Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revisionNext revision | Previous revision |
nov._22_2017 [2017/11/22 08:55] – nbatta | nov._22_2017 [2017/11/22 09:15] (current) – nbatta |
---|
| |
STM update (Nick) | STM update (Nick) |
| |
| The STM is here [[start:stm|Science Traceability Matrix]] |
| |
| Legacy Catalogs |
| |
| | 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) | | |
| |
AOB | AOB |
| |
__Minutes__ | __Minutes__ |