4.7 Article

SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS OF THE BULLET CLUSTER (1E 0657-56) WITH APEX-SZ

Journal

ASTROPHYSICAL JOURNAL
Volume 701, Issue 1, Pages 42-51

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/701/1/42

Keywords

cosmic microwave background; cosmology: observations; galaxies: clusters: individual (1E 0657-56)

Funding

  1. National Science Foundation [AST-0138348, AST-0709497]
  2. Director, Office of Science, Office of High Energy and Nuclear Physics, of the U.S. Department of Energy [DE-AC02-05CH11231]
  3. Natural Sciences and Engineering Research Council of Canada
  4. Canadian Institute for Advanced Research
  5. MPG Berkeley-Munich
  6. Alfred P. Sloan Research Fellowship
  7. STFC [ST/G002711/1] Funding Source: UKRI

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We present observations of the Sunyaev-Zel'dovich effect (SZE) in the Bullet cluster (1E 0657-56) using the APEX-SZ instrument at 150 GHz with a resolution of 1'. The main results are maps of the SZE in this massive, merging galaxy cluster. The cluster is detected with 23 sigma significance within the central 1' radius of the source position. The SZE map has a broadly similar morphology to that in existing X-ray maps of this system, and we find no evidence for significant contamination of the SZE emission by radio or IR sources. In order to make simple quantitative comparisons with cluster gas models derived from X-ray observations, we fit our data to an isothermal elliptical beta model, despite the inadequacy of such a model for this complex merging system. With an X-ray-derived prior on the power-law index, beta = 1.04(-0.10)(+0.16), we find a core radius r(c) = 142 '' +/- 18 '', an axial ratio of 0.889 +/- 0.072, and a central temperature decrement of -771 +/- 71 mu K-CMB, including a +/- 5.5% flux calibration uncertainty. Combining the APEX-SZ map with a map of projected electron surface density from Chandra Xray observations, we determine the mass-weighted temperature of the cluster gas to be T-mg = 10.8 +/- 0.9 keV, significantly lower than some previously reported X-ray spectroscopic temperatures. Under the assumption of an isothermal cluster gas distribution in hydrostatic equilibrium, we compute the gas mass fraction for prolate and oblate spheroidal geometries and find it to be consistent with previous results from X-ray and weak-lensing observations. This work is the first result from the APEX-SZ experiment, and represents the first reported scientific result from observations with a large array of multiplexed superconducting transition-edge sensor bolometers.

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