activity
19982005
most citedStochastic gravitational wave background from cold dark matter halos

18 citations · 21 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph200518 cited

Stochastic gravitational wave background from cold dark matter halos

Carmelita Carbone, Carlo Baccigalupi, Sabino Matarrese

The current knowledge of cosmological structure formation suggests that Cold Dark Matter (CDM) halos possess a nonspherical density profile, implying that cosmic structures can be…

astro-ph20042 cited

Imaging the first light: experimental challenges and future perspectives in the observation of the Cosmic Microwave Background Anisotropy

A. Mennella, C. Baccigalupi, A. Balbi +17

Measurements of the cosmic microwave background (CMB) allow high precision observation of the Last Scattering Surface at redshift 1100. After the success of the NASA satelli…

astro-ph2004

Impact of foregrounds on Cosmic Microwave Background maps

G. De Zotti, C. Burigana, C. Baccigalupi +1

We discuss the possible impact of astrophysical foregrounds on three recent exciting results of Cosmic Microwave Background (CMB) experiments: the WMAP measurements of the temperat…

astro-ph20031 cited

Weak lensing, structure formation and dark energy

Fabio Giovi, Carlo Baccigalupi, Francesca Perrotta

We study how CMB bispectrum, produced by weak gravitational lensing and structure formation, can constrain the redshift evolution of the dark energy equation of state independently…

astro-ph2002

Millimeter-band Surveys of Extragalactic Sources

Gianfranco De Zotti, Francesca Perrotta, Gian Luigi Granato +5

Surveys at mm wavelengths emphasize rare classes of extragalactic radio sources characterized by spectra keeping flat or inverted up to high frequencies (such as blazars, GPS sourc…

astro-ph2001

Clustering properties and gravitational lensing of forming spheroidal galaxies

F. Perrotta, M. Magliocchetti, C. Baccigalupi +5

We show that the predictions of the recent physical model by Granato et al. (2001) are fully consistent with the available estimates of the clustering properties of galaxies at (su…