Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82

Pereira, Maria E. S.; Soares-Santos, Marcelle; Makler, Martin; Annis, James; Lin, Huan; Palmese, Antonella; Vitorelli, Andre Z.; Welch, Brian; Caminha, Gabriel B.; Erben, Thomas; Moraes, Bruno; Shan, Huanyuan

doi:10.1093/mnras/stx2831

Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82

Journal Article · Wed Nov 01 00:00:00 EDT 2017 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stx2831· OSTI ID:1407125

^[1]; ^[2]; Makler, Martin ^[3]; Annis, James ^[4]; Lin, Huan ^[4]; Palmese, Antonella ^[5]; ^[6]; Welch, Brian ^[7]; Caminha, Gabriel B. ^[8]; Erben, Thomas ^[9]; Moraes, Bruno ^[10]; Shan, Huanyuan ^[9]

Brandeis Univ., Waltham, MA (United States); Centro Brasileiro do Pesquisas Fisicas, Rio de Janeiro (Brazil)
Brandeis Univ., Waltham, MA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Centro Brasileiro do Pesquisas Fisicas, Rio de Janeiro (Brazil)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. College London, London (United Kingdom)
Instituto de Astronomia, Sao Paulo-SP (Brazil)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
Univ. degli Studi di Ferrara, Ferrara (Italy); INAF-Osservatorio Astronomico di Bologna, Bologna (Italy)
Argelander-Institut fur Astronomie, Bonn (Germany)
Univ. College London, London (United Kingdom)

Here, we present the first weak lensing calibration of μ*, a new galaxy cluster mass proxy corresponding to the total stellar mass of red and blue members, in two cluster samples selected from the SDSS Stripe 82 data: 230 red-sequence Matched-filter Probabilistic Percolation (redMaPPer) clusters at redshift 0.1 ≤ z < 0.33 and 136 Voronoi Tessellation (VT) clusters at 0.1 ≤ z < 0.6. We use the CS82 shear catalogue and stack the clusters in μ* bins to measure a mass-observable power-law relation. For redMaPPer clusters we obtain M0 = (1.77 ± 0.36) × 10¹⁴ h^–1M_⊙, α = 1.74 ± 0.62. For VT clusters, we find M₀ = (4.31 ± 0.89) × 10¹⁴ h^–1M_⊙, α = 0.59 ± 0.54 and M0 = (3.67 ± 0.56) × 10¹⁴ h^–1M_⊙, α = 0.68 ± 0.49 for a low and a high redshift bin, respectively. Our results are consistent, internally and with the literature, indicating that our method can be applied to any cluster-finding algorithm. In particular, we recommend that μ* be used as the mass proxy for VT clusters. Catalogues including μ* measurements will enable its use in studies of galaxy evolution in clusters and cluster cosmology.

View Accepted Manuscript (DOE)

Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1407125

Report Number(s):: FERMILAB-PUB--17-455-AE; arXiv:1708.03329; 1615728

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 474; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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