# Data Releases

**NOTE: **Data releases from specific analyses (e.g., bandpowers and covariances from power spectrum analyses, catalogs from galaxy cluster and point-source analyses) are linked along with the publications for those analyses below. These data are all also hosted at NASA's Legacy Archive for Microwave Background Data (LAMBDA) website.

## Data Releases

"CMB/kSZ and Compton-y Maps from 2500 square degrees of SPT-SZ and Planck Survey Data", ApJ submitted, arXiv:2102.05033 [Data Products]

"Maps of the Southern Millimeter-wave Sky from Combined 2500 square-degree SPT-SZ and Planck Temperature Data",

*ApJS 239 (2018) 10, arXiv:1803.10682*[Data Products]"Maps of the Magellanic Clouds from Combined South Pole Telescope and Planck Data",

*ApJS 227 (2016) 23, arXiv:1605:00966*

[Data Products]"SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey",

*ApJS 227 (2016) 3, arXiv:1609.05211*[Data Products]"The First Public Release of South Pole Telescope Data: Maps of a 95 deg^2 Field from 2008 Observations",

*ApJ 743 (2011) 90, arXiv:1111:7245*[Data Products]

## Bandpowers and Catalogs

"Constraints on Î›CDM Extensions from the SPT-3G 2018 EE and TE Power Spectra" and "Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data",

*PRD,**submitted,**arXiv:2103.13618,**arXiv:**2101.01684*[Associated Data]"Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol",

*PRD 102 (2020) 083504, arXiv:2006.08061*[Associated Data]"Millimeter-wave Point Sources from the 2500-square-degree SPT-SZ Survey: Catalog and Population Statistics",

*ApJ 900 (2020) 55, arXiv:2003.03431*[Associated Data]"An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys",

*ApJ**908 (2021) 199**, arXiv:2002.06197*[Associated Data]"Constraints on Cosmological Parameters from the 500 deg2 SPTpol Lensing Power Spectrum",

*ApJ 888 (2020) 119, arXiv:1910.07157*[Associated Data]"Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data",

*PRD 101 (2020) 122003, arXiv:1910.05748*[Associated Data]"The SPTpol Extended Cluster Survey",

*ApJS 247 (2020) 25, arXiv:1910.04121*[Associated Data]"A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg$^2$ of SPTpol Temperature and Polarization Data",

*ApJ 884 (2019) 70, arXiv:1905.05777*[Associated Data]"Measuring Cross-Spectra of the Cosmic Infrared Background from 95 to 1200 GHz",

*ApJ 881 (2019) 96, arXiv:1810.10643*

"Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol data",

*ApJ 852 (2018) 97, arXiv:1707.09353*[Associated Data]"A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data",

*ApJ 849 (2017) 124, arXiv:1705.00743*[Associated Data]"Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data",

*ApJ 807 (2015), 151, arXiv:1503.02315*[Associated Data]"Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data",

*ApJ 805 (2015), 36, arXiv:1411.1042*[Associated Data]"Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ Survey",

*ApJS 216 (2015), 27, arXiv:1409.0850*[Associated Data]"A measurement of secondary cosmic microwave background anisotropies from the 2500-square-degree SPT-SZ survey",

*ApJ 799 (2015), 177, arXiv:1408.3161*[Associated Data]"Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope",

*PRL 111 (2013) 141301, arXiv:1307.5830*[Associated Data]"Extragalactic millimeter-wave point source catalog, number counts and statistics from 771 square degrees of the SPT-SZ Survey",

*ApJ 779 (2013) 61, arXiv:1306.3470*[Associated Data]"A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data",

*ApJ 784 (2014) 143, arXiv:1303.3535*[Associated Data]"Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500-square-degree SPT-SZ survey",

*ApJ 782 (2014) 74, arXiv:1212.6267*[Associated Data]"A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey",

*ApJ 779 (2013) 86, arXiv:1210.7231*[Associated Data]"A measurement of gravitational lensing of the microwave background using South Pole Telescope data",

*ApJ 756 (2012) 142, arXiv:1202.0546*[Associated Data]"Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey",

*ApJ 763 (2013) 147, arXiv:1112.5435*[Associated Data]"A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations",

*ApJ 755 (2012) 70, arXiv:1111.0932*[Associated Data]"A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope",

*ApJ 743 (2011) 28, arXiv:1105.3182*[Associated Data]"Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data",

*ApJ 736 (2011) 61, arXiv:1012.4788*[Associated Data]"Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations",

*ApJ 722 (2010) 1180, arXiv:1003.0003*"Measurements of Secondary Cosmic Microwave Background Anisotropies with the South Pole Telescope",

*ApJ 719 (2010) 1045, arXiv:0912.4317*[Associated Data]"Angular Power Spectra of the Millimeter Wavelength Background Light from Dusty Star-forming Galaxies with the South Pole Telescope",

*ApJ 718 (2010) 632, arXiv:0912.4315*[Associated Data]"Extragalactic point sources in South Pole Telescope survey data: source counts, catalog, and statistics for an 87 square-degree field",

*ApJ 719 (2010) 763, arXiv:0912.2338*[Associated Source Catalog and Number Counts]