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We present measurements of the power spectra of cosmic infrared background(CIB) and cosmic microwave background (CMB) fluctuations in six frequencybands. Maps at the lower three frequency bands, 95, 150, and 220 GHz (3330,2000, 1360 $\mu$m) are from the South Pole Telescope, while the upper threefrequency bands, 600, 857, and 1200 GHz (500, 350, 250 $\mu$m) are observedwith Herschel/SPIRE. From these data, we produce 21 angular power spectra (sixauto- and fifteen cross-frequency) spanning the multipole range $600 \le \ell\le 11,000$. Our measurements are the first to cross-correlate measurementsnear the peak of the CIB spectrum with maps at 95 GHz, complementing andextending the measurements from Planck Collaboration et al. (2014) at 218, 550,and 857 GHz. The observed fluctuations originate largely from clustered,infrared-emitting, dusty star-forming galaxies, the CMB, and to a lesser extentradio galaxies, active galactic nuclei, and the Sunyaev-Zel'dovich effect.

Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz