most citedTheory of Cosmic Microwave Background Polarization

28 citations · 28 across the 2 of their papers we have counts for

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astro-ph200868 cited

Needlet Detection of Features in WMAP CMB Sky and the Impact on Anisotropies and Hemispherical Asymmetries

Davide Pietrobon, Alexandre Amblard, Amedeo Balbi +3

We apply spherical needlets to the Wilkinson Microwave Anisotropy Probe 5-year cosmic microwave background (CMB) dataset, to search for imprints of non-isotropic features in the CM…

astro-ph20084 cited

Detecting the B-mode Polarisation of the CMB with Clover

C. E. North, B. R. Johnson, P. A. R. Ade +41

We describe the objectives, design and predicted performance of Clover, which is a ground-based experiment to measure the faint ``B-mode'' polarisation pattern in the cosmic microw…

astro-ph200816 cited

Harmonic Inpainting of the Cosmic Microwave Background Sky: Formulation and Error Estimate

Kaiki Taro Inoue, Paolo Cabella, Eiichiro Komatsu

We develop a new interpolation scheme, based on harmonic inpainting, for reconstructing the cosmic microwave background temperature data within the Galaxy mask from the data outsid…

astro-ph200786 cited

Constraints on CPT violation from WMAP three year polarization data: a wavelet analysis

Paolo Cabella, Paolo Natoli, Joseph Silk

We perform a wavelet analysis of the temperature and polarization maps of the Cosmic Microwave Background (CMB) delivered by the WMAP experiment in search for a parity violating si…

astro-ph200428 cited

Theory of Cosmic Microwave Background Polarization

Paolo Cabella, Marc Kamionkowski

These lectures introduce some of the basic theory of cosmic microwave background (CMB) polarization with the primary aim of developing the theory of CMB polarization from inflation…

astro-ph2003

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…