activity
20022009
most citedHigh Galactic latitude polarized emission at 1.4 GHz and implications for cosmic microwave background observations

49 citations · 264 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.CO2009★ 19 cited

The Parkes Galactic Meridian Survey (PGMS): observations and CMB polarization foreground analysis

E. Carretti, M. Haverkorn, D. McConnell +4

We present observations and CMB foreground analysis of the Parkes Galactic Meridian Survey (PGMS), an investigation of the Galactic latitude behaviour of the polarized synchrotron…

astro-ph2008★ 1 cited

PGMS: to study the Galactic magnetism out of the Galactic plane

E. Carretti, M. Haverkorn, D. McConnell +4

The Parkes Galactic Meridian Survey (PGMS) is a 5 deg X 90 deg strip to map the polarized synchrotron emission along a Galactic meridian from the Galactic plane down to the south G…

astro-ph2006★ 2 cited

Basic considerations about experimental approaches to the B-mode of the CMB Polarization

S. Cortiglioni, E. Carretti

The B-mode detection of Cosmic Microwave Background polarization will require new technological developments, able to get sensitivities at least 2 orders of magnitude better than f…

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-ph2006★ 3 cited

Systematic effects induced by a flat isotropic dielectric slab

Claudio Macculi, Mario Zannoni, Oscar Antonio Peverini +3

The instrumental polarization induced by a flat isotropic dielectric slab in microwave frequencies is faced. We find that, in spite of its isotropic nature, such a dielectric can p…

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…