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Maps of the Millimetre Sky from the BOOMERanG Experiment

Published online by Cambridge University Press:  23 September 2016

P. de Bernardis ,
G. De Troia ,
M. Giacometti ,
A. Iacoangeli ,
S. Masi ,
A. Melchiorri ,
F. Nati ,
F. Piacentini ,
G. Polenta  and
S. Ricciardi
...Show all authors
P. de Bernardis
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
G. De Troia
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
M. Giacometti
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
A. Iacoangeli
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
S. Masi
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
A. Melchiorri
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
F. Nati
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
F. Piacentini
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
G. Polenta
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
S. Ricciardi
Affiliation:
Dipartimento di Fisica, Universita' La Sapienza, Roma, Italy
P. A. R. Ade
Affiliation:
Dept. of Physics and Astronomy, Cardiff University, Wales, UK
P. D. Mauskopf
Affiliation:
Dept. of Physics and Astronomy, Cardiff University, Wales, UK
A. Balbi
Affiliation:
Dipartimento di Fisica, Universita' di Tor Vergata, Roma, Italy
P. Cabella
Affiliation:
Dipartimento di Fisica, Universita' di Tor Vergata, Roma, Italy
G. De Gasperis
Affiliation:
Dipartimento di Fisica, Universita' di Tor Vergata, Roma, Italy
P. Natoli
Affiliation:
Dipartimento di Fisica, Universita' di Tor Vergata, Roma, Italy
N. Vittorio
Affiliation:
Dipartimento di Fisica, Universita' di Tor Vergata, Roma, Italy
J. J. Bock
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA, USA
J. R. Bond
Affiliation:
CITA, University of Toronto, Canada
C. R. Contaldi
Affiliation:
CITA, University of Toronto, Canada
J. Borrill
Affiliation:
NERSC, LBNL, Berkeley, CA, USA
A. Boscaleri
Affiliation:
IFAC-CNR, Firenze, Italy
E. Pascale
Affiliation:
IFAC-CNR, Firenze, Italy Depts. of Physics and Astronomy, University of Toronto, Canada
W. C. Jones
Affiliation:
California Institute of Technology, Pasadena, CA, USA
A. E. Lange
Affiliation:
California Institute of Technology, Pasadena, CA, USA
P. Mason
Affiliation:
California Institute of Technology, Pasadena, CA, USA
V. V. Hristov
Affiliation:
California Institute of Technology, Pasadena, CA, USA
B. P. Crill
Affiliation:
California Institute of Technology, Pasadena, CA, USA CSU Dominguez Hills, Carson, CA, USA
A. De-Oliveira Costa
Affiliation:
Phys. Dept. University of Pennsylvanya, Philadelphia, PA, USA
M. Tegmark
Affiliation:
Phys. Dept. University of Pennsylvanya, Philadelphia, PA, USA
K. Ganga
Affiliation:
IPAC, CalTech, Pasadena, CA, USA
E. Hivon
Affiliation:
IPAC, CalTech, Pasadena, CA, USA
T. Montroy
Affiliation:
IPAC, CalTech, Pasadena, CA, USA
T. Kisner
Affiliation:
Physics Department, CWRU, Cleveland, OH, USA
J. E. Ruhl
Affiliation:
Physics Department, CWRU, Cleveland, OH, USA
A. H. Jaffe
Affiliation:
Astrophysics Group, Imperial College, London, UK
C. MacTavish
Affiliation:
Depts. of Physics and Astronomy, University of Toronto, Canada
C. B. Netterfield
Affiliation:
Depts. of Physics and Astronomy, University of Toronto, Canada
D. Pogosyan
Affiliation:
Physics Dept., University of Alberta, Alberta, Canada
S. Prunet
Affiliation:
Institut d'Astrophysique, Paris, France
G. Romeo
Affiliation:
Istituto Nazionale di Geofisica, Roma, Italy

Abstract

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In the 1998-99 flight, BOOMERanG has produced maps of ∼4% of the sky at high Galactic latitudes, at frequencies of 90, 150, 240 and 410 GHz, with resolution ≳ 10'. The faint structure of the Cosmic Microwave Background at horizon and sub-horizon scales is evident in these maps. These maps compare well to the maps recently obtained at lower frequencies by the WMAP experiment. Here we compare the amplitude and morphology of the structures observed in the two sets of maps. We also outline the polarization sensitive version of BOOMERanG, which was flown early this year to measure the linear polarization of the microwave sky at 150, 240 and 350 GHz.

Type
Session I: Cosmic Microwave Background and Cosmology
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 35 - 42
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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