activity
20052008
most citedSimulating polarized Galactic synchrotron emission at all frequencies, the Hammurabi code

118 citations · 308 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph2008118 cited

Simulating polarized Galactic synchrotron emission at all frequencies, the Hammurabi code

A. Waelkens, T. Jaffe, M. Reinecke +2

We present a publicly available code called Hammurabi for generating mock polarized observations of Galactic synchrotron emission for telescopes like LOFAR, SKA, Planck and WMAP, b…

astro-ph200684 cited

Bianchi Type VII_h Models and the WMAP 3-year Data

T. R. Jaffe, A. J. Banday, H. K. Eriksen +2

Context. A specific example of Bianchi Type VIIh models, i.e. those including universal rotation (vorticity) and differential expansion (shear), has been shown in Jaffe et al. (200…

astro-ph200679 cited

Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data

T. R. Jaffe, A. J. Banday, H. K. Eriksen +2

We explore methods of fitting templates to cosmic microwave background (CMB) data, and in particular demonstrate the application of the total convolver algorithm as a fast method o…

astro-ph200627 cited

No Higher Criticism of the Bianchi Corrected WMAP Data

L. Cayon, A. J. Banday, T. Jaffe +4

Motivated by the success of the Bianchi VII_h model in addressing many of the anomalies observed in the WMAP data (Jaffe et al.), we present calculations in real and in wavelet spa…

astro-ph2005

On the Viability of Bianchi Type VIIh Models with Dark Energy

T. R. Jaffe, S. Hervik, A. J. Banday +1

We generalize the predictions for the CMB anisotropy patterns arising in Bianchi type VIIh universes to include a dark energy component. We consider these models in light of the re…

astro-ph2005

A determination of the Spectra of Galactic components observed by WMAP

R. D. Davies, C. Dickinson, A. J. Banday +3

WMAP data when combined with ancillary data on free-free, synchrotron and dust allow an improved understanding of the spectrum of emission from each of these components. Here we ex…