South Pole Telescope
E157654
cosmic microwave background experiment
ground-based observatory
millimeter-wave telescope
radio telescope
The South Pole Telescope is a large millimeter-wave radio telescope located at the Amundsen–Scott South Pole Station, designed primarily to study the cosmic microwave background and the large-scale structure of the universe.
All labels observed (1)
| Label | Occurrences |
|---|---|
| South Pole Telescope canonical | 4 |
Statements (66)
| Predicate | Object |
|---|---|
| instanceOf |
cosmic microwave background experiment
ⓘ
ground-based observatory ⓘ millimeter-wave telescope ⓘ radio telescope ⓘ |
| altitude |
2800 meters
ⓘ
~9300 feet ⓘ |
| aperture | 10-meter primary mirror ⓘ |
| associatedSurvey |
SPT-3G survey
ⓘ
Southern MAssive Cluster Survey ⓘ
surface form:
SPT-SZ survey
SPTpol survey ⓘ |
| collaborationIncludes |
Canadian institutions
ⓘ
East Asian institutions ⓘ European institutions ⓘ United States institutions ⓘ |
| commissioned | 2007 ⓘ |
| constructionStart | 2003 ⓘ |
| country |
United States of America
ⓘ
surface form:
United States
|
| dataUsedFor |
cluster cosmology
ⓘ
cosmological parameter estimation ⓘ cross-correlation with X-ray surveys ⓘ cross-correlation with gravitational lensing surveys ⓘ cross-correlation with optical surveys ⓘ |
| detectorTechnology | transition-edge sensor bolometers ⓘ |
| firstLight | 2007 ⓘ |
| fundedBy |
National Science Foundation
ⓘ
National Science Foundation ⓘ
surface form:
United States National Science Foundation
|
| hemisphere | Southern Hemisphere ⓘ |
| instrument |
SPT-3G camera
ⓘ
SPT-SZ camera ⓘ SPTpol camera ⓘ |
| locatedIn |
Antarctica
ⓘ
South Pole ⓘ |
| location | Amundsen–Scott South Pole Station ⓘ |
| mirrorType | segmented primary mirror ⓘ |
| mountType | alt-azimuth mount ⓘ |
| nearbyFacility |
BICEP experiments
ⓘ
surface form:
BICEP/Keck Array
IceCube Neutrino Observatory ⓘ |
| observatoryComplex |
Amundsen–Scott South Pole Station
ⓘ
surface form:
Amundsen–Scott South Pole Station Dark Sector
|
| observes | southern sky ⓘ |
| operatedBy |
SPT collaboration
ⓘ
University of Chicago ⓘ |
| operationalStatus | active ⓘ |
| primaryPurpose | study of the cosmic microwave background ⓘ |
| researchFocus |
CMB polarization
ⓘ
Sunyaev–Zel’dovich effect ⓘ dark energy ⓘ galaxy clusters ⓘ gravitational lensing of the CMB ⓘ inflationary cosmology ⓘ large-scale structure of the universe ⓘ neutrino mass constraints ⓘ |
| siteAdvantage |
continuous access to same sky region
ⓘ
stable, dry, cold atmosphere ⓘ very low atmospheric water vapor ⓘ |
| SPT-3GFrequencyBands |
150 GHz
ⓘ
220 GHz ⓘ 95 GHz ⓘ |
| SPT-SZCameraFrequencyBands |
150 GHz
ⓘ
220 GHz ⓘ 90 GHz ⓘ |
| SPTpolFrequencyBands |
150 GHz
ⓘ
95 GHz ⓘ |
| surfaceAccuracy | tens of microns ⓘ |
| telescopeDiameter | 10 meters ⓘ |
| wavelengthRange |
millimeter
ⓘ
submillimeter ⓘ |
Referenced by (4)
Full triples — surface form annotated when it differs from this entity's canonical label.