SPTpol camera

E651440

The SPTpol camera is a highly sensitive polarization-sensitive receiver used on the South Pole Telescope to measure the polarization of the cosmic microwave background for cosmological studies.

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Predicate Object
instanceOf cosmic microwave background instrument
polarization-sensitive receiver
commissionedOn early 2010s
contributesTo constraints on inflationary models
precision cosmology
tests of ΛCDM cosmological model
dataUsedFor CMB lensing reconstruction
CMB power spectrum measurements
cluster cosmology via Sunyaev–Zel’dovich effect
designedFor cosmological studies
designedTo measure polarization of the cosmic microwave background
enablesMeasurement CMB polarization power spectra
temperature–polarization cross-correlation
environment operates in extreme Antarctic conditions
followedBy SPT-3G camera NERFINISHED
hasArrayConfiguration focal plane array of bolometers
hasDetectorType polarization-sensitive bolometers
hasKeyFeature high angular resolution
high sensitivity to polarization
multi-frequency capability
hasObservationBand 150 GHz
90 GHz
locatedAt Amundsen–Scott South Pole Station NERFINISHED
locatedOn Antarctic Plateau NERFINISHED
mountedOn 10-meter South Pole Telescope NERFINISHED
observes southern sky
operatedBy South Pole Telescope collaboration NERFINISHED
University of Chicago NERFINISHED
collaboration of multiple international institutions
operationalStatus superseded by SPT-3G for primary observations
replacedInstrument original SPT-SZ camera
scienceGoal constrain cosmological parameters
improve constraints on neutrino masses
measure CMB E-mode polarization
measure small-scale CMB anisotropy
search for signatures of inflation in CMB polarization
study dark energy through CMB measurements
study large-scale structure via CMB lensing
sensitiveTo CMB polarization
CMB temperature anisotropy
telescopeType ground-based CMB telescope
usedOn South Pole Telescope NERFINISHED
usesDetectorTechnology transition-edge sensor bolometers

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South Pole Telescope instrument SPTpol camera