Campuses:
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imagerteleconnotes20180425 [2018/04/25 13:57] – hanany | imagerteleconnotes20180425 [2018/04/25 16:04] (current) – wenxx181 | ||
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====== Telecon 20180425 ====== | ====== Telecon 20180425 ====== | ||
- | Attending: | + | Attending: |
Notes by : Qi | Notes by : Qi | ||
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=== Agenda=== | === Agenda=== | ||
- | * [[http:// | + | * [[http:// |
* Comparing NETS: PICO, CORE, LiteBIRD | * Comparing NETS: PICO, CORE, LiteBIRD | ||
* {{:: | * {{:: | ||
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=== Notes === | === Notes === | ||
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+ | * link for workshop | ||
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+ | * Noise comparison (Karl) | ||
+ | * page 2 | ||
+ | * left is in