activity
19982024
most citedMAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

1.3k citations · 7.4k across the 101 of their papers we have counts for

collaborators
Showing 2007Show all

6 papers · 1 filter

astro-ph2007★ 22 cited

Peculiar acceleration

Luca Amendola, Claudia Quercellini, Amedeo Balbi

It has been proposed recently to observe the change in cosmological redshift of distant galaxies or quasars with the next generation of large telescope and ultra-stable spectrograp…

astro-ph2007★ 194 cited

Spherical Needlets for CMB Data Analysis

D. Marinucci, D. Pietrobon, A. Balbi +6

We discuss Spherical Needlets and their properties. Needlets are a form of spherical wavelets which do not rely on any kind of tangent plane approximation and enjoy good localizati…

astro-ph2007★ 59 cited

Affine equation of state from quintessence and k-essence fields

Claudia Quercellini, Marco Bruni, Amedeo Balbi

We explore the possibility that a scalar field with appropriate Lagrangian can mimic a perfect fluid with an affine barotropic equation of state. The latter can be thought of as a…

astro-ph2007★ 68 cited

The time evolution of cosmological redshift as a test of dark energy

A. Balbi, C. Quercellini

The variation of the expansion rate of the Universe with time produces an evolution in the cosmological redshift of distant sources (for example quasar Lyman- absorption lines),…

astro-ph2007★ 35 cited

Making Maps from Planck LFI 30GHz Data

M. A. J. Ashdown, C. Baccigalupi, A. Balbi +16

This paper is one of a series describing the performance and accuracy of map-making codes as assessed by the Planck CTP working group. We compare the performance of multiple codes…

astro-ph2007★ 75 cited

DM: Observational constraints on unified dark matter with constant speed of sound

Amedeo Balbi, Marco Bruni, Claudia Quercellini

We consider the hypothesis that dark energy and dark matter are the two faces of a single dark component, a unified dark matter (UDM) that we assume can be modeled by the affine eq…