BOOMERANG-BO3 observations of CMB anisotropy and polarization

P. De Bernardis; P. A.R. Ade; J. J. Bock; J. R. Bond; J. Borrill; A. Boscaleri; P. Cabella; C. R. Contaldi; B. P. Crill; G. De Gasperis; A. De Oliveira-Costa; G. De Ivoia; G. Di Stefano; P. Ehlers; E. Hivon; V. Hristov; A. Iacoangeli; A. H. Jaffe; W. C. Jones; T. S. Kisner; A. E. Lange; C. J. MacTavish; C. Marini Bettolo; S. Masi; P. Mason; P. D. Mauskopr; A. Melchiorri; T. E. Montroy; F. Nati; L. Nati; P. Natoli; C. B. Netterfield; E. Pascale; F. Piacentini; D. Pogosyan; G. Polenta; S. Prunet; S. Ricciardi; G. Romeo; J. E. Ruhl; P. Santini; M. Tegmark; E. Torbet; M. Veneziani; N. Vittorio

BOOMERANG-BO3 observations of CMB anisotropy and polarization

P. De Bernardis, P. A.R. Ade, J. J. Bock, J. R. Bond, J. Borrill, A. Boscaleri, P. Cabella, C. R. Contaldi, B. P. Crill, G. De Gasperis, A. De Oliveira-Costa, G. De Ivoia, G. Di Stefano, P. Ehlers, E. Hivon, V. Hristov, A. Iacoangeli, A. H. Jaffe, W. C. Jones, T. S. KisnerA. E. Lange, C. J. MacTavish, C. Marini Bettolo, S. Masi, P. Mason, P. D. Mauskopr, A. Melchiorri, T. E. Montroy, F. Nati, L. Nati, P. Natoli, C. B. Netterfield, E. Pascale, F. Piacentini, D. Pogosyan, G. Polenta, S. Prunet, S. Ricciardi, G. Romeo, J. E. Ruhl, P. Santini, M. Tegmark, E. Torbet, M. Veneziani, N. Vittorio

Research output: Contribution to conference › Paper › peer-review

Abstract

The BOOMERANg-B03 experiment has performed three surveys (deep, shallow, galactic) of selected regions of the southern sky. Maps of the Stores parameters I. Q, U at 145, 245, 345 GHz have been obtained, covering several hundreds of square degrees, with a resolution of ~ 10'. In the deep and shallow surveys, both at high Galactic: Latitudes, the 1 45 GHz I map is dominated by CMB anisotropy. The angular power spectrum cj 1 is consistent with previous measurements from BOOMERanG-B98 . with extended multipoles range and improved precision. A polarized CMB component is detected in the deep survey. The level and shape of cjE and cfE are consistent with the CMB polarization expected in the adiabatic inflationary model best fitting the c7r. Foregrounds are shown to be negligible in the deep survey at 145 GHz.

Original language	English (US)
Pages	57-64
Number of pages	8
State	Published - 2006
Externally published	Yes
Event	41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006 - La Thuile, Italy Duration: Mar 18 2006 → Mar 25 2006

Conference

Conference	41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006
Country/Territory	Italy
City	La Thuile,
Period	3/18/06 → 3/25/06

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics

Cite this

Bernardis, P. D., Ade, P. A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C. R., Crill, B. P., Gasperis, G. D., Oliveira-Costa, A. D., Ivoia, G. D., Stefano, G. D., Ehlers, P., Hivon, E., Hristov, V., Iacoangeli, A., Jaffe, A. H., Jones, W. C., ... Vittorio, N. (2006). BOOMERANG-BO3 observations of CMB anisotropy and polarization. 57-64. Paper presented at 41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006, La Thuile, Italy.

@conference{ab3b9fff78784a4eb37d2cf60fbc0644,

title = "BOOMERANG-BO3 observations of CMB anisotropy and polarization",

abstract = "The BOOMERANg-B03 experiment has performed three surveys (deep, shallow, galactic) of selected regions of the southern sky. Maps of the Stores parameters I. Q, U at 145, 245, 345 GHz have been obtained, covering several hundreds of square degrees, with a resolution of ~ 10'. In the deep and shallow surveys, both at high Galactic: Latitudes, the 1 45 GHz I map is dominated by CMB anisotropy. The angular power spectrum cj 1 is consistent with previous measurements from BOOMERanG-B98 . with extended multipoles range and improved precision. A polarized CMB component is detected in the deep survey. The level and shape of cjE and cfE are consistent with the CMB polarization expected in the adiabatic inflationary model best fitting the c7r. Foregrounds are shown to be negligible in the deep survey at 145 GHz.",

author = "Bernardis, {P. De} and Ade, {P. A.R.} and Bock, {J. J.} and Bond, {J. R.} and J. Borrill and A. Boscaleri and P. Cabella and Contaldi, {C. R.} and Crill, {B. P.} and Gasperis, {G. De} and Oliveira-Costa, {A. De} and Ivoia, {G. De} and Stefano, {G. Di} and P. Ehlers and E. Hivon and V. Hristov and A. Iacoangeli and Jaffe, {A. H.} and Jones, {W. C.} and Kisner, {T. S.} and Lange, {A. E.} and MacTavish, {C. J.} and Bettolo, {C. Marini} and S. Masi and P. Mason and Mauskopr, {P. D.} and A. Melchiorri and Montroy, {T. E.} and F. Nati and L. Nati and P. Natoli and Netterfield, {C. B.} and E. Pascale and F. Piacentini and D. Pogosyan and G. Polenta and S. Prunet and S. Ricciardi and G. Romeo and Ruhl, {J. E.} and P. Santini and M. Tegmark and E. Torbet and M. Veneziani and N. Vittorio",

