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Cited by 31Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesStellar, planetary, and galactic studies

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Mass, light and colour of the cosmic web in the supercluster SCL2243-0935 (z = 0.447)

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Schirmer, M., Hildebrandt, H., Kuijken, K., Erben, T.·2011·Astronomy & Astrophysics
DOI 10.1051/0004-6361/201016348
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Abstract

Aims. In archival 2.2 m MPG-ESO/WFI data we discovered several mass peaks through weak gravitational lensing, forming a possible supercluster at redshift 0.45. Through wide-field imaging and spectroscopy we aim to identify the supercluster centre, confirm individual member clusters, and detect possible connecting filaments.

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  • von der Linden et al. (2014) and Schirmer et al. (2011) confirm a single smooth, round, high-signal-to-noise mass concentration centered on the galaxy concentration in MACS J2243.

    “Their maps cover a much broader field at lower resolution and so are not presented here, but they confirm the von der Linden et al. (2014) picture of a single smooth, round, high-S/N mass concentration centered on the galaxy concentration that appears at the center of the bottom panel of Figure 6.”

    From The Mismeasure of Mergers: Revised Limits on Self-interacting Dark Matter in Merging Galaxy Clusters (2018) · cites this paper as Schirmer et al. (2011)

    Section 3.5 (page unavailable) reports a 10σ weak-lensing detection of MACS J2243, and Section 3.3 says the mass contours are overlaid on a map of its galaxy distribution. These passages support a high-S/N mass concentration associated with the cluster, but the text does not establish that it is single, smooth, round, or precisely centered on the galaxy concentration. (LLM, conf=0.83)

    Experimental — accuracy not yet measured

  • For MACS J2243 east, there is no convincing concentration of galaxies at the Harvey et al. position in either panel or in Schirmer et al. (2011), and neither von der Linden et al. (2014) nor Schirmer et al. (2011) find a lensing peak there.

    “However, there is no convincing concentration of galaxies at this position in either panel of Figure 6, nor in Schirmer et al. (2011).Furthermore, neither von der Linden et al. (2014) nor Schirmer et al. (2011) find a lensing peak here.”

    From The Mismeasure of Mergers: Revised Limits on Self-interacting Dark Matter in Merging Galaxy Clusters (2018) · cites this paper as Schirmer et al. (2011)

    Section 3.3 describes a galaxy-luminosity map with weak-lensing contours, and Section 3.5 reports a detection of MACS J2243. Neither passage identifies the Harvey et al. position or says whether a galaxy concentration or lensing peak is present there. Searches for an eastern substructure and a peak at that position did not resolve the claim. (LLM, conf=0.69)

    Experimental — accuracy not yet measured

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Metadata

Authors
Schirmer, M., Hildebrandt, H., Kuijken, K., & Erben, T.
Affiliations
  • University of Bonn (DE)
  • Leiden University (NL)
ORCID
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2011-07-22
Volume
532
Pages
A57
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361/201016348
OpenAlex
W2081932325
Cited by
31
References
0
Citations by year
2026: 1 · 2024: 1 · 2023: 1 · 2022: 2 · 2020: 1 · 2018: 5 · 2017: 2 · 2016: 5 · 2015: 3 · 2014: 1 · 2013: 3 · 2012: 3
FWCI
1.63
Type
journal article
Language
en
Open access
Locations
  • Astronomy and Astrophysics (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • Springer Link (Chiba Institute of Technology) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • Alfred P. Sloan Foundation
  • Princeton University
  • Ohio State University
  • University of Washington
  • Johns Hopkins University
  • University of Pittsburgh
  • Case Western Reserve University
  • Drexel University
  • Universität Basel
  • University of Portsmouth
  • New Mexico State University
  • European Commission (252760)
  • Deutsche Forschungsgemeinschaft (SPP 1177, ER 327/3-1, TR 33)
  • Bundesministerium für Bildung und Forschung (05AV5PDA/3)
  • Chinese Academy of Sciences
  • Max-Planck-Gesellschaft
  • Max-Planck-Institut für Astronomie
  • Deutsches Elektronen-Synchrotron
  • U.S. Naval Observatory
  • Fermilab
  • Los Alamos National Laboratory
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
cosmic web, superclusters, weak gravitational lensing, galaxy clusters, wide-field imaging, spectroscopy

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