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Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise
M. A. J. Ashdown, C. Baccigalupi, J. G. Bartlett +21
The Planck satellite will observe the full sky at nine frequencies from 30 to 857 GHz. The goal of this paper is to examine the effects of four realistic instrument systematics in…
Instrumental and Analytic Methods for Bolometric Polarimetry
W. C. Jones, T. E. Montroy, B. P. Crill +6
We discuss instrumental and analytic methods that have been developed for the first generation of bolometric cosmic microwave background (CMB) polarimeters. The design, characteriz…
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…