Goodness-of-fit tests for the 2018 Planck temperature and polarization spectra.
|TT, full, binned …||30–2508||−380.34||760.68||765||0.54|
|TE, full, binned …||30–1996||−428.68||857.36||762||0.0090|
|EE, full, binned …||30–1996||−371.48||742.96||762||0.68|
|TTTEEE, full, binned …||30–2508||−1172.47||2344.94||2289||0.20|
|TT, coadded, unbinned …||30–2508||−1274.57||2549.14||2479||0.16|
|TE, coadded, unbinned …||30–1996||−1035.77||2071.54||1967||0.050|
|EE, coadded, unbinned …||30–1996||−1028.55||2057.10||1967||0.077|
|TTTEEE, coadded, unbinned …||30–2508||−3328.51||6657.02||6413||0.016|
|Low-ℓ TT (Commander) …||2–29||−11.63||23.25||27||...|
|Low-ℓ EE (SimAll) …||2–29||−198.02||...||27||...|
Notes. The reference model is our best-fit base-ΛCDM cosmology from the Planck TT,TE,EE+lowE+lensing likelihood combination. The first set of rows show the results for the full binned Plik high-ℓ likelihood, while the second set of rows show the results from the coadded, unbinned CMB high-ℓ spectra. The last two rows show the results for the low-ℓ TT and low-ℓ EE likelihoods. The effective χ2 is defined as χeff = −2log(ℒ). The number of degrees of freedom (Ndof) is set equal to the number of multipoles. The last column lists the probability to exceed (PTE). The log(ℒ) value for the low-ℓ EE likelihood is normalized up to an arbitrary additive constant and so further entries are not shown in this case. Similarly, the non-Gaussian nature of the low-ℓ TT likelihood precludes us from displaying a PTE in this case.
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