Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey
We study the Sunyaev-Zel'dovich effect (SZE) signature in South Pole Telescope (SPT) data for an ensemble of 719 optically identified galaxy clusters selected from 124.6 deg$^2$ of the Dark Energy Survey (DES) science verification data, detecting a stacked SZE signal down to richness $λ\sim20$....
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Format: | Text |
Language: | unknown |
Published: |
arXiv
2016
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.1605.08770 https://arxiv.org/abs/1605.08770 |
id |
ftdatacite:10.48550/arxiv.1605.08770 |
---|---|
record_format |
openpolar |
spelling |
ftdatacite:10.48550/arxiv.1605.08770 2023-05-15T18:23:17+02:00 Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey Saro, A. Bocquet, S. Mohr, J. Rozo, E. Benson, B. A. Dodelson, S. Rykoff, E. S. Bleem, L. Abbott, T. M. C. Abdalla, F. B. Allen, S. Annis, J. Benoit-Levy, A. Brooks, D. Burke, D. L. Capasso, R. Rosell, A. Carnero Kind, M. Carrasco Carretero, J. Chiu, I. Crawford, T. M. Cunha, C. E. D'Andrea, C. B. da Costa, L. N. Desai, S. Dietrich, J. P. Evrard, A. E. Neto, A. Fausti Flaugher, B. Fosalba, P. Frieman, J. Gangkofner, C. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Grandis, S. Gruen, D. Gruendl, R. A. Gupta, N. Gutierrez, G. Holzapfel, W. L. James, D. J. Kuehn, K. Kuropatkin, N. Lima, M. Marshall, J. L. McDonald, M. Melchior, P. Menanteau, F. Miquel, R. Ogando, R. Plazas, A. A. Rapetti, D. Reichardt, C. L. Reil, K. Romer, A. K. Sanchez, E. Scarpine, V. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Soergel, B. Strazzullo, V. Suchyta, E. Swanson, M. E. C. Tarle, G. Thomas, D. Vikram, V. Walker, A. R. Zenteno, A. 2016 https://dx.doi.org/10.48550/arxiv.1605.08770 https://arxiv.org/abs/1605.08770 unknown arXiv https://dx.doi.org/10.1093/mnras/stx594 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2016 ftdatacite https://doi.org/10.48550/arxiv.1605.08770 https://doi.org/10.1093/mnras/stx594 2022-04-01T11:42:30Z We study the Sunyaev-Zel'dovich effect (SZE) signature in South Pole Telescope (SPT) data for an ensemble of 719 optically identified galaxy clusters selected from 124.6 deg$^2$ of the Dark Energy Survey (DES) science verification data, detecting a stacked SZE signal down to richness $λ\sim20$. The SZE signature is measured using matched-filtered maps of the 2500 deg$^2$ SPT-SZ survey at the positions of the DES clusters, and the degeneracy between SZE observable and matched-filter size is broken by adopting as priors SZE and optical mass-observable relations that are either calibrated using SPT selected clusters or through the Arnaud et al. (2010, A10) X-ray analysis. We measure the SPT signal to noise $ζ$-$λ$, relation and two integrated Compton-$y$ $Y_\textrm{500}$-$λ$ relations for the DES-selected clusters and compare these to model expectations accounting for the SZE-optical center offset distribution. For clusters with $λ> 80$, the two SPT calibrated scaling relations are consistent with the measurements, while for the A10-calibrated relation the measured SZE signal is smaller by a factor of $0.61 \pm 0.12$ compared to the prediction. For clusters at $20 < λ< 80$, the measured SZE signal is smaller by a factor of $\sim$0.20-0.80 (between 2.3 and 10~$σ$ significance) compared to the prediction, with the SPT calibrated scaling relations and larger $λ$ clusters showing generally better agreement. We quantify the required corrections to achieve consistency, showing that there is a richness dependent bias that can be explained by some combination of contamination of the observables and biases in the estimated masses. We discuss possible physical effects, as contamination from line-of-sight projections or from point sources, larger offsets in the SZE-optical centering or larger scatter in the $λ$-mass relation at lower richnesses. Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
spellingShingle |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Saro, A. Bocquet, S. Mohr, J. Rozo, E. Benson, B. A. Dodelson, S. Rykoff, E. S. Bleem, L. Abbott, T. M. C. Abdalla, F. B. Allen, S. Annis, J. Benoit-Levy, A. Brooks, D. Burke, D. L. Capasso, R. Rosell, A. Carnero Kind, M. Carrasco Carretero, J. Chiu, I. Crawford, T. M. Cunha, C. E. D'Andrea, C. B. da Costa, L. N. Desai, S. Dietrich, J. P. Evrard, A. E. Neto, A. Fausti Flaugher, B. Fosalba, P. Frieman, J. Gangkofner, C. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Grandis, S. Gruen, D. Gruendl, R. A. Gupta, N. Gutierrez, G. Holzapfel, W. L. James, D. J. Kuehn, K. Kuropatkin, N. Lima, M. Marshall, J. L. McDonald, M. Melchior, P. Menanteau, F. Miquel, R. Ogando, R. Plazas, A. A. Rapetti, D. Reichardt, C. L. Reil, K. Romer, A. K. Sanchez, E. Scarpine, V. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Soergel, B. Strazzullo, V. Suchyta, E. Swanson, M. E. C. Tarle, G. Thomas, D. Vikram, V. Walker, A. R. Zenteno, A. Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
