… Planck 2015 likelihoods, statistical descriptions of the 2-point correlationfunctions of the cosmic
microwave background (CMB) … , ie, a pixel-based likelihood at low multipoles (ℓ< 30) and …

… This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point
correlation functions of the cosmic microwave background (CMB) temperature and polarization …

… We further validate the robustness of the likelihood results … power spectra of the cosmic
microwave background (CMB) … fix all parameters that are not sampled to their Planck 2015 …

… Planck 2015 likelihoods, statistical descriptions of the 2-point correlationfunctions of the cosmic
microwave background (CMB… , ie, a pixel-based likelihood at low multipoles (ℓ < 30) and …

… We use Planck baseline best-fit power spectrum to Planck 2015 TT and … power spectra at
all multipoles without interpolation. We use publicly available Planck 2015 data and likelihood …

… infer the CMB power spectrum and the BipoSH spectrum in a … The robustness of analysis
for different choices of prior has been … , with the canonical values known from the CMB dipole …

… We find that Planck TT best fit ΛCDM power spectrum is … we will use EE + lowTEB likelihood,
but when we compare TT + … parameters and the primordial power spectrum parameters to …

… We use the 2015 Planck likelihood in combination with the Bicep2/Keck likelihood (BKP …
other cosmological parameters; furthermore, in the same section we provide forecast for future …

… in wave number, using both CMB data from the Planck satellite and LSS data from the … the
new oscillation parameters (amplitude, frequency and phase), both CMB-only and CMB + LSS …

… on cosmological parameters obtained with the Planck 2015 po… In addition, we investigate
the robustness of the cosmological … the Planck maps and the sky region for the power spectra …