Combined Cosmology Programs with SPIRE and Planck HFI

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Cosmology: Galaxy Clusters, Star Formation, Missions: First, Planck

Scientific paper

The early-release Planck sub-millimeter all-sky survey will detect galaxies at significant cosmological distances, including a fraction that may be gravitationally lensed. Follow-up spectral line surveys with SPIRE will determine the redshift and will probe the interstellar medium in these extremely far-infrared luminous galaxies. Spectral and imaging observations of clusters of galaxies, detected by Planck via the Sunyaev-Zel'dovich effect, may assess relativistic corrections to the S-Z distortion, and probe the contribution from thermal dust emission. Finally, the evolution and clustering of galaxies at high redshift may be probed by fluctuations in the extra-galactic far-infrared background. A P(D) analysis with a deep SPIRE survey will probe the far-infrared background at higher sensitivity and angular resolution over a smaller region of sky, complementing proposed studies of the far-infrared background with Planck.

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