note = "Publisher Copyright: {\textcopyright} Copyright 2006 by Rencontres de Moriond.; 41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006 ; Conference date: 18-03-2006 Through 25-03-2006",

year = "2006",

language = "English (US)",

pages = "57--64",

}

Bernardis, PD, Ade, PAR, Bock, JJ, Bond, JR, Borrill, J, Boscaleri, A, Cabella, P, Contaldi, CR, Crill, BP, Gasperis, GD, Oliveira-Costa, AD, Ivoia, GD, Stefano, GD, Ehlers, P, Hivon, E, Hristov, V, Iacoangeli, A, Jaffe, AH, Jones, WC, Kisner, TS, Lange, AE, MacTavish, CJ, Bettolo, CM, Masi, S, Mason, P, Mauskopr, PD, Melchiorri, A, Montroy, TE, Nati, F, Nati, L, Natoli, P, Netterfield, CB, Pascale, E, Piacentini, F, Pogosyan, D, Polenta, G, Prunet, S, Ricciardi, S, Romeo, G, Ruhl, JE, Santini, P, Tegmark, M, Torbet, E, Veneziani, M & Vittorio, N 2006, 'BOOMERANG-BO3 observations of CMB anisotropy and polarization', Paper presented at 41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006, La Thuile, Italy, 3/18/06 - 3/25/06 pp. 57-64.

TY - CONF

T1 - BOOMERANG-BO3 observations of CMB anisotropy and polarization

AU - Bernardis, P. De

AU - Ade, P. A.R.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Boscaleri, A.

AU - Cabella, P.

AU - Contaldi, C. R.

AU - Crill, B. P.

AU - Gasperis, G. De

AU - Oliveira-Costa, A. De

AU - Ivoia, G. De

AU - Stefano, G. Di

AU - Ehlers, P.

AU - Hivon, E.

AU - Hristov, V.

AU - Iacoangeli, A.

AU - Jaffe, A. H.

AU - Jones, W. C.

AU - Kisner, T. S.

AU - Lange, A. E.

AU - MacTavish, C. J.

AU - Bettolo, C. Marini

AU - Masi, S.

AU - Mason, P.

AU - Mauskopr, P. D.

AU - Melchiorri, A.

AU - Montroy, T. E.

AU - Nati, F.

AU - Nati, L.

AU - Natoli, P.

AU - Netterfield, C. B.

AU - Pascale, E.

AU - Piacentini, F.

AU - Pogosyan, D.

AU - Polenta, G.

AU - Prunet, S.

AU - Ricciardi, S.

AU - Romeo, G.

AU - Ruhl, J. E.

AU - Santini, P.

AU - Tegmark, M.

AU - Torbet, E.

AU - Veneziani, M.

AU - Vittorio, N.

PY - 2006

Y1 - 2006

N2 - The BOOMERANg-B03 experiment has performed three surveys (deep, shallow, galactic) of selected regions of the southern sky. Maps of the Stores parameters I. Q, U at 145, 245, 345 GHz have been obtained, covering several hundreds of square degrees, with a resolution of ~ 10'. In the deep and shallow surveys, both at high Galactic: Latitudes, the 1 45 GHz I map is dominated by CMB anisotropy. The angular power spectrum cj 1 is consistent with previous measurements from BOOMERanG-B98 . with extended multipoles range and improved precision. A polarized CMB component is detected in the deep survey. The level and shape of cjE and cfE are consistent with the CMB polarization expected in the adiabatic inflationary model best fitting the c7r. Foregrounds are shown to be negligible in the deep survey at 145 GHz.

AB - The BOOMERANg-B03 experiment has performed three surveys (deep, shallow, galactic) of selected regions of the southern sky. Maps of the Stores parameters I. Q, U at 145, 245, 345 GHz have been obtained, covering several hundreds of square degrees, with a resolution of ~ 10'. In the deep and shallow surveys, both at high Galactic: Latitudes, the 1 45 GHz I map is dominated by CMB anisotropy. The angular power spectrum cj 1 is consistent with previous measurements from BOOMERanG-B98 . with extended multipoles range and improved precision. A polarized CMB component is detected in the deep survey. The level and shape of cjE and cfE are consistent with the CMB polarization expected in the adiabatic inflationary model best fitting the c7r. Foregrounds are shown to be negligible in the deep survey at 145 GHz.

UR - http://www.scopus.com/inward/record.url?scp=85088888347&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85088888347&partnerID=8YFLogxK

M3 - Paper

AN - SCOPUS:85088888347

SP - 57

EP - 64

T2 - 41st Rencontres de Moriond on Cosmology: Contents and Structures of the Universe 2006

Y2 - 18 March 2006 through 25 March 2006

ER -

BOOMERANG-BO3 observations of CMB anisotropy and polarization

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