Qubic experiment


Q&U Bolometric Interferometer for Cosmology
Alternative namesQubic experiment Edit this at Wikidata
Location(s)Puna de Atacama
Coordinates25°04′06″S 66°38′52″W / 25.068304°S 66.647809°W / -25.068304; -66.647809Coordinates: 25°04′06″S 66°38′52″W / 25.068304°S 66.647809°W / -25.068304; -66.647809 Edit this at Wikidata
Wavelength150, 220 GHz (2.0, 1.4 mm)
First light2019 Edit this on Wikidata
Telescope stylecosmic microwave background experiment
radio interferometer Edit this on Wikidata
Angular resolution23.5 minute of arc Edit this on Wikidata
Websitequbic.in2p3.fr Edit this at Wikidata
Qubic experiment is located in Argentina
Qubic experiment
Location of Qubic experiment

QUBIC is a cosmology project to study cosmic inflation by measuring the B-modes of the polarization of the Cosmic Microwave Background (CMB), by observing the sky with a millimeter wave radio telescope interferometer. It uses bolometric interferometry, which combines the advantages of interferometry (reduction of systematic errors) and those of the bolometer detectors (high signal sensitivity).[1] QUBIC observes the sky at two frequencies, 150 and 220 GHz, so that it can separate the cosmological signal from foreground emission, in particular thermal dust emission.[2]

The QUBIC project began in 2008 with the merger of BRAIN and MBI projects. A technical demonstrator of the instrument is being manufactured and should be tested in France in 2017. A first module should then be installed in Argentina in the region of Alto Chorrillos next to the Large Latin American Millimeter Array.[1]

QUBIC is an international collaboration involving universities and laboratories in France, Italy, Argentina, the U.K. and the U.S.A.[1]

Observing instrument

The observing instrument is a millimeter wave interferometer contained in a cryostat which is cooled to 4K with pulse tube coolers, to avoid contaminating the received signal with thermal radiation. Since millimeter waves are absorbed by water vapor in the atmosphere the device must be located at high altitudes above most of the atmosphere. The first module will be installed at the Large Latin American Millimeter Array (LLAMA) site at Alto de Chorillo near Salta, Argentina, at an altitude of 4,825 meters (15,830 ft).

The millimeter waves pass through a 45 cm polyethylene window in the cryostat and then through a rotating half-wave plate which modulates the polarization, followed by a polarizing grid which selects one of the two polarizing angles. The radiation then passes through an array of 400 microwave horns which


  1. ^ a b c "QUBIC Home". Retrieved 6 December 2019.
  2. ^ "QUBIC instrument". Retrieved 14 June 2017.