SPT-3G Data Products

2018 Likelihood

We provide files in a zip archive here that can be added to the June 2021 version of CosmoMC to interface with the SPT-3G 2018 TT/TE/EE bandpowers discussed above. These files include the SPT-3G likelihood, SPT-3G data (multi-frequency bandpowers, covariance matrix, band power window functions, beam covariance, effective band centres, and calibration covariance), batch file, a sample .ini file, the baseline priors on foreground parameters, a proposal matrix for LCDM assuming the baseline priors, and a README with instructions for how to compile CosmoMC with the SPT-3G 2018 TT/TE/EE likelihood. If you have any questions regarding the use of this likelihood, please contact Lennart Balkenhol (lbalkenhol_at_student_dot_unimelb_dot_edu_dot_au).

Additional Details:

  • Information on this page was taken from this SPT site
  • Balkenhol et al.(2022), "Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set
    from SPT-3G 2018 Data”, arXiv:2212.05642

A service of the HEASARC and of the Astrophysics Science Division at NASA/GSFC
Goddard Space Flight Center, National Aeronautics and Space Administration
HEASARC Director: Dr. Andrew F. Ptak
LAMBDA Director: Dr. Thomas M. Essinger-Hileman
NASA Official: Dr. Thomas M. Essinger-Hileman
Web Curator: Mr. Michael R. Greason