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| sept._20_2017 [2017/09/27 08:38] – nbatta | sept._20_2017 [2017/10/03 13:53] (current) – hanany |
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| Nick - Clusters | Nick - Clusters |
| Nick - Some interesting cluster neutrino mass constraints: | Nick - Some interesting cluster neutrino mass constraints: |
| * Unordered List ItemS4-max + Optical lensing calibration: ~ 25 meV (Planck tau) | * S4-max + Optical lensing calibration: ~ 25 meV (Planck tau) |
| * Unordered List ItemCMB Probe + Optical lensing calibration: ~ 20 meV (CMB Probe tau) | * CMB Probe + Optical lensing calibration: ~ 20 meV (CMB Probe tau) |
| * Unordered List ItemS4-max + Optical lensing calibration: ~ 10 meV (CMB Probe tau) | * S4-max + Optical lensing calibration: ~ 10 meV (CMB Probe tau) |
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| Alex - Lensing S/N estimates | Alex - Lensing S/N estimates |
| * Unordered List Itemhttp://www.cita.utoronto.ca/~engelen/plots/cmbprobe_noisecurves.pdf - The noise curves for Cmbprobe which Nick sent me, together with the minimum-variance combination that I get when I just coadd them all without regard to the existence of any foreground power (or any non-CMB signals) (thick black). The result has a temperature noise of 0.8 uK-arcmin. | * http://www.cita.utoronto.ca/~engelen/plots/cmbprobe_noisecurves.pdf - The noise curves for Cmbprobe which Nick sent me, together with the minimum-variance combination that I get when I just coadd them all without regard to the existence of any foreground power (or any non-CMB signals) (thick black). The result has a temperature noise of 0.8 uK-arcmin. |
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| * Unordered List Itemhttp://www.cita.utoronto.ca/~engelen/plots/cmbprobe_lensingnoise.pdf - Lensing noise curves for Cmbprobe (red) and CMB-S4 (blue). Note CMB-S4 has slightly higher noise but much better angular resolution. I set lmax = 5000 for both TT and pol (although usually we set it to 3000 for TT) and I assumed f_sky = 0.4. The EB curves include the impact of iterative delensing for both experiments. | * http://www.cita.utoronto.ca/~engelen/plots/cmbprobe_lensingnoise.pdf - Lensing noise curves for Cmbprobe (red) and CMB-S4 (blue). Note CMB-S4 has slightly higher noise but much better angular resolution. I set lmax = 5000 for both TT and pol (although usually we set it to 3000 for TT) and I assumed f_sky = 0.4. The EB curves include the impact of iterative delensing for both experiments. |
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| Colin & Max & Nick - Component separation / y-maps | Colin & Max & Nick - Component separation / y-maps |