Hostname: page-component-8448b6f56d-cfpbc Total loading time: 0 Render date: 2024-04-25T01:26:06.695Z Has data issue: false hasContentIssue false
  • English
  • Français

Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver

Published online by Cambridge University Press:  23 September 2016

J. B. Peterson ,
A. K. Romer ,
P. L. Gomez ,
P. A. R. Ade ,
J. J. Bock ,
J. R. Bond ,
C. R. Contaldi ,
D. Pogosyan ,
C. Cantalupo  and
M. D. Daub
...Show all authors
J. B. Peterson
Affiliation:
Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213
A. K. Romer
Affiliation:
Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213
P. L. Gomez
Affiliation:
Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213
P. A. R. Ade
Affiliation:
Department of Physics and Astronomy, Cardiff University, CF24 3YB Wales, UK
J. J. Bock
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91125
J. R. Bond
Affiliation:
Canadian Institute for Theoretical Astrophysics, University of Toronto, Canada
C. R. Contaldi
Affiliation:
Canadian Institute for Theoretical Astrophysics, University of Toronto, Canada
D. Pogosyan
Affiliation:
Canadian Institute for Theoretical Astrophysics, University of Toronto, Canada
C. Cantalupo
Affiliation:
Lawrence Berkeley National Laboratory, Berkeley, CA 94720
M. D. Daub
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720
W. L. Holzapfel
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720
M. Lueker
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720
M. Newcomb
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720
D. Woolsey
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720
C. L. Kuo
Affiliation:
Department of Physics, University of California at Berkeley, Berkeley, CA 94720 Department of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125
A. E. Lange
Affiliation:
Department of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125
M. C. Runyan
Affiliation:
Department of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125 Department of Physics, University of Chicago, Chicago, IL 60637
J. Ruhl
Affiliation:
Department of Physics, Case Western Reserve University, Cleveland, OH 44106
J. H. Goldstein
Affiliation:
Department of Physics, Case Western Reserve University, Cleveland, OH 44106 Department of Physics, University of California, Santa Barbara, CA 93106
E. Torbet
Affiliation:
Department of Physics, University of California, Santa Barbara, CA 93106

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Arcminute Cosmology Bolometer Array Receiver (Acbar) is a multifrequency millimeter-wave receiver optimized for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich (SZ) effect in clusters of galaxies. Acbar was installed on the 2.1 m Viper telescope at the South Pole in January 2001 and the results presented here incorporate data through July 2002. The power spectrum of the CMB at 150 GHz over the range ℓ = 150 — 3000 measured by Acbar is presented along with estimates for the values of the cosmological parameters within the context of ΛCDM models. The inclusion of ΩΛ greatly improves the fit to the power spectrum. Three-frequency images of the SZ decrement/increment are also presented for the galaxy cluster 1E0657–67.

Type
Session I: Cosmic Microwave Background and Cosmology
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 43 - 50
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Andreani, P., et al. 1999, ApJ, 513, 23 Google Scholar
Bennett, C. L., et al. 1996, ApJ, 464, L1 Google Scholar
Bond, J. R., Jaffe, A. H., & Knox, L. 1998, Phys. Rev. D, 57, 2117 Google Scholar
Goldstein, J., et al. 2003, ApJ, 599, 773 CrossRefGoogle Scholar
Hinshaw, G., et al. 2003, ApJS, 148, 135.Google Scholar
Kinney, W. H., Kolb, E. W., Melchiorri, A., & Riotto, A. 2003, FERMILAB-Pub-03/117-A, hep-ph/0305130 Google Scholar
Kuo, C. L., et al. 2004, ApJ, 600, 32 Google Scholar
Lay, O. P., & Halverson, N. W. 2000, ApJ, 543, 787 Google Scholar
Markevitch, M., et al. 2002, ApJ, 567, L27 Google Scholar
Peterson, J. B., et al. 2003, PASP, 115, 383 CrossRefGoogle Scholar
Runyan, M. C., et al. 2003, ApJS, 149, 265 CrossRefGoogle Scholar
Spergel, D. N., et al. 2003, ApJS, 148, 175.Google Scholar
Tucker, W. H., Tananbaum, H., & Remillard, R. A. 1995, ApJ, 444, 532 CrossRefGoogle Scholar
Turner, A. D., et al. 2001, Appl. Optics, 40, 4921 Google Scholar