2.4k citations · 15.1k across the 96 of their papers we have counts for
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Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps
G. De Troia, P. A. R. Ade, J. J. Bock +38
We analyze the BOOMERanG 2003 (B03) 145 GHz temperature map to constrain the amplitude of a non Gaussian, primordial contribution to CMB fluctuations. We perform a pixel space anal…
Direct probes of Dark Matter in the cluster 1ES0657-556 through microwave observations
S. Colafrancesco, P. de Bernardis, S. Masi +2
The cluster 1ES0657-556 is an ideal astrophysical laboratory to study the distribution and the nature of Dark Matter because this last component is spatially separated from the int…
Archeops In-flight Performance, Data Processing and Map Making
J. F. Macias-Perez, G. Lagache, B. Maffei +69
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave B…
Trends in Space Astronomy and Cosmic Vision 2015-2025
Catherine Turon, Chris Done, Andreas Quirrenbach +14
As a short introduction to the astronomy session, the response of the community to the Call for Themes issued by ESA and the specific themes selected by the Astronomy Working Group…
A Measurement of the CMB <EE> Spectrum from the 2003 Flight of BOOMERANG
T. E. Montroy, P. A. R. Ade, J. J. Bock +34
We report measurements of the CMB polarization power spectra from the January 2003 Antarctic flight of BOOMERANG. The primary results come from six days of observation of a patch c…
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG
S Masi, P Ade, J Bock +41
We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern…
A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave Background from the 2003 flight of BOOMERANG
F Piacentini, P Ade, J Bock +34
We present a measurement of the temperature-polarization angular cross power spectrum, <TE>, of the Cosmic Microwave Background. The result is based on hours of data fro…
Cosmological Parameters from the 2003 flight of BOOMERANG
C. J. MacTavish, P. A. R. Ade, J. J. Bock +35
We present the cosmological parameters from the CMB intensity and polarization power spectra of the 2003 Antarctic flight of the BOOMERANG telescope. The BOOMERANG data alone const…
Elliptic CMB Sky
V. G. Gurzadyan, P. de Bernardis, G. De Troia +7
The ellipticity of the anisotropy spots of the Cosmic Microwave Background measured by the Wilkinson Microwave Anisotropy Probe (WMAP) has been studied. We find an average elliptic…
The CMB temperature power spectrum from an improved analysis of the Archeops data
M. Tristram, G. Patanchon, J. F. Macias-Perez +47
We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops…
Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?
V. G. Gurzadyan, P. A. R. Ade, P. de Bernardis +19
We have measured the ellipticity of several degree scale anisotropies in the BOOMERanG maps of the Cosmic Microwave Background (CMB) at 150 GHz. The average ellipticity is around 2…
Maps of the millimetre sky from the BOOMERanG experiment
P. de Bernardis, P. A. R. Ade, A. Balbi +38
In the 1998-99 flight, BOOMERanG has produced maps of of the sky at high Galactic latitudes, at frequencies of 90, 150, 240 and 410 GHz, with resolution $\simgt 10'$. Th…
First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops
A. Benoit, P. Ade, A. Amblard +65
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--bor…
Observations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes
K. Coble, P. A. R. Ade, J. J. Bock +32
We present millimeter-wave observations of three extra-galactic and six Galactic sources in the Southern sky. Observations were made at 90, 150, 240 and 400 GHz with resolutions of…
The trispectrum of the Cosmic Microwave Background on sub-degree angular scales: an analysis of the BOOMERanG data
G. De Troia, P. A. R. Ade, J. J. Bock +21
The trispectrum of the cosmic microwave background can be used to assess the level of non-Gaussianity on cosmological scales. It probes the fourth order moment, as a function of an…
Cosmological constraints from Archeops
A. Benoit, P. Ade, A. Amblard +65
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum ha…
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
A. Benoit, P. Ade, A. Amblard +65
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Arch…
Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data
S. Prunet, P. A. R. Ade, J. J. Bock +35
We describe here an iterative method for jointly estimating the noise power spectrum from a CMB experiment's time-ordered data, together with the maximum-likelihood map. We test th…
Foregrounds in the BOOMERANG-LDB data: a preliminary rms analysis
S. Masi, P. A. R. Ade, J. Bock +18
We present a preliminary analysis of the BOOMERanG LDB maps, focused on foregrounds. BOOMERanG detects dust emission at moderately low galactic latitudes () in bands cen…
Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment
P. de Bernardis, P. A. R. Ade, J. J. Bock +35
BOOMERanG has recently resolved structures on the last scattering surface at redshift 1100 with high signal to noise ratio. We review the technical advances which made this…
CMB Analysis of Boomerang & Maxima & the Cosmic Parameters {Omega_tot,Omega_b h^2,Omega_cdm h^2,Omega_Lambda,n_s}
J. R. Bond, P. Ade, A. Balbi +40
We show how estimates of parameters characterizing inflation-based theories of structure formation localized over the past year when large scale structure (LSS) information from ga…
Mapping the CMB Sky: The BOOMERANG experiment
P. de Bernardis, P. A. R. Ade, R. Artusa +23
We describe the BOOMERanG experiment, a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and t…
ARGO CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
Bharat Ratra, Ken Ganga, Radoslaw Stompor +3
We use data from the ARGO cosmic microwave background (CMB) anisotropy experiment to constrain cosmogonies. We account for the ARGO beamwidth and calibration uncertainties, and mar…
CMB anisotropy measurements using stratospheric balloons
P. de Bernardis, S. Masi
We review the topic of Cosmic Microwave Background Anisotropy measurements carried out by means of balloon-borne telescopes. After a short description of the experimental methodolo…