use this signal as a proxy for the mean cluster mass of the DES sample. In this work, we employ three versions of the redMaPPer catalogue: a Flux-Limited sample containing 8865 clusters, a Volume-Limited sample with 5391 clusters, and a Volume&Redshift-Limited sample with 4450 clusters. For the three samples, we find the mean cluster masses to be ${M}_{200{\rm{m}}}=1.66\pm0.13$ [stat.]$\pm0.03$ [sys.], $1.97\pm0.18$ [stat.]$\pm0.05$ [sys.], and $2.11\pm0.20$ [stat.]$\pm0.05$ [sys.]$\times{10}^{14}\ {\rm{M}}_{\odot }$, respectively. This is a factor of $\sim2$ improvement relative to the precision of measurements with previous generations of SPT surveys and the most constraining cluster mass measurements using CMB cluster lensing to date. Overall, we find no significant tensions between our results and masses given by redMaPPer mass-richness scaling relations of previous works, which were calibrated using CMB cluster lensing, optical weak lensing, and velocity dispersion measurements from various combinations of DES, SDSS and Planck data. We then divide our sample into 3 redshift and 3 richness bins, finding no significant tensions with optical weak-lensing calibrated masses in these bins. We forecast a $5.7\%$ constraint on the mean cluster mass of the DES Y3 sample with the complete SPT-3G surveys when using both temperature and polarization data and including an additional $\sim1400$ deg$^2$ of observations from the 'Extended' SPT-3G survey.
title	Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing
topic	Cosmology and Nongalactic Astrophysics
url	https://arxiv.org/abs/2404.02153