A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background

C. B. Netterfield, P. A.R. Ade, J. J. Bock, J. R. Bond, J. Borrill, A. Boscaleri, K. Coble, C. R. Contaldi, B. P. Crill, P. De Bernardis, P. Parese, K. Ganga, M. Giacometti, E. Hivon, V. V. Hristov, A. Iacoangeli, A. H. Jaffe, W. C. Jones, A. E. Lange, L. MartinisS. Masi, P. Mason, P. D. Mauskopf, A. Melchiorri, T. Montroy, E. Pascale, F. Piacentini, D. Pogosyan, F. Pongetti, S. Prunet, G. Romeo, J. E. Ruhl, F. Scaramuzzi

Research output: Contribution to journalArticle

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Abstract

This paper presents a measurement of the angular power spectrum of the cosmic microwave background from l = 75 to l = 1025 (∼10′ to 2°.4) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic inflationary models in which the primordial plasma undergoes acoustic oscillations. These results, in concert with other types of cosmological measurements and theoretical models, significantly constrain the values of Ωtot, Ωbh2, Ω ch2, and ns.

Original languageEnglish (US)
Pages (from-to)604-614
Number of pages11
JournalAstrophysical Journal
Volume571
Issue number2 I
DOIs
StatePublished - Jun 1 2002

Fingerprint

power spectra
microwaves
acoustics
oscillation
plasma
oscillations
experiment
microwave
analysis

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Cosmic microwave background
  • Cosmology: observations

Cite this

Netterfield, C. B., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., ... Scaramuzzi, F. (2002). A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background. Astrophysical Journal, 571(2 I), 604-614. https://doi.org/10.1086/340118
Netterfield, C. B. ; Ade, P. A.R. ; Bock, J. J. ; Bond, J. R. ; Borrill, J. ; Boscaleri, A. ; Coble, K. ; Contaldi, C. R. ; Crill, B. P. ; De Bernardis, P. ; Parese, P. ; Ganga, K. ; Giacometti, M. ; Hivon, E. ; Hristov, V. V. ; Iacoangeli, A. ; Jaffe, A. H. ; Jones, W. C. ; Lange, A. E. ; Martinis, L. ; Masi, S. ; Mason, P. ; Mauskopf, P. D. ; Melchiorri, A. ; Montroy, T. ; Pascale, E. ; Piacentini, F. ; Pogosyan, D. ; Pongetti, F. ; Prunet, S. ; Romeo, G. ; Ruhl, J. E. ; Scaramuzzi, F. / A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background. In: Astrophysical Journal. 2002 ; Vol. 571, No. 2 I. pp. 604-614.
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abstract = "This paper presents a measurement of the angular power spectrum of the cosmic microwave background from l = 75 to l = 1025 (∼10′ to 2°.4) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic inflationary models in which the primordial plasma undergoes acoustic oscillations. These results, in concert with other types of cosmological measurements and theoretical models, significantly constrain the values of Ωtot, Ωbh2, Ω ch2, and ns.",
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Netterfield, CB, Ade, PAR, Bock, JJ, Bond, JR, Borrill, J, Boscaleri, A, Coble, K, Contaldi, CR, Crill, BP, De Bernardis, P, Parese, P, Ganga, K, Giacometti, M, Hivon, E, Hristov, VV, Iacoangeli, A, Jaffe, AH, Jones, WC, Lange, AE, Martinis, L, Masi, S, Mason, P, Mauskopf, PD, Melchiorri, A, Montroy, T, Pascale, E, Piacentini, F, Pogosyan, D, Pongetti, F, Prunet, S, Romeo, G, Ruhl, JE & Scaramuzzi, F 2002, 'A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background', Astrophysical Journal, vol. 571, no. 2 I, pp. 604-614. https://doi.org/10.1086/340118

A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background. / Netterfield, C. B.; Ade, P. A.R.; Bock, J. J.; Bond, J. R.; Borrill, J.; Boscaleri, A.; Coble, K.; Contaldi, C. R.; Crill, B. P.; De Bernardis, P.; Parese, P.; Ganga, K.; Giacometti, M.; Hivon, E.; Hristov, V. V.; Iacoangeli, A.; Jaffe, A. H.; Jones, W. C.; Lange, A. E.; Martinis, L.; Masi, S.; Mason, P.; Mauskopf, P. D.; Melchiorri, A.; Montroy, T.; Pascale, E.; Piacentini, F.; Pogosyan, D.; Pongetti, F.; Prunet, S.; Romeo, G.; Ruhl, J. E.; Scaramuzzi, F.

In: Astrophysical Journal, Vol. 571, No. 2 I, 01.06.2002, p. 604-614.

Research output: Contribution to journalArticle

TY - JOUR

T1 - A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background

AU - Netterfield, C. B.

AU - Ade, P. A.R.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Boscaleri, A.

AU - Coble, K.

AU - Contaldi, C. R.

AU - Crill, B. P.

AU - De Bernardis, P.

AU - Parese, P.

AU - Ganga, K.

AU - Giacometti, M.

AU - Hivon, E.

AU - Hristov, V. V.

AU - Iacoangeli, A.

AU - Jaffe, A. H.

AU - Jones, W. C.

AU - Lange, A. E.

AU - Martinis, L.

AU - Masi, S.

AU - Mason, P.

AU - Mauskopf, P. D.

AU - Melchiorri, A.

AU - Montroy, T.

AU - Pascale, E.

AU - Piacentini, F.

AU - Pogosyan, D.

AU - Pongetti, F.

AU - Prunet, S.

AU - Romeo, G.

AU - Ruhl, J. E.

AU - Scaramuzzi, F.

PY - 2002/6/1

Y1 - 2002/6/1

N2 - This paper presents a measurement of the angular power spectrum of the cosmic microwave background from l = 75 to l = 1025 (∼10′ to 2°.4) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic inflationary models in which the primordial plasma undergoes acoustic oscillations. These results, in concert with other types of cosmological measurements and theoretical models, significantly constrain the values of Ωtot, Ωbh2, Ω ch2, and ns.

AB - This paper presents a measurement of the angular power spectrum of the cosmic microwave background from l = 75 to l = 1025 (∼10′ to 2°.4) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic inflationary models in which the primordial plasma undergoes acoustic oscillations. These results, in concert with other types of cosmological measurements and theoretical models, significantly constrain the values of Ωtot, Ωbh2, Ω ch2, and ns.

KW - Cosmic microwave background

KW - Cosmology: observations

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U2 - https://doi.org/10.1086/340118

DO - https://doi.org/10.1086/340118

M3 - Article

VL - 571

SP - 604

EP - 614

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2 I

ER -