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  • Palmese, A. (author)

Stellar mass as a galaxy cluster mass proxy : application to the Dark Energy Survey redMaPPer clusters

  • Article/chapterEnglish2020

Publisher, publication year, extent ...

  • 2020-02-21
  • Oxford University Press (OUP),2020
  • electronicrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:uu-431904
  • https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-431904URI
  • https://doi.org/10.1093/mnras/staa526DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • We introduce a galaxy cluster mass observable, μ⋆, based on the stellar masses of cluster members, and we present results for the Dark Energy Survey (DES) Year 1 (Y1) observations. Stellar masses are computed using a Bayesian model averaging method, and are validated for DES data using simulations and COSMOS data. We show that μ⋆ works as a promising mass proxy by comparing our predictions to X-ray measurements. We measure the X-ray temperature–μ⋆ relation for a total of 129 clusters matched between the wide-field DES Y1 redMaPPer catalogue and Chandra and XMM archival observations, spanning the redshift range 0.1 < z < 0.7. For a scaling relation that is linear in logarithmic space, we find a slope of α = 0.488 ± 0.043 and a scatter in the X-ray temperature at fixed μ⋆ of σlnTX|μ⋆=0.266+0.019−0.020 for the joint sample. By using the halo mass scaling relations of the X-ray temperature from the Weighing the Giants program, we further derive the μ⋆-conditioned scatter in mass, finding σlnM|μ⋆=0.26+0.15−0.10⁠. These results are competitive with well-established cluster mass proxies used for cosmological analyses, showing that μ⋆ can be used as a reliable and physically motivated mass proxy to derive cosmological constraints.

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  • Brooks, D. (author)
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  • Sahlén, Martin,Associate Professor (docent),1979-Uppsala universitet,Observationell astrofysik(Swepub:uu)marsa668 (author)
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  • Walker, A. R. (author)
  • Collaboration, D E S (author)
  • Uppsala universitetObservationell astrofysik (creator_code:org_t)

Related titles

  • In:\mnras: Oxford University Press (OUP)493:4, s. 4591-4606
  • In:Monthly Notices of the Royal Astronomical Society: Oxford University Press (OUP)493:4, s. 4591-46060035-87111365-2966

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