The combined data maps, in Healpix format, with resolution parameter Nside = 8192. The maps are in Equatorial coordinates, and in RING ordering. The resolution is 1.85 arcmin. They can be easily read using the healpy read_map function.

Five combined null maps for each band (15 maps in total), in the same format as the combined data maps. These maps should contain no astrophysical signal but have the same noise properties as the data.

The two-dimensional filter M_lm. These are double precision real arrays, and are indexed the same as the alm arrays. The alms for each frequency band have been multiplied by their corresponding filters (indicated by the filenames).

One SPT-SZ data map for each band, in the same Healpix format as the other maps described above. These are the same maps that we combine with Planck data. They have been multiplied by the appropriate calibration factors to convert to units of uK_CMB. The resolution of these maps is described by a Gaussian with FWHM equal to 1.75 arcmin (slightly different from the combined data maps). The SPT filter response has not been deconvolved from these maps. Bright sources have not been masked from these maps. Only a boundary mask was applied.

Half-depth SPT-SZ data maps (2 maps for each band). These are produced by splitting the observations into two sets with independent noise. These have the same resolution, mask, and format as the SPT data maps.

The filter transfer functions (t_lm as described in the paper) for each SPT-SZ data map, up to lmax = 10000. These are stored in the same way as the combined data a_lm files. Note that t_lm does not include the 1.75 arcmin Gaussian beam.

Data products related to the cosmological parameter analysis of the SPT+Planck 2500 square-degrees lensing measurement presented in Simard et al. (2017), based on results presented in Omori et al. (2017) More...

Data products associated with the SPT measurement of the millimeter-wavelength anisotropy power spectra described in George et al. (2014) arXiV:1408.3161. More...

These files contain the statistical-only, systematic-only, and statistical-plus-systematic parameter covariance matrices for each level of cluster masking. More...

These files contain realizations of the SPT beam used in constructing the systematic error covariance matrix described in Section 4.2.1 of Crawford et al.(2013). More...

These files contain the predicted thermal SZ bispectrum for three different levels of cluster cuts (no clusters cut, clusters above M200(rho_crit)=8e14 Msun/h cut, and clusters above M200(rho_crit)=3e14 Msun/h cut). More...

These files contain the bispectrum measurements and associated covariance matrices (statistical only) at 95, 150, and 220 GHz from 2008+2009 observations. More...

The data files and updated CMBlikes.f90 file necessary to incorporate the SPT likelihood in current versions of CosmoMC can be found here in a gzipped tarball. The included README has instructions. More...

These are the SPT 150 GHz Bandpowers from 2008 to 2011 observations. The bandpowers cover the multipole range 650 < ell < 3000 in bins of delta-ell = 50. More...