We study the Sunyaev-Zel'dovich effect (SZE) signature in South Pole Telescope (SPT) data for an ensemble of 719 optically identified galaxy clusters selected from 124.6 deg$^2$ of the Dark Energy Survey (DES) science verification data, detecting a stacked SZE signal down to richness $λ\sim20$. The SZE signature is measured using matched-filtered maps of the 2500 deg$^2$ SPT-SZ survey at the positions of the DES clusters, and the degeneracy between SZE observable and matched-filter size is broken by adopting as priors SZE and optical mass-observable relations that are either calibrated using SPT selected clusters or through the Arnaud et al. (2010, A10) X-ray analysis. We measure the SPT signal to noise $ζ$-$λ$, relation and two integrated Compton-$y$ $Y_\textrm{500}$-$λ$ relations for the DES-selected clusters and compare these to model expectations accounting for the SZE-optical center offset distribution. For clusters with $λ> 80$, the two SPT calibrated scaling relations are consistent with the measurements, while for the A10-calibrated relation the measured SZE signal is smaller by a factor of $0.61 \pm 0.12$ compared to the prediction. For clusters at $20 < λ< 80$, the measured SZE signal is smaller by a factor of $\sim$0.20-0.80 (between 2.3 and 10~$σ$ significance) compared to the prediction, with the SPT calibrated scaling relations and larger $λ$ clusters showing generally better agreement. We quantify the required corrections to achieve consistency, showing that there is a richness dependent bias that can be explained by some combination of contamination of the observables and biases in the estimated masses. We discuss possible physical effects, as contamination from line-of-sight projections or from point sources, larger offsets in the SZE-optical centering or larger scatter in the $λ$-mass relation at lower richnesses. |
format |
Text |
author |
Saro, A. Bocquet, S. Mohr, J. Rozo, E. Benson, B. A. Dodelson, S. Rykoff, E. S. Bleem, L. Abbott, T. M. C. Abdalla, F. B. Allen, S. Annis, J. Benoit-Levy, A. Brooks, D. Burke, D. L. Capasso, R. Rosell, A. Carnero Kind, M. Carrasco Carretero, J. Chiu, I. Crawford, T. M. Cunha, C. E. D'Andrea, C. B. da Costa, L. N. Desai, S. Dietrich, J. P. Evrard, A. E. Neto, A. Fausti Flaugher, B. Fosalba, P. Frieman, J. Gangkofner, C. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Grandis, S. Gruen, D. Gruendl, R. A. Gupta, N. Gutierrez, G. Holzapfel, W. L. James, D. J. Kuehn, K. Kuropatkin, N. Lima, M. Marshall, J. L. McDonald, M. Melchior, P. Menanteau, F. Miquel, R. Ogando, R. Plazas, A. A. Rapetti, D. Reichardt, C. L. Reil, K. Romer, A. K. Sanchez, E. Scarpine, V. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Soergel, B. Strazzullo, V. Suchyta, E. Swanson, M. E. C. Tarle, G. Thomas, D. Vikram, V. Walker, A. R. Zenteno, A. |
author_facet |
Saro, A. Bocquet, S. Mohr, J. Rozo, E. Benson, B. A. Dodelson, S. Rykoff, E. S. Bleem, L. Abbott, T. M. C. Abdalla, F. B. Allen, S. Annis, J. Benoit-Levy, A. Brooks, D. Burke, D. L. Capasso, R. Rosell, A. Carnero Kind, M. Carrasco Carretero, J. Chiu, I. Crawford, T. M. Cunha, C. E. D'Andrea, C. B. da Costa, L. N. Desai, S. Dietrich, J. P. Evrard, A. E. Neto, A. Fausti Flaugher, B. Fosalba, P. Frieman, J. Gangkofner, C. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Grandis, S. Gruen, D. Gruendl, R. A. Gupta, N. Gutierrez, G. Holzapfel, W. L. James, D. J. Kuehn, K. Kuropatkin, N. Lima, M. Marshall, J. L. McDonald, M. Melchior, P. Menanteau, F. Miquel, R. Ogando, R. Plazas, A. A. Rapetti, D. Reichardt, C. L. Reil, K. Romer, A. K. Sanchez, E. Scarpine, V. Schubnell, M. Sevilla-Noarbe, I. Smith, R. C. Soares-Santos, M. Soergel, B. Strazzullo, V. Suchyta, E. Swanson, M. E. C. Tarle, G. Thomas, D. Vikram, V. Walker, A. R. Zenteno, A. |
author_sort |
Saro, A. |
title |
Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
title_short |
Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
title_full |
Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
title_fullStr |
Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
title_full_unstemmed |
Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey |
title_sort |
optical-sze scaling relations for des optically selected clusters within the spt-sz survey |
publisher |
arXiv |
publishDate |
2016 |
url |
https://dx.doi.org/10.48550/arxiv.1605.08770 https://arxiv.org/abs/1605.08770 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1093/mnras/stx594 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1605.08770 https://doi.org/10.1093/mnras/stx594 |
_version_ |
1766202845107847168 |