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. Martinis; S. 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

doi:10.1086/340118

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

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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 Ω_tot, Ω_bh², Ω _ch², and n_s.

Original language	English (US)
Pages (from-to)	604-614
Number of pages	11
Journal	Astrophysical Journal
Volume	571
Issue number	2 I
DOIs	https://doi.org/10.1086/340118
State	Published - Jun 1 2002
Externally published	Yes

Keywords

Cosmic microwave background
Cosmology: observations

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/340118

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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., ... 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, 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

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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.",

keywords = "Cosmic microwave background, Cosmology: observations",

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

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doi = "10.1086/340118",

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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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JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 I

ER -

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

Abstract

Keywords

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