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The BaR-SPOrt experiment: measuring the CMBP E-mode power spectrum from Dome C

Published online by Cambridge University Press:  05 January 2006

M. Giard ,
F. Casoli ,
F. Paletou ,
E. Carretti ,
S. Cortiglioni ,
G. Bernardi ,
L. Casarini ,
S. Cecchini ,
C. Macculi ,
M. Ramponi ,
C. Sbarra ,
G. Ventura ,
J. Monari ,
M. Poloni ,
S. Poppi ,
M. Baralis ,
O. A. Peverini ,
R. Tascone ,
G. Virone ,
M. Zannoni ,
S. Bonometto ,
L. Colombo ,
M. Gervasi ,
G. Sironi ,
R. Fabbri ,
V. Natale ,
R. Nesti ,
L. Nicastro ,
P. de Bernardis ,
S. Masi ,
M. de Petris ,
A. Boscaleri ,
M. Sazhin  and
E. Vinyajkin
E. Carretti
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
S. Cortiglioni
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
G. Bernardi
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
L. Casarini
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
S. Cecchini
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
C. Macculi
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
M. Ramponi
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
C. Sbarra
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
G. Ventura
Affiliation:
IASF/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
J. Monari
Affiliation:
IRA/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
M. Poloni
Affiliation:
IRA/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
S. Poppi
Affiliation:
IRA/CNR Bologna, Via Gobetti 101, 40129 Bologna, Italy
M. Baralis
Affiliation:
IEIIT/CNR Torino, C.so Duca degli Abruzzi 24, 10129 Torino, Italy
O. A. Peverini
Affiliation:
IEIIT/CNR Torino, C.so Duca degli Abruzzi 24, 10129 Torino, Italy
R. Tascone
Affiliation:
IEIIT/CNR Torino, C.so Duca degli Abruzzi 24, 10129 Torino, Italy
G. Virone
Affiliation:
IEIIT/CNR Torino, C.so Duca degli Abruzzi 24, 10129 Torino, Italy
M. Zannoni
Affiliation:
IASF/CNR Milano, Via Bassini 15, 20133 Milano, Italy
S. Bonometto
Affiliation:
Dip. di Fisica, Universitá di Milano-Bicocca, P.za della Scienza 3, 20126 Milano, Italy
L. Colombo
Affiliation:
Dip. di Fisica, Universitá di Milano-Bicocca, P.za della Scienza 3, 20126 Milano, Italy
M. Gervasi
Affiliation:
Dip. di Fisica, Universitá di Milano-Bicocca, P.za della Scienza 3, 20126 Milano, Italy
G. Sironi
Affiliation:
Dip. di Fisica, Universitá di Milano-Bicocca, P.za della Scienza 3, 20126 Milano, Italy
R. Fabbri
Affiliation:
Dip. di Fisica, Universitá di Firenze, Via Sansone 1, 50019 Sesto Fiorentino (FI), Italy
V. Natale
Affiliation:
IRA/CNR Firenze, Largo E. Fermi 5, 50125 Firenze, Italy
R. Nesti
Affiliation:
IRA/CNR Firenze, Largo E. Fermi 5, 50125 Firenze, Italy
L. Nicastro
Affiliation:
IASF/CNR Palermo, Via La Malfa 153, 90146 Palermo, Italy
P. de Bernardis
Affiliation:
Universitá di Roma la Sapienza, P.le A. Moro 2, 00185 Roma, Italy
S. Masi
Affiliation:
Universitá di Roma la Sapienza, P.le A. Moro 2, 00185 Roma, Italy
M. de Petris
Affiliation:
Universitá di Roma la Sapienza, P.le A. Moro 2, 00185 Roma, Italy
A. Boscaleri
Affiliation:
IFAC/CNR Firenze, Via Panciatichi 64, 50127, Firenze, Italy
M. Sazhin
Affiliation:
Schternberg Astronomical Institute, Moscow State University, Moscow 119899, Russia
E. Vinyajkin
Affiliation:
NIRFI, 25 B. Pecherskaya St., Nizhnij Novgorod 603600/GSP-51, Russia
Corresponding
E-mail address:
carretti@bo.iasf.cnr.it
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Abstract

The BaR-SPOrt experiment is designed to measure the E-mode power spectrum of the Cosmic Microwave Background Polarization (CMBP) in the multipole range 50 < l < 1000. In the current configuration at 32 GHz it can explore up to l = 400. Recent low frequency observations of the target region show that the synchrotron emission should not contamine the CMBP already at 32 GHz. A 6-month observation of a 6° × 6° sky area during the polar night, in ideal environmental conditions, will allow the Italian-French collaboration to both measure the E–mode power spectrum with appropriate sensitivity and perform important tests of the anomalous dust emission. The BaR-SPOrt 32 GHz instrument, now under test and ready for operations by Spring 2005, is proposed for 1–2 years Winter operations at Dome C.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 14: Dome C Astronomy and Astrophysics Meeting , 2005 , pp. 81 - 86
Copyright
© EAS, EDP Sciences, 2005

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