Limits on the peculiar velocities of two distant clusters using the kinematic Sunyaev-Zeldovich effect

W. L. Holzapfel, P. A R Ade, S. E. Church, Philip Mauskopf, Y. Rephaeli, T. M. Wilbanks, A. E. Lange

Research output: Contribution to journalArticle

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Abstract

We report millimeter-wavelength observations of the Sunyaev-Zeldovich (S-Z) effect in two distant galaxy clusters. A relativistically correct analysis of the S-Z data is combined with the results of X-ray observations to determine the radial peculiar velocities (vr) of the clusters. We observed Abell 2163 (z = 0.201) in three millimeter-wavelength bands centered at 2.1, 1.4, and 1.1 mm. We report a significant detection of the thermal component of the S-Z effect seen as both a decrement in the brightness of the CMB at 2.1 mm and as an increment at 1.1 mm. Including uncertainties due to the calibration of the instrument, distribution and temperature of the intracluster gas, and astrophysical confusion, a simultaneous fit to the data in all three bands gives vr = +490-880 +1370 km s-1 at 68% confidence. We observed Abell 1689 (z = 0.181) in the 2.1 and 1.4 mm bands. Including the same detailed accounting of uncertainty, a simultaneous fit to the data in both bands gives vr = +170-630 +815 km s-1. The limits on the peculiar velocities of A2163 and A1689 correspond to deviations from the uniform Hubble flow of ≲2%-3%.

Original languageEnglish (US)
Pages (from-to)35-48
Number of pages14
JournalAstrophysical Journal
Volume481
Issue number1 PART I
DOIs
StatePublished - 1997
Externally publishedYes

Fingerprint

Sunyaev-Zeldovich effect
kinematics
wavelength
confusion
wavelengths
calibration
confidence
astrophysics
brightness
galaxies
deviation
gas
effect
temperature
gases
x rays

Keywords

  • Cosmic microwave background
  • Cosmology: observations
  • Galaxies: clusters: individual (Abell 2163, Abell 1689)
  • Large-scale structure of universe
  • Radio continuum: galaxies
  • X-rays: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Holzapfel, W. L., Ade, P. A. R., Church, S. E., Mauskopf, P., Rephaeli, Y., Wilbanks, T. M., & Lange, A. E. (1997). Limits on the peculiar velocities of two distant clusters using the kinematic Sunyaev-Zeldovich effect. Astrophysical Journal, 481(1 PART I), 35-48. https://doi.org/10.1086/304019

Limits on the peculiar velocities of two distant clusters using the kinematic Sunyaev-Zeldovich effect. / Holzapfel, W. L.; Ade, P. A R; Church, S. E.; Mauskopf, Philip; Rephaeli, Y.; Wilbanks, T. M.; Lange, A. E.

In: Astrophysical Journal, Vol. 481, No. 1 PART I, 1997, p. 35-48.

Research output: Contribution to journalArticle

Holzapfel, WL, Ade, PAR, Church, SE, Mauskopf, P, Rephaeli, Y, Wilbanks, TM & Lange, AE 1997, 'Limits on the peculiar velocities of two distant clusters using the kinematic Sunyaev-Zeldovich effect', Astrophysical Journal, vol. 481, no. 1 PART I, pp. 35-48. https://doi.org/10.1086/304019
Holzapfel, W. L. ; Ade, P. A R ; Church, S. E. ; Mauskopf, Philip ; Rephaeli, Y. ; Wilbanks, T. M. ; Lange, A. E. / Limits on the peculiar velocities of two distant clusters using the kinematic Sunyaev-Zeldovich effect. In: Astrophysical Journal. 1997 ; Vol. 481, No. 1 PART I. pp. 35-48.
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AB - We report millimeter-wavelength observations of the Sunyaev-Zeldovich (S-Z) effect in two distant galaxy clusters. A relativistically correct analysis of the S-Z data is combined with the results of X-ray observations to determine the radial peculiar velocities (vr) of the clusters. We observed Abell 2163 (z = 0.201) in three millimeter-wavelength bands centered at 2.1, 1.4, and 1.1 mm. We report a significant detection of the thermal component of the S-Z effect seen as both a decrement in the brightness of the CMB at 2.1 mm and as an increment at 1.1 mm. Including uncertainties due to the calibration of the instrument, distribution and temperature of the intracluster gas, and astrophysical confusion, a simultaneous fit to the data in all three bands gives vr = +490-880 +1370 km s-1 at 68% confidence. We observed Abell 1689 (z = 0.181) in the 2.1 and 1.4 mm bands. Including the same detailed accounting of uncertainty, a simultaneous fit to the data in both bands gives vr = +170-630 +815 km s-1. The limits on the peculiar velocities of A2163 and A1689 correspond to deviations from the uniform Hubble flow of ≲2%-3%.

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