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20032018
most citedB-Mode contamination by synchrotron emission from 3-years WMAP data

291 citations · 515 across the 13 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2018★ 15 cited

Advanced Diagnostics for the Study of Linearly Polarized Emission. II: Application to Diffuse Interstellar Radio Synchrotron Emission

C. A. Herron, Blakesley Burkhart, B. M. Gaensler +8

Diagnostics of polarized emission provide us with valuable information on the Galactic magnetic field and the state of turbulence in the interstellar medium, which cannot be obtain…

astro-ph.CO2018★ 28 cited

Simulations of Galactic polarized synchrotron emission for Epoch of Reionization observations

M. Spinelli, G. Bernardi, M. G. Santos

The detection of the redshifted cosmological ~cm line signal requires the removal of the Galactic and extragalactic foreground emission, which is orders of magnitude brighter a…

astro-ph2006★ 9 cited

Growing Supermassive Black Holes by Chaotic Accretion

A R King, J E Pringle

We consider the problem of growing the largest supermassive black holes from stellar--mass seeds at high redshift. Rapid growth without violating the Eddington limit requires that…

astro-ph2006★ 291 cited

B-Mode contamination by synchrotron emission from 3-years WMAP data

E. Carretti, G. Bernardi, S. Cortiglioni

We study the contamination of the B-mode of the Cosmic Microwave Background Polarization (CMBP) by Galactic synchrotron in the lowest emission regions of the sky. The 22.8-GHz pola…

astro-ph2006★ 11 cited

1.4 GHz polarimetric observations of the two fields imaged by the DASI experiment

G. Bernardi, E. Carretti, R. J. Sault +2

We present results of polarization observations at 1.4 GHz of the two fields imaged by the DASI experiment (, and $α= 00^{\rm h} 30^{\rm…

astro-ph2005★ 9 cited

Deep 1.4-GHz observations of diffuse polarized emission

E. Carretti, S. Poppi, W. Reich +5

Polarized diffuse emission observations at 1.4-GHz in a high Galactic latitude area of the northern Celestial hemisphere are presented. The 3.2 X 3.2 deg^2 field, centred at RA = 1…