MITO (Millimetric and Infrared Testa Grigia Observatory) is a 3 m telescope dedicated to the study of Cosmic Background Anisotropies. It is located at 3500 m above sea-level at Plateau Rosa, Cervinia. We describe the Observatory and discuss two on-going research programs: a cleaning procedure in order to remove galactic dust signals from cosmological data and a search for cosmic strings toward double-lensed quasars. Both the programs will be carried out by means of a He-3 photometer operating at the frequencies of 5, 10, 12, 30 cm(-1)
The Atacama Cosmology Telescope (ACT) is a 6-meter diameter telescope designed to make detailed meas...
Abstract: The Cherenkov Telescope Array (CTA) project aims at building two observatories, one in the...
To advance the state of the art in very-high-energy (VHE) γ-ray astrophysics, an international conso...
We describe a new ground based telescope dedicated to millimetre cosmological research: MITO, Millim...
MITO is a multi-purpose experiment mainly finalized for sub/mm cosmological observations. Here we de...
High atmospheric performances are necessary to ensure efficient sub/millimetre cosmological observat...
Ground-based observations at millimeter wavelengths are still competitive with space observatories i...
International audienceWe have designed and built a large-throughput dual channel photometer, Diabolo...
Muon telescopes are instruments devoted to the observation of muons. They are produced in the atmosp...
We have designed and built a large-throughput dual channel photometer; Diabolo. This photometer is d...
High atmospheric performances are necessary to ensure efficient sub/millimetre cosmological observat...
Astrophysical observations at millimeter and sub-millimeter wavelengths are one of the most useful t...
We describe the MAXIMA experiment, a balloon-borne measurement designed to map temperature anisotrop...
The European Space Agency Rosetta Spacecraft, launched on March 2, 2004 toward Comet 67P/Churyumov-G...
The satellite MITA, carrying on board the scientific payload NINA-2, was launched on July the 15(th)...
The Atacama Cosmology Telescope (ACT) is a 6-meter diameter telescope designed to make detailed meas...
Abstract: The Cherenkov Telescope Array (CTA) project aims at building two observatories, one in the...
To advance the state of the art in very-high-energy (VHE) γ-ray astrophysics, an international conso...
We describe a new ground based telescope dedicated to millimetre cosmological research: MITO, Millim...
MITO is a multi-purpose experiment mainly finalized for sub/mm cosmological observations. Here we de...
High atmospheric performances are necessary to ensure efficient sub/millimetre cosmological observat...
Ground-based observations at millimeter wavelengths are still competitive with space observatories i...
International audienceWe have designed and built a large-throughput dual channel photometer, Diabolo...
Muon telescopes are instruments devoted to the observation of muons. They are produced in the atmosp...
We have designed and built a large-throughput dual channel photometer; Diabolo. This photometer is d...
High atmospheric performances are necessary to ensure efficient sub/millimetre cosmological observat...
Astrophysical observations at millimeter and sub-millimeter wavelengths are one of the most useful t...
We describe the MAXIMA experiment, a balloon-borne measurement designed to map temperature anisotrop...
The European Space Agency Rosetta Spacecraft, launched on March 2, 2004 toward Comet 67P/Churyumov-G...
The satellite MITA, carrying on board the scientific payload NINA-2, was launched on July the 15(th)...
The Atacama Cosmology Telescope (ACT) is a 6-meter diameter telescope designed to make detailed meas...
Abstract: The Cherenkov Telescope Array (CTA) project aims at building two observatories, one in the...
To advance the state of the art in very-high-energy (VHE) γ-ray astrophysics, an international conso...