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    Rights statement: This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version V Wetzell, J Scott, [et al]. (DES Collaboration), Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue, Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 4, August 2022, Pages 4696–4717, https://doi.org/10.1093/mnras/stac1623 is available online at: https://academic.oup.com/mnras/article-abstract/514/4/4696/6615472

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Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue

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Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue. / DES Collaboration.
In: Monthly Notices of the Royal Astronomical Society, Vol. 514, No. 4, 31.08.2022, p. 4696-4717.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

DES Collaboration 2022, 'Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4, pp. 4696-4717. https://doi.org/10.1093/mnras/stac1623

APA

DES Collaboration (2022). Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue. Monthly Notices of the Royal Astronomical Society, 514(4), 4696-4717. https://doi.org/10.1093/mnras/stac1623

Vancouver

DES Collaboration. Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue. Monthly Notices of the Royal Astronomical Society. 2022 Aug 31;514(4):4696-4717. Epub 2022 Jun 23. doi: 10.1093/mnras/stac1623

Author

DES Collaboration. / Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue. In: Monthly Notices of the Royal Astronomical Society. 2022 ; Vol. 514, No. 4. pp. 4696-4717.

Bibtex

@article{ee1c2f9205a543f5b5358d77b0322ef5,
title = "Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue",
abstract = "We measure the velocity dispersions of clusters of galaxies selected by the red-sequence Matched-filter Probabilistic Percolation (redMaPPer) algorithm in the first three years of data from the Dark Energy Survey (DES), allowing us to probe cluster selection and richness estimation, λ, in light of cluster dynamics. Our sample consists of 126 clusters with sufficient spectroscopy for individual velocity dispersion estimates. We examine the correlations between cluster velocity dispersion, richness, X-ray temperature, and luminosity, as well as central galaxy velocity offsets. The velocity dispersion-richness relation exhibits a bimodal distribution. The majority of clusters follow scaling relations between velocity dispersion, richness, and X-ray properties similar to those found for previous samples; however, there is a significant population of clusters with velocity dispersions that are high for their richness. These clusters account for roughly 22 per cent of the λ < 70 systems in our sample, but more than half (55 per cent) of λ < 70 clusters at z > 0.5. A couple of these systems are hot and X-ray bright as expected for massive clusters with richnesses that appear to have been underestimated, but most appear to have high velocity dispersions for their X-ray properties likely due to line-of-sight structure. These results suggest that projection effects contribute significantly to redMaPPer selection, particularly at higher redshifts and lower richnesses. The redMaPPer determined richnesses for the velocity dispersion outliers are consistent with their X-ray properties, but several are X-ray undetected and deeper data are needed to understand their nature.",
keywords = "galaxies: clusters: general, X-rays: galaxies: clusters",
author = "{DES Collaboration} and V. Wetzell and Jeltema, {T. E.} and B. Hegland and S. Everett and Giles, {P. A.} and R. Wilkinson and A. Farahi and M. Costanzi and Hollowood, {D. L.} and E. Upsdell and A. Saro and J. Myles and A. Bermeo and S. Bhargava and Collins, {C. A.} and D. Cross and O. Eiger and G. Gardner and M. Hilton and J. Jobel and P. Kelly and D. Laubner and Liddle, {A. R.} and Mann, {R. G.} and V. Martinez and J. Mayers and A. McDaniel and Romer, {A. K.} and P. Rooney and M. Sahlen and J. Stott and A. Swart and Turner, {D. J.} and Viana, {P. T. P.} and Abbott, {T. M. C.} and M. Aguena and S. Allam and F. Andrade-Oliveira and J. Annis and J. Asorey and E. Bertin and Burke, {D. L.} and J. Calcino and {Carnero Rosell}, A. and D. Carollo and {Carrasco Kind}, M. and J. Carretero and A. Choi and M. Crocce and {da Costa}, {L. N.}",
note = "This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version V Wetzell, J Scott, [et al]. (DES Collaboration), Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue, Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 4, August 2022, Pages 4696–4717, https://doi.org/10.1093/mnras/stac1623 is available online at: https://academic.oup.com/mnras/article-abstract/514/4/4696/6615472",
year = "2022",
month = aug,
day = "31",
doi = "10.1093/mnras/stac1623",
language = "English",
volume = "514",
pages = "4696--4717",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "4",

}

RIS

TY - JOUR

T1 - Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue

AU - DES Collaboration

AU - Wetzell, V.

AU - Jeltema, T. E.

AU - Hegland, B.

AU - Everett, S.

AU - Giles, P. A.

AU - Wilkinson, R.

