SPT-3G camera
E651441
The SPT-3G camera is a third-generation, highly sensitive receiver on the South Pole Telescope designed to map the cosmic microwave background with improved resolution and polarization measurements.
Statements (46)
| Predicate | Object |
|---|---|
| instanceOf |
cosmic microwave background instrument
ⓘ
polarization-sensitive camera ⓘ telescope receiver ⓘ |
| collaboratingInstitution |
Argonne National Laboratory
NERFINISHED
ⓘ
Canadian Institute for Advanced Research NERFINISHED ⓘ Fermi National Accelerator Laboratory NERFINISHED ⓘ Kavli Institute for Cosmological Physics NERFINISHED ⓘ McGill University NERFINISHED ⓘ National Science Foundation NERFINISHED ⓘ University of California, Berkeley NERFINISHED ⓘ University of California, Davis NERFINISHED ⓘ University of Chicago NERFINISHED ⓘ |
| designedFor |
CMB polarization measurements
ⓘ
CMB temperature anisotropy mapping ⓘ high-resolution CMB surveys ⓘ |
| environment |
extreme cold temperatures
ⓘ
high atmospheric stability at the South Pole ⓘ |
| follows | SPTpol NERFINISHED ⓘ |
| generation | third-generation receiver for the South Pole Telescope ⓘ |
| hasImprovementOver |
SPT-SZ camera
NERFINISHED
ⓘ
SPTpol NERFINISHED ⓘ |
| hasProperty |
high sensitivity
ⓘ
large number of detectors ⓘ multi-frequency capability ⓘ polarization sensitivity ⓘ |
| hostTelescope | South Pole Telescope NERFINISHED ⓘ |
| locatedAt | South Pole NERFINISHED ⓘ |
| locatedIn |
Amundsen–Scott South Pole Station
NERFINISHED
ⓘ
Antarctica ⓘ |
| mountedOn | 10-meter South Pole Telescope NERFINISHED ⓘ |
| observes | cosmic microwave background ⓘ |
| observingStrategy |
deep, high-sensitivity fields
ⓘ
wide-area CMB survey ⓘ |
| partOf | South Pole Telescope NERFINISHED ⓘ |
| scienceGoal |
constraints on dark energy
ⓘ
constraints on neutrino masses ⓘ improved measurements of CMB polarization ⓘ mapping large-scale structure via CMB lensing ⓘ search for primordial B-mode polarization ⓘ |
| successorTo | SPTpol receiver NERFINISHED ⓘ |
| telescopeType | ground-based CMB telescope receiver ⓘ |
| usedFor |
cosmological parameter estimation
ⓘ
galaxy cluster detection via the Sunyaev–Zel’dovich effect ⓘ studies of inflationary gravitational waves ⓘ tests of ΛCDM cosmology ⓘ weak gravitational lensing of the CMB ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.