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| Both sides previous revisionPrevious revisionNext revision | Previous revision |
| nov._22_2017 [2017/11/22 08:58] – nbatta | nov._22_2017 [2017/11/22 09:15] (current) – nbatta |
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| The STM is here [[start:stm|Science Traceability Matrix]] | The STM is here [[start:stm|Science Traceability Matrix]] |
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| | Legacy Catalogs |
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| | | Catalog | Impact | Science | |
| | ^ proto-clusters | Thousands of proto-clusters selected homogeneously, compared to heterogeneous samples of a few ^ galaxy cluster formation, early ICM properties, ... ^ |
| | | Lensed Point sources | 3,000 rare highly magnified dusty sources compared to ~10s sources found by Planck | sub-structure, high-z star formation,... | |
| | | High-z galaxy clusters | ~ 100s of virialized clusters and z >~ 2 | galaxy formation in dense environments at the peak of star formation for most cluster galaxies, ICM,... | |
| | | Polarized Point Sources | Direct counts in polarization both for radio sources and for dusty galaxies (1st time) | | |
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| AOB | AOB |
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| __Minutes__ | __Minutes__ |