activity
20052022
most citedA 100-parsec elliptical and twisted ring of cold and dense molecular clouds revealed by Herschel around the Galactic Center

364 citations · 2.4k across the 30 of their papers we have counts for

collaborators
Showing 2009Show all

7 papers · 1 filter

physics.gen-ph2009

1st Roman Young Researchers Meeting Proceedings

E. Cannuccia, M. Migliaccio, D. Pietrobon +29

During the last few decades scientists have been able to test the bases of the physics paradigms, where the quantum mechanics has to match the cosmological scales. Between the extr…

astro-ph.CO2009★ 14 cited

Foreground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year data

P. Cabella, D. Pietrobon, M. Veneziani +5

We constrain the amplitude of primordial non-Gaussianity in the CMB data taking into account the presence of foreground residuals in the maps. We generalise the needlet bispectrum…

astro-ph.CO2009★ 78 cited

Properties of Galactic cirrus clouds observed by BOOMERanG

M. Veneziani, P. A. R. Ade, J. J. Bock +24

The physical properties of galactic cirrus emission are not well characterized. BOOMERanG is a balloon-borne experiment designed to study the cosmic microwave background at high an…

astro-ph.CO2009★ 21 cited

BOOMERanG Constraints on Primordial Non-Gaussianity from Analytical Minkowski Functionals

P. Natoli, G. De Troia, C. Hikage +32

We use Minkowski Functionals (MF) to constrain a primordial non-Gaussian contribution to the CMB intensity field as observed in the 150 GHz and 145 GHz BOOMERanG maps from the 1998…

astro-ph.CO2009★ 12 cited

Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations

M. Veneziani, A. Amblard, A. Cooray +36

The Sunyaev-Zel'dovich (SZ) effect is the inverse Compton-scattering of cosmic microwave background (CMB) photons by hot electrons in the intervening gas throughout the universe. T…

astro-ph.CO2009★ 4 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…