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

Abstract

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) × 10 14 h –1M , α = 1.74 ± 0.62. For VT clusters, we find M 0 = (4.31 ± 0.89) × 10 14 h –1M , α = 0.59 ± 0.54 and M0 = (3.67 ± 0.56) × 10 14 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 evolutionmore » in clusters and cluster cosmology.« less

Authors:
ORCiD logo [1]; ORCiD logo [2];  [3];  [4];  [4];  [5]; ORCiD logo [6];  [7];  [8];  [9];  [10];  [9]
  1. Brandeis Univ., Waltham, MA (United States); Centro Brasileiro do Pesquisas Fisicas, Rio de Janeiro (Brazil)
  2. Brandeis Univ., Waltham, MA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  3. Centro Brasileiro do Pesquisas Fisicas, Rio de Janeiro (Brazil)
  4. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  5. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. College London, London (United Kingdom)
  6. Instituto de Astronomia, Sao Paulo-SP (Brazil)
  7. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  8. Univ. degli Studi di Ferrara, Ferrara (Italy); INAF-Osservatorio Astronomico di Bologna, Bologna (Italy)
  9. Argelander-Institut fur Astronomie, Bonn (Germany)
  10. Univ. College London, London (United Kingdom)
Publication Date:
Research Org.:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
OSTI Identifier:
1407125
Report Number(s):
FERMILAB-PUB-17-455-AE; arXiv:1708.03329
Journal ID: ISSN 0035-8711; 1615728
Grant/Contract Number:  
AC02-07CH11359
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 474; Journal Issue: 1; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; gravitational lensing: weak; galaxies: clusters: general; cosmology: observations

Citation Formats

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, and Shan, Huanyuan. Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82. United States: N. p., 2017. Web. doi:10.1093/mnras/stx2831.
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. Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82. United States. doi:10.1093/mnras/stx2831.
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, and Shan, Huanyuan. Wed . "Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82". United States. doi:10.1093/mnras/stx2831. https://www.osti.gov/servlets/purl/1407125.
@article{osti_1407125,
title = {Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82},
author = {Pereira, Maria E. S. and Soares-Santos, Marcelle and Makler, Martin and Annis, James and Lin, Huan and Palmese, Antonella and Vitorelli, Andre Z. and Welch, Brian and Caminha, Gabriel B. and Erben, Thomas and Moraes, Bruno and Shan, Huanyuan},
abstractNote = {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.},
doi = {10.1093/mnras/stx2831},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 474,
place = {United States},
year = {2017},
month = {11}
}

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