activity
19982020
most citedThe contribution of the Unresolved Extragalactic Radio Sources to the Brightness Temperature of the sky

80 citations · 467 across the 17 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2020★ 10 cited

QUBIC: the Q & U Bolometric Interferometer for Cosmology

E. S. Battistelli, P. Ade, J. G. Alberro +136

The Q & U Bolometric Interferometer for Cosmology, QUBIC, is an innovative experiment designed to measure the polarization of the Cosmic Microwave Background and in particular the…

astro-ph.IM2016★ 2 cited

Challenges and prospects for better measurements of the CMB intensity spectrum

Giorgio Sironi

Spectral distortions of the Cosmic Microwave Background (CMB) offer the possibility of probing processes which occurred during the evolution of our Universe going back up to Z$\sim…

astro-ph.CO2013★ 27 cited

An improved upper limit to the CMB circular polarization at large angular scales

R. Mainini, D. Minelli, M. Gervasi +7

Circular polarization of the Cosmic Microwave Background (CMB) offers the possibility of detecting rotations of the universe and magnetic fields in the primeval universe or in dist…

astro-ph.HE2010

On the detectability of cosmic ray electron spectral features in the microwave/mm-wave range

Andrea Tartari, Massimo Gervasi, Giorgio Sironi +2

Recent measurements of cosmic ray electron energy spectra suggest that above 10 GeV there may be deviations from a single power law spectrum. There are hints (ATIC) for a bump occu…

astro-ph.CO2010

Confidence Level Estimator for cosmological model (Research Note)

Giorgio Sironi

Models of the Universe like the Concordance Model today used to interpret cosmological observations give expectation values for many cosmological observable so accurate that freque…

astro-ph.IM2010★ 66 cited

QUBIC: The QU Bolometric Interferometer for Cosmology

The QUBIC collaboration, E. Battistelli, A. Baù +57

One of the major challenges of modern cosmology is the detection of B-mode polarization anisotropies in the CMB. These originate from tensor fluctuations of the metric produced dur…