Campuses:
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| private:teleconsnotes20171004 [2017/10/09 16:01] – hanany | private:teleconsnotes20171004 [2017/10/09 16:04] (current) – hanany | ||
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| since there was no time to discuss them, and I didn't include the numbers in the slides, I just thought I would send an update here. Some of the numbers relevant for the STM I find for the strawperson are (the numbers are the uncertainty on the parameter) | since there was no time to discuss them, and I didn't include the numbers in the slides, I just thought I would send an update here. Some of the numbers relevant for the STM I find for the strawperson are (the numbers are the uncertainty on the parameter) | ||
| - | ^ | + | | | 55 % |
| - | | | + | | ns |
| - | | ns| 0.0015|0.0012| | + | | tau | 0.0021 |
| - | |tau| 0.0021|0.0018| | + | | n_run | 0.0024 |
| - | |n_run|0.0024|0.002| | + | | N_eff | 0.039 |
| - | |N_eff|0.039| 0.033| | + | | m_nu |
| - | |m_nu|43 meV|36 meV | | + | |Omega_k | 0.0018 |
| - | Omega_k| 0.0018 | 0.0015| | + | |
| Neutrino mass does not include DESI BAO prior here. I should get in touch with Nick to see if we can provide a joint constraint on neutrino mass from lensing and clusters internal to the probe. It seems one can get interesting numbers without using any other data. | Neutrino mass does not include DESI BAO prior here. I should get in touch with Nick to see if we can provide a joint constraint on neutrino mass from lensing and clusters internal to the probe. It seems one can get interesting numbers without using any other data. | ||