activity
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most citedX-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope

1.2k citations · 2.9k across the 14 of their papers we have counts for

collaborators

14 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.IM2012★ 18 cited

Intensity and polarization of the atmospheric emission at millimetric wavelengths at Dome Concordia

E. S. Battistelli, G. Amico, A. Baù +32

Atmospheric emission is a dominant source of disturbance in ground-based astronomy at mm wavelengths. The Antarctic plateau is recognized to be an ideal site for mm and sub-mm obse…

astro-ph.IM2011★ 1.2k cited

X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope

Joel Vernet, H. Dekker, S. D'Odorico +87

X-shooter is the first 2nd generation instrument of the ESO Very Large Telescope(VLT). It is a very efficient, single-target, intermediate-resolution spectrograph that was installe…

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…

astro-ph.IM2010★ 902 cited

Design Concepts for the Cherenkov Telescope Array

The CTA Consortium

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray…

astro-ph2006★ 30 cited

Archeops In-flight Performance, Data Processing and Map Making

J. F. Macias-Perez, G. Lagache, B. Maffei +69

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave B…