Measurements of the CIB power spectra from Planck Collaboration XXX (2014), Viero et al. (2013), and Lenz et al. (2019). The best-fit models shown in this figure are obtained when Planck and Herschel data are fit separately. The SPIRE data have been rescaled to Planck data using the cross-calibration factor derived in Bertincourt et al. (2016) and the factor that allows converting the measurement through the SPIRE bandpass into a measurement as it would be obtained through the Planck bandpass from Lagache et al. (2020). Overall, .