Cited by 322Galaxies: Formation, Evolution, PhenomenaCosmology and Gravitation TheoriesAstrophysics and Cosmic Phenomena

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GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY

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Staniszewski, Z., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Joy, M., Keisler, R., Lanting, T. M., Lee, A. T., Leitch, E. M., Loehr, A., Lueker, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mohr, J. J., Montroy, T. E., Ngeow, C.-C., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Stalder, B., Stark, A. A., Vanderlinde, K., Vieira, J. D., Zahn, O., Zenteno, A.·2009·The Astrophysical Journal

Abstract

The South Pole Telescope (SPT) is conducting a Sunyaev–Zel'dovich (SZ) effect survey over large areas of the southern sky, searching for massive galaxy clusters to high redshift. In this preliminary study, we focus on a 40 deg 2 area targeted by the Blanco Cosmology Survey (BCS), which is centered roughly at right ascension 5 h 30 m , declination −53° (J2000). Over two seasons of observations, this entire region has been mapped by the SPT at 95 GHz, 150 GHz, and 225 GHz. We report the four most significant SPT detections of SZ clusters in this field, three of which were previously unknown and, therefore, represent the first galaxy clusters discovered with an SZ survey. The SZ clusters are detected as decrements with greater than 5σ significance in the high-sensitivity 150 GHz SPT map. The SZ spectrum of these sources is confirmed by detections of decrements at the corresponding locations in the 95 GHz SPT map and nondetections at those locations in the 225 GHz SPT map. Multiband optical images from the BCS survey demonstrate significant concentrations of similarly colored galaxies at the positions of the SZ detections. Photometric redshift estimates from the BCS data indicate that two of the clusters lie at moderate redshift ( z ∼ 0.4) and two at high redshift ( z ≳ 0.8). One of the SZ detections was previously identified as a galaxy cluster in the optical as part of the Abell supplementary southern cluster catalog and in the X-ray using data from the ROSAT All-Sky Survey (RASS). Potential RASS counterparts (not previously identified as clusters) are also found for two of the new discoveries. These first four galaxy clusters are the most significant SZ detections from a subset of the ongoing SPT survey. As such, they serve as a demonstration that SZ surveys, and the SPT in particular, can be an effective means for finding galaxy clusters.

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Citations

Cites

  • A Universal Density Profile from Hierarchical Clustering

    Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917 · cited 1×

    “…all motivated by some guess at the underlying threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ…”
    Background
  • The Structure of Cold Dark Matter Halos

    Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×

    “…all motivated by some guess at the underlying threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ…”
    Background
  • A catalog of rich clusters of galaxies

    Abell, G. O., Jr. Corwin Harold, G., & Olowin, R. P. (1989) · The Astrophysical Journal Supplement Series · doi:10.1086/191333 · Cited by 1,406 · cited 2×

    “In SPT-CL 0517-5430, the cluster that was previously included in the Abell supplementary southern cluster catalog (Abell et al. 1989) and the REFLEX catalog (Böhringer et al. 2004), there is a strong red sequence population apparent in g − r versus r and a peak in the photo-z histogram.”
    Background
  • Cosmology with the Sunyaev-Zel’dovich Effect

    Carlstrom, J. E., Holder, G. P., & Reese, E. D. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093803 · Cited by 957

    Self-citation
  • “A catalog of clusters with masses and redshifts can be used to constrain the matter density, the density fluctuation amplitude, and the dark energy equation of state (Wang & Steinhardt 1998; Haiman et al. 2001; Holder et al. 2001; Molnar et al. 2004; Wang et al. 2004; Lima & Hu 2007).”
    Method
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    “Observations of the SZ effect, therefore, permit the detection of clusters with a selection function that is nearly redshift-independent (Birkinshaw 1999; Carlstrom et al. 2002).”
  • SUMSS: a wide-field radio imaging survey of the southern sky - II. The source catalogue

    Mauch, T., Murphy, T., Buttery, H. J., Curran, J., Hunstead, R. W., Piestrzynski, B., Robertson, J. G., & Sadler, E. M. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06605.x · Cited by 823 · cited 1×

    “The astrometry of the pointing model is tied to the PMN and SUMSS catalogs (Wright et al. 1994; Mauch et al. 2003) and is accurate to 10 arcsec in the final maps.”
    Method
  • The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey

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  • Detection of polarization in the cosmic microwave background using DASI

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    MethodSelf-citation
  • Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium

    Nagai, D., Kravtsov, A. V., & Vikhlinin, A. (2007) · The Astrophysical Journal · doi:10.1086/521328 · Cited by 536 · cited 1×

    “…threedimensional pressure profile of clusters: a modified version of the Navarro-Frenk-White (NFW; Navarro et al. 1996, 1997) model as suggested in Nagai et al. (2007), numerically integrated along the line of sight to produce a model for the SZ surface brightness; a Gaussian profile; and a…”
    Method

Show all 46 references

Research works printed but not linked: 6

  1. Carlstrom, 2009, PASP
  2. Halverson, 2009, ApJ
  3. Sunyaev, 1970, Comments Astrophys. Space Phys., 2, 66
  4. Sunyaev, 1972, Comments Astrophys. Space Phys., 4, 173
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Metadata

Authors
Staniszewski, Z., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., de Haan, T., Dobbs, M. A., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Joy, M., Keisler, R., Lanting, T. M., Lee, A. T., Leitch, E. M., Loehr, A., Lueker, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mohr, J. J., Montroy, T. E., Ngeow, C.-C., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Ruhl, J. E., Schaffer, K. K., Shaw, L., Shirokoff, E., Spieler, H. G., Stalder, B., Stark, A. A., Vanderlinde, K., Vieira, J. D., Zahn, O., & Zenteno, A.
Affiliations
  • Case Western Reserve University (US)
  • Cardiff University (GB)
  • University of Chicago (US)
  • University of California, Berkeley (US)
  • McGill University (CA)
  • University of Colorado Boulder (US)
  • Marshall Space Flight Center (US)
  • Lawrence Berkeley National Laboratory (US)
  • Center for Astrophysics Harvard & Smithsonian (US)
  • University of Illinois Urbana-Champaign (US)
Venue
The Astrophysical Journal
Published
2009-07-20
Volume
701
Issue
1
Pages
32-41
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2149892437
Cited by
322
References
46
Citations by year
2026: 4 · 2025: 11 · 2024: 12 · 2023: 5 · 2022: 4 · 2021: 14 · 2020: 15 · 2019: 35 · 2018: 19 · 2017: 9 · 2016: 17 · 2015: 19 · 2014: 17 · 2013: 24 · 2012: 21
FWCI
19.66
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (publishedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (0114422, 0813534, 0130612, 0715036, 0638937, 0708539)
  • Gordon and Betty Moore Foundation
  • University of Chicago
  • Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley
  • McGill University
  • Kavli Institute for Cosmological Physics, University of Chicago
  • Office of Polar Programs
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 › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
Keywords
galaxy clusters, Sunyaev-Zel'dovich effect, South Pole Telescope, high-redshift clusters, photometric redshifts, millimeter-wave observations

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