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

• Published in: The Astrophysical Journal
• Main Authors: Viero, M. P., Crites, A. T., Moncelsi, L., Serra, P.
• Format: Article in Journal/Newspaper
• Language: English
• Published: American Astronomical Society 2019
• Subjects: South Pole; South pole
• Online Access: https://authors.library.caltech.edu/97945/; https://authors.library.caltech.edu/97945/1/Viero_2019_ApJ_881_96.pdf; https://authors.library.caltech.edu/97945/2/1810.10643.pdf; https://resolver.caltech.edu/CaltechAUTHORS:20190816-101819572

We present measurements of the power spectra of cosmic infrared background (CIB) and cosmic microwave background (CMB) fluctuations in six frequency bands. Maps at the lower three frequency bands, 95, 150, and 220 GHz (3330, 2000, and 1360 μm) are from the South Pole Telescope, while the upper three frequency bands, 600, 857, and 1200 GHz (500, 350, 250 μm) are observed with Herschel/SPIRE. From these data, we produce 21 angular power spectra (6 auto- and 15 cross-frequency) spanning the multipole range 600 ≤ ℓ≤ 11,000. Our measurements are the first to cross-correlate measurements near the peak of the CIB spectrum with maps at 95 GHz, complementing and extending the measurements from Planck Collaboration et al. at 143–857 GHz. The observed fluctuations originate largely from clustered, infrared-emitting, dusty star-forming galaxies, the CMB, and to a lesser extent radio galaxies, active galactic nuclei, and the Sunyaev–Zel'dovich effect.