Campuses:
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| private:teleconsnotes20171004 [2017/10/09 16:02] – [Table] 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 % |
| - | | | 55 % | | + | |
| | ns | 0.0015 | | ns | 0.0015 | ||
| | tau | 0.0021 | | tau | 0.0021 | ||
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| | N_eff | 0.039 | 0.033 | | | N_eff | 0.039 | 0.033 | | ||
| | m_nu | 43 meV | 36 meV | | | m_nu | 43 meV | 36 meV | | ||
| - | Omega_k| 0.0018 | 0.0015| | + | |Omega_k | 0.0018 |
| 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. | ||