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., Reichardt, C.L., Benson, B.A., Bleem, L.E., Bock, J., Carlstrom, J.E., Chang, C.L., Cho, H-M., Crawford, T.M., Crites, A.T., de Haan, T., Dobbs, M.A., Everett, W.B., George, E.M., Halverson, N.W., Harrington, N.L., Holder, G., Holzapfel, W.L., Hou, Z., Hrubes, J.D., Knox, L., Lee, A.T., Luong-Van, D., Marrone, D.P., Mcmahon, J.J., Meyer, S.S., Millea, M., Mocanu, L.M., Mohr, J.J., Moncelsi, L., Padin, S., Pryke, C., Ruhl, J.E., Schaffer, K.K., Serra, P., Shirokoff, E., Staniszewski, Z., Stark, A.A., Story, K.T., Vanderlinde, K., Vieira, J.D., Williamson, R., Zemcov, M.
• Other Authors: Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES)
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 2019
• Subjects: [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; South Pole; South pole
• Online Access: https://hal.science/hal-01914656; https://doi.org/10.3847/1538-4357/ab2da0

International audience 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, 1360 $\mu$m) are from the South Pole Telescope, while the upper three frequency bands, 600, 857, and 1200 GHz (500, 350, 250 $\mu$m) are observed with Herschel/SPIRE. From these data, we produce 21 angular power spectra (six auto- and fifteen cross-frequency) spanning the multipole range $600 \le \ell \le 11,000$. 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. (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 extent radio galaxies, active galactic nuclei, and the Sunyaev-Zel'dovich effect.