Campuses:
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| sept._13_2017 [2017/09/27 08:35] – created nbatta | sept._13_2017 [2017/10/09 19:34] (current) – hanany | ||
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| Clusters (Nick) | Clusters (Nick) | ||
| - | Note: fsky for these forecast was 0.7 | ||
| + | Cluster numbers for the probe with and without 555 GHz and greater. __Note: fsky for these forecast was 0.7__ | ||
| + | |||
| + | **With 555 GHz and above:** | ||
| + | |||
| + | Full CMB probe w/ LSST WL mass calibration + Planck tau: | ||
| + | # clusters ~27200 | ||
| + | |||
| + | Mnu 1-sigma : 29.3 meV | ||
| + | |||
| + | w0 1-sigma : 5.08 % | ||
| + | |||
| + | wa 1-sigma : 0.25 | ||
| + | |||
| + | **Only up to (and excluding?) 555 GHz** | ||
| + | |||
| + | Full CMB probe w/ LSST WL mass calibration + Planck tau | ||
| + | |||
| + | # clusters ~24600 | ||
| + | |||
| + | Mnu 1-sigma : 30.0 meV | ||
| + | |||
| + | w0 1-sigma : 5.35 % | ||
| + | |||
| + | wa 1-sigma : 0.26 | ||
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| + | Please note that the foregrounds in these forecasts are stochastic and not correlated, so to see the real impact of the these higher frequencies we need to include correlated foregrounds. Furthermore we can update the tau constraints to include CMB-Probe estimates which should be close to CV limited. | ||
| Other Business: | Other Business: | ||