Qubic experiment

Last updated
Q&U Bolometric Interferometer for Cosmology
Qubic instrument shelter 1.jpg
Alternative namesQubic experiment OOjs UI icon edit-ltr-progressive.svg
Location(s)Puna de Atacama
Coordinates 24°11′32″S66°28′29″W / 24.1921°S 66.4747°W / -24.1921; -66.4747 OOjs UI icon edit-ltr-progressive.svg
Altitude4,820 m (15,810 ft) OOjs UI icon edit-ltr-progressive.svg
Wavelength 150, 220 GHz (2.0, 1.4 mm)
Telescope style bolometer
radio interferometer  OOjs UI icon edit-ltr-progressive.svg
Website www.qubic.org.ar OOjs UI icon edit-ltr-progressive.svg
Relief Map of Argentina.jpg
Red pog.svg
Location of Qubic experiment
  Commons-logo.svg Related media on Commons

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]

Contents

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.

On 26 October 2022 the first module was installed and began operating. [3] [1]

QUBIC is an international collaboration involving universities and laboratories in Ireland, 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. 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

Observing site

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 instrument has been 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).

References

  1. 1 2 3 "QUBIC Home" . Retrieved 6 December 2019.
  2. "QUBIC instrument" . Retrieved 14 June 2017.
  3. "QUBIC Installed and In Operation". Qubic Project. Qubic Project. Archived from the original on 24 November 2022. Retrieved 24 November 2022.