activity
20032005
most citedConstraining dark energy with cross-correlated CMB and Large Scale Structure data

122 citations · 129 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2005122 cited

Constraining dark energy with cross-correlated CMB and Large Scale Structure data

P. S. Corasaniti, T. Giannantonio, A. Melchiorri

We investigate the possibility of constraining dark energy with the Integrated Sachs Wolfe effect recently detected by cross-correlating the WMAP maps with several Large Scale Stru…

astro-ph20042 cited

New Constraints on Dark Energy

Alessandro Melchiorri

New Cosmic Microwave Background, Galaxy Clustering and Supernovae type Ia data are increasingly constraining the dark energy component of our Universe. While the cosmological const…

hep-ph20042 cited

Does the Low CMB Quadrupole Provide a New Cosmic Coincidence Problem ?

Alessandro Melchiorri, Laura Mersini-Houghton

We point out that the recent WMAP findings of a suppressed large scale power in the Cosmic Microwave Background anisotropy power spectrum, if of cosmological origin, make the case…

hep-ph20041 cited

Proceedings to the 'Euroconference on Symmetries Beyond the Standard Model', 12. - 17. July 2003, Portoroz, Slovenia (Part 1 of 2)

P. H. Frampton, A. Melchiorri, L. Bonora +7

Contents of Part 1: 1. Status of the Standard Model(P.H. Frampton), 2. Cosmological Constraints from MBA and Polarization (A. Melchiorri), 3. AdS/CFT Correspondence and Unification…

hep-ph20032 cited

Cosmological constraints from Microwave Background Anisotropy and Polarization

Alessandro Melchiorri

The recent high-quality measurements of the Cosmic Microwave Background anisotropies have presented cosmologists with the possibility of studying the large scale properties of our…

astro-ph2003

Maps of the millimetre sky from the BOOMERanG experiment

P. de Bernardis, P. A. R. Ade, A. Balbi +38

In the 1998-99 flight, BOOMERanG has produced maps of of the sky at high Galactic latitudes, at frequencies of 90, 150, 240 and 410 GHz, with resolution $\simgt 10'$. Th…