Published May 8, 2002
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ℓ-space spectroscopy of the Cosmic Microwave Background with the BOOMERanG experiment
Chicago
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Abstract
The BOOMERanG experiment has recently produced detailed maps of the Cosmic Microwave Background, where sub-horizon structures are resolved with good signal to noise ratio. A power spectrum (spherical harmonics) analysis of the maps detects three peaks, at multipoles ℓ = (213_(-13)^(+10)),(541_(-32)^(+20))(845_(-25)^(+12)). In this paper we discuss the data analysis and the implications of these results for cosmology.
Additional Information
© 2002 American Institute of Physics. Issue Date: 8 May 2002. This activity has been supported by the University of Rome La Sapienza, Programma Nazionale di Ricerche in Antartide and Agenzia Spaziale Italiana in Italy, by NASA and NSF in USA, by PPARC in UK and by Univ. of Toronto in Canada.Attached Files
Published - BERaipcp02a.pdf
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Additional details
- Eprint ID
- 27568
- Resolver ID
- CaltechAUTHORS:20111102-072248256
- University of Rome La Sapienza Programma Nazionale de Ricerche in Antartide and Agenzia Spaziale Italiana (Italy)
- NASA
- NSF
- PPARC (UK)
- University of Toronto (Canada)
- Created
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2011-11-02Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Series Name
- AIP Conference Series
- Series Volume or Issue Number
- 616