Chapters
- Relevant source populations
- Strongly lensed high-z galaxies
- Proto-clusters of galaxies
- Source polarization
Abstract
| I
will discuss the potential of next generation Cosmic Microwave
Background (CMB) experiments for studies of extragalactic sources,
starting from what we learned from the Planck mission. The
substantially better angular resolution foreseen for projects like
CORE, PICO, CMB-S4 translates into substantially fainter detection
limits. This will not only boost by large factors the number of
detections but will also make possible entirely new science such as:
the detection of thousands of high-z extreme strongly gravitationally
lensed galaxies; the direct detection of large samples of galaxy
proto-clusters up to z~4; the study of the evolution of the
star-formation in virialized groups and clusters of galaxies; the study
of the polarization properties of large samples of radio sources and,
for the first time, of dusty galaxies at mm and sub-mm wavelengths. |
Bibliography
- Articles
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al. 2016. Exploring Cosmic Origins with CORE: Extragalactic sources in
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- Negrello, M., et al.
2017. The Herschel-ATLAS: a sample of 500 micron-selected lensed
galaxies over 600 sq. deg.. MNRAS 465, 3558.
- Negrello, M., et al.
2017. On the statistics of proto-cluster candidates detected in the
Planck all-sky survey. MNRAS 470, 2253.
- Planck Collaboration
2016. Planck 2015 results. XXVI. The Second Planck Catalogue of Compact
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- Planck Collaboration
2016. Planck intermediate results. XXXIX. The Planck list of
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