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South Pole Telescope

The South Pole Telescope is a 10 meter diameter telescope operating at the NSF South Pole research station. The telescope is designed for conducting large-area millimeter and sub-millimeter wave surveys of faint, low contrast emission, as required to map primary and secondary anisotropies in the cosmic microwave background. The SPT is a collaboration between the U of Chicago, UC Berkley, Case Western Reserve University, U of Illinois, and Smithsonian Astrophysical Observatory, and is primarily funded through NSF OPP.


Science Goals, Design, Site, etc.

Click on the links below or on the menu above to read more about the SPT.



Measurements of the anisotropy in the Cosmic Microwave Background (CMB), including new results from SPT [Lueker et al., 2009]. The model curves represent the best-fit primary, lensed CMB (red dashed line); thermal and kinetic SZ effect (black lines); residual point sources (yellow solid line); and total (thick red solid line).

KICP Berkeley UIUC Case JPL Harvard-Smithsonian McGill U CU Boulder







Last update:


October 18, 2017