The 10 Meter South Pole Telescope
arXiv:0907.4445 · doi:10.1086/659879
Abstract
The South Pole Telescope (SPT) is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, multi-color, millimeter-wave, bolometer camera. It is located at the Amundsen-Scott South Pole station in Antarctica. The design of the SPT emphasizes careful control of spillover and scattering, to minimize noise and false signals due to ground pickup. The key initial project is a large-area survey at wavelengths of 3, 2 and 1.3 mm, to detect clusters of galaxies via the Sunyaev-Zeldovich effect and to measure the small-scale angular power spectrum of the cosmic microwave background (CMB). The data will be used to characterize the primordial matter power spectrum and to place constraints on the equation of state of dark energy. A second-generation camera will measure the polarization of the CMB, potentially leading to constraints on the neutrino mass and the energy scale of inflation.
47 pages, 14 figures, updated to match version to be published in PASP 123 903 (May, 2011)
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- Maps of the Magellanic Clouds from Combined South Pole Telescope and Planck Data
- Probing Oort clouds around Milky Way stars with CMB surveys
- Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
- Feeding and feedback processes in the Spiderweb proto-intracluster medium
- Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
- Consistency of cosmic microwave background temperature measurements in three frequency bands in the 2500-square-degree SPT-SZ survey
- Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
- Source structure and molecular gas properties from high-resolution CO imaging of SPT-selected dusty star-forming galaxies
- Asteroid Measurements at Millimeter Wavelengths with the South Pole Telescope
- The Evolution of AGN Activity in Brightest Cluster Galaxies
- The infrared-luminous progenitors of high-z quasars
- The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
- An Implementation of a Channelizer based on a Goertzel Filter Bank for the Read-Out of Cryogenic Sensors
- Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
- Broadband, millimeter-wave antireflection coatings for large-format, cryogenic aluminum oxide optics
- Galaxy cluster scaling relations measured with APEX-SZ
- SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
- Probing the time variation of fine structure constant using galaxy clusters and quintessence model
- Flaring Stars in a Non-targeted mm-wave Survey with SPT-3G
- Observational constrained Weyl type gravity cosmological model and the dynamical system analysis
- Search for GeV Gamma-Ray Emission from SPT-SZ selected Galaxy Clusters with 15 years of Fermi-LAT data
- Optimization and analysis of code-division multiplexed TES microcalorimeters
- The PSZ-MCMF catalogue of Planck clusters over the DES region
- XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
- Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
- Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
- Note on Structure Formation from Cosmic String Wakes
- An X-ray Detection of Star Formation In a Highly Magnified Giant Arc
- Order statistics applied to the most massive and most distant galaxy clusters
- Kinematic analysis of galaxies in the SPT234956 protocluster core
- Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300
- The 1.4 mm core of Centaurus A: First VLBI results with the South Pole Telescope
- Recent developments in astrophysical and cosmological exploitation of microwave surveys
- Clusters of Galaxies Masquerading as X-Ray Quasars
- Galaxy populations in the most distant SPT-SZ clusters -- II. Galaxy structural properties in massive clusters at 1.4<z<1.7
- SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
- CMB Telescopes and Optical Systems
- Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
- Mass-Richness relations for X-ray and SZE-selected clusters at as seen by at 4.5m
- Pairwise kSZ signal extraction efficacy and optical depth estimation
- Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring State
- A model-independent test of the evolution of gas depletion factor for SPT-SZ and Planck ESZ clusters
- Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
- New Identifications and Multi-wavelength Properties of Extragalactic Fermi Gamma-Ray Sources in the SPT-SZ Survey Field
- CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
- Characterization and performance of the second-year SPT-3G focal plane
- Observation and Confirmation of Nine Strong Lensing Systems in Dark Energy Survey Year 1 Data
- Increasing the census of L and T dwarfs in wide binary and multiple systems using Dark Energy Survey DR1 and Gaia DR2 data
- Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
- On the modelling of the excesses of galaxy clusters over high-mass thresholds
- Spherical collapse in coupled quintessence with a CDM background
- The Greenland Telescope: Antenna Retrofit Status and Future Plans
- SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
- The spectral energy distribution of galaxies at z > 2.5: Implications from the Herschel/SPIRE color-color diagram
- The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at
- Unveiling the Universe with Emerging Cosmological Probes
- Freeform three-mirror anastigmatic large-aperture telescope and receiver optics for CMB-S4
- Euclid preparation LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey
- A Large Molecular Gas Reservoir in the Protocluster SPT234956 at
- Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel'dovich effect
- A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population
- Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
- Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
- Fabrication of a Monolithic 5-Meter Aluminum Reflector for Millimeter-Wavelength Observations of the Cosmic Microwave Background
- Cosmoglobe DR1. III. First full-sky model of polarized synchrotron emission from all WMAP and Planck LFI data
- Extremely-bright submillimeter galaxies beyond the Lupus-I star-forming region
- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
- DES Science Portal: Creating Science-Ready Catalogs
- RF-ICE: large-scale gigahertz readout of frequency-multiplexed microwave kinetic inductance detectors
- The LABOCA/ACT Survey of Clusters at All Redshifts: multi-wavelength analysis of background submillimeter galaxies
- Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
- The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue
- Probing the dynamical and X-ray mass proxies of the cluster of galaxies Abell S1101
- A fast map-making preconditioner for regular scanning patterns
- Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
- The Greenland Telescope (GLT): Antenna status and future plans
- Study on the filters of atmospheric contamination in ground based CMB observation
- Design and performance of a multi-terahertz Fourier transform spectrometer for axion dark matter experiments
- Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO
- Evidence for AGN-Regulated Cooling in Clusters at : A Multi-Wavelength View of SPT-CL J0607-4448
- A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
- A Massive Molecular Gas Reservoir in the z=2.221 Type-2 Quasar Host Galaxy SMM J0939+8315 Lensed by the Radio Galaxy 3C220.3
- Clustering of red and blue galaxies around high-redshift 3C radio sources as seen by the Hubble Space Telescope
- Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
- Biasing and Demodulation Firmware for Kilopixel TES Bolometer Arrays
- Lensing Noise in mm-wave Galaxy Cluster Surveys
- The Cold Dust Content of the Nearby Galaxies IC 5325, NGC 7496, NGC 7590, and NGC 7599
- Future constraints on variations of the fine structure constant from combined CMB and weak lensing measurements
- Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
- Filtering in CMB data analysis with application to ACT DR4 and Planck observations
- A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields
- kSZ Pairwise Velocity Reconstruction with Machine Learning
- Demonstration of Weak-Link Physics in the Dynamical Response of Transition-Edge Sensors
- Self-supervised component separation for the extragalactic submillimeter sky
- Cross-correlating radial peculiar velocities and CMB lensing convergence
- SPT-3G secondary mirror geometry
- Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
- The Atacama Cosmology Telescope: Systematic Transient Search of Single Observation Maps
- Infrared galaxies detected by the Atacama Cosmology Telescope
- A Stacked Analysis of GeV Gamma-Ray Emission from SPT-SZ Galaxy Clusters with 16 Years of Fermi-LAT Data
- Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning
- Bright [CII]158m Streamers as a Beacon for Giant Galaxy Formation in SPT234956 at
- A VLBI receiving system for the South Pole Telescope
- VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
- CMB delensing with deep learning
- Demonstration of wideband metal mesh filters for submillimeter astrophysics using flexible printed circuits
- Radio observations of Planck clusters
- Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
- ComPACT: ACT+Planck galaxy cluster catalogue
- Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
- Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
- Optical and Near-IR Microwave Kinetic Inductance Detectors (MKIDs) in the 2020s
- Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
- Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
- The gas distribution in the high-redshift cluster MS 1054-0321
- Broadband anti-reflection coating for sub-terahertz optics using dielectric multilayers
- Ultra-Thin Large-Aperture Vacuum Windows for Millimeter Wavelengths Receivers
- Cluster optical depth and pairwise velocity estimation using machine learning
- Atacama Cosmology Telescope: Observations of supermassive black hole binary candidates. Strong sinusoidal variations at 95, 147 and 225 GHz in PKS 2131021 and PKS J08050111
- Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect
- Implications of scattering for CMB foreground emission modelling
- The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10
- Pressure profiles of distant Galaxy clusters with Planck-SPT data
- The Atacama Cosmology Telescope: Machine Learning Driven Tools for Detecting Millimeter Sources in Timestream Pre-processing
- The Simons Observatory: HoloSim-ML: machine learning applied to the efficient analysis of radio holography measurements of complex optical systems
- Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf
- The Design and Integrated Performance of SPT-3G
- High frequency radio SEDs and polarization fractions of sources in an ACT survey field
- Towards including super-sample covariance in the unbinned likelihood for cluster abundance cosmology
- A Serverless Architecture for Efficient and Scalable Monte Carlo Markov Chain Computation
- Probing the evolution of galaxy clusters with the SZ Effect
- Combining Planck and SPT cluster catalogs: cosmological analysis and impact on Planck scaling relation calibration
- SZ effect or Not? - Detecting most galaxy clusters' main foreground effect
- Artificial Broadcasts as Galactic Populations: III. Constraints on Radio Broadcasts from the Cosmic Population of Inhabited Galaxies