Unbinned EE spectrum for 2 ≤ ℓ ≤ 30 and binned EE spectrum for 31 ≤ ℓ < 301. The binned EE spectrum is available using two different bin widths: Δℓ=10 and Δℓ=18. More...
Jupyter notebook describing CLASS implementation of conversion from thermodynamic
temperature to antenna temperature, including terms for color correction of a
power-law SED and thermodynamic to Rayleigh-Jeans unit conversion. More...
Code that allows for quick interpolation between Cosmic Microwave Background polarized power spectra as a function of scalar fluctuations, tensor fluctuations, and the optical depth to reionization. More...