AU - Farahi, A.

AU - Costanzi, M.

AU - Hollowood, D. L.

AU - Upsdell, E.

AU - Saro, A.

AU - Myles, J.

AU - Bermeo, A.

AU - Bhargava, S.

AU - Collins, C. A.

AU - Cross, D.

AU - Eiger, O.

AU - Gardner, G.

AU - Hilton, M.

AU - Jobel, J.

AU - Kelly, P.

AU - Laubner, D.

AU - Liddle, A. R.

AU - Mann, R. G.

AU - Martinez, V.

AU - Mayers, J.

AU - McDaniel, A.

AU - Romer, A. K.

AU - Rooney, P.

AU - Sahlen, M.

AU - Stott, J.

AU - Swart, A.

AU - Turner, D. J.

AU - Viana, P. T. P.

AU - Abbott, T. M. C.

AU - Aguena, M.

AU - Allam, S.

AU - Andrade-Oliveira, F.

AU - Annis, J.

AU - Asorey, J.

AU - Bertin, E.

AU - Burke, D. L.

AU - Calcino, J.

AU - Carnero Rosell, A.

AU - Carollo, D.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Choi, A.

AU - Crocce, M.

AU - da Costa, L. N.

N1 - This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version V Wetzell, J Scott, [et al]. (DES Collaboration), Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue, Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 4, August 2022, Pages 4696–4717, https://doi.org/10.1093/mnras/stac1623 is available online at: https://academic.oup.com/mnras/article-abstract/514/4/4696/6615472

PY - 2022/8/31

Y1 - 2022/8/31

N2 - We measure the velocity dispersions of clusters of galaxies selected by the red-sequence Matched-filter Probabilistic Percolation (redMaPPer) algorithm in the first three years of data from the Dark Energy Survey (DES), allowing us to probe cluster selection and richness estimation, λ, in light of cluster dynamics. Our sample consists of 126 clusters with sufficient spectroscopy for individual velocity dispersion estimates. We examine the correlations between cluster velocity dispersion, richness, X-ray temperature, and luminosity, as well as central galaxy velocity offsets. The velocity dispersion-richness relation exhibits a bimodal distribution. The majority of clusters follow scaling relations between velocity dispersion, richness, and X-ray properties similar to those found for previous samples; however, there is a significant population of clusters with velocity dispersions that are high for their richness. These clusters account for roughly 22 per cent of the λ < 70 systems in our sample, but more than half (55 per cent) of λ < 70 clusters at z > 0.5. A couple of these systems are hot and X-ray bright as expected for massive clusters with richnesses that appear to have been underestimated, but most appear to have high velocity dispersions for their X-ray properties likely due to line-of-sight structure. These results suggest that projection effects contribute significantly to redMaPPer selection, particularly at higher redshifts and lower richnesses. The redMaPPer determined richnesses for the velocity dispersion outliers are consistent with their X-ray properties, but several are X-ray undetected and deeper data are needed to understand their nature.

AB - We measure the velocity dispersions of clusters of galaxies selected by the red-sequence Matched-filter Probabilistic Percolation (redMaPPer) algorithm in the first three years of data from the Dark Energy Survey (DES), allowing us to probe cluster selection and richness estimation, λ, in light of cluster dynamics. Our sample consists of 126 clusters with sufficient spectroscopy for individual velocity dispersion estimates. We examine the correlations between cluster velocity dispersion, richness, X-ray temperature, and luminosity, as well as central galaxy velocity offsets. The velocity dispersion-richness relation exhibits a bimodal distribution. The majority of clusters follow scaling relations between velocity dispersion, richness, and X-ray properties similar to those found for previous samples; however, there is a significant population of clusters with velocity dispersions that are high for their richness. These clusters account for roughly 22 per cent of the λ < 70 systems in our sample, but more than half (55 per cent) of λ < 70 clusters at z > 0.5. A couple of these systems are hot and X-ray bright as expected for massive clusters with richnesses that appear to have been underestimated, but most appear to have high velocity dispersions for their X-ray properties likely due to line-of-sight structure. These results suggest that projection effects contribute significantly to redMaPPer selection, particularly at higher redshifts and lower richnesses. The redMaPPer determined richnesses for the velocity dispersion outliers are consistent with their X-ray properties, but several are X-ray undetected and deeper data are needed to understand their nature.

KW - galaxies: clusters: general

KW - X-rays: galaxies: clusters

U2 - 10.1093/mnras/stac1623

DO - 10.1093/mnras/stac1623

M3 - Journal article

VL - 514

SP - 4696

EP - 4717

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -