SPT-3G survey

E651443

The SPT-3G survey is a cosmic microwave background observation program using the third-generation camera on the South Pole Telescope to map the sky with high sensitivity and resolution for cosmology research.

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Statements (45)

Predicate Object
instanceOf astronomical survey
cosmic microwave background survey
aimsTo constrain cosmological parameters
detect galaxy clusters via the Sunyaev–Zel’dovich effect
map the microwave sky with high angular resolution
map the microwave sky with high sensitivity
measure polarization anisotropies of the CMB
measure temperature anisotropies of the CMB
probe neutrino properties
study large-scale structure via CMB lensing
test models of dark energy
test models of inflation
benefitsFrom low atmospheric water vapor at South Pole
collaboration South Pole Telescope collaboration NERFINISHED
country Antarctica NERFINISHED
dataType CMB polarization maps
CMB temperature maps
millimeter-wave sky maps
environment high, dry Antarctic plateau
field astrophysics
cosmology
goal produce high signal-to-noise CMB maps for cosmology research
hostFacility South Pole Telescope facility NERFINISHED
hostTelescopeAperture 10-meter dish
location Amundsen–Scott South Pole Station NERFINISHED
South Pole NERFINISHED
observes cosmic microwave background
observingSiteAltitude ~2800 meters
predecessor SPT-SZ survey NERFINISHED
SPTpol survey NERFINISHED
relatedProject SPT-3G experiment NERFINISHED
scienceCategory CMB lensing
cluster cosmology
large-scale structure
neutrino cosmology
secondary CMB anisotropies
scienceCategory dark energy studies
inflationary cosmology
skyCoverage wide-area southern sky survey
startEra late 2010s
surveyType ground-based CMB survey
telescopeGeneration third-generation camera
usesInstrument SPT-3G camera
usesTelescope South Pole Telescope NERFINISHED
wavelengthBand millimeter

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

South Pole Telescope associatedSurvey SPT-3G survey