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Ali CMB Polarization Telescope (AliCPT)

Blocky building sits on dirt hill with snowy mountain and blue sky in background.
Ali CMB Polarization Telescope (AliCPT)
Credit: Yong-Ping Li

Telescope Details

Location

Tibet, China

Purpose

Measure cosmic microwave background (CMB) polarization to search for signals of primordial gravitational waves that could confirm the theory of inflation.

NIST’s role

NIST scientists designed, fabricated and characterized the telescopes’ superconducting detector arrays and electronics. NIST delivered an integrated focal plane module to Stanford University, where scientists installed it into the cryostat receiver (a cooled camera), and checked for functionality. The components have been shipped to China, where they are being installed and tested by collaborators.

Significant discoveries

The telescope is currently being commissioned.

Other interesting facts

AliCPT is the only CMB imager to be located in the Northern Hemisphere, which will allow the telescope access to map new regions of the sky to great depths. This will be important in checking other telescopes’ measurements, because signals need to be detected in multiple parts of the sky to be confirmed.

Supported by

Chinese Academy of Sciences

Operated by

An international collaboration led by the Institute of High Energy Physics, with about 100 scientists from China, the United States and Europe.

Media

Light-colored rectangle on black stripe with white above and pink beneath.
Single NIST sensor
Credit: NIST
Six-sided bronze-colored plate lies on a metal surface.
Feedhorn array in stack of gold-plated silicon wafers that directs incoming light to sensors
Credit: NIST

Contacts

Created September 30, 2021, Updated July 17, 2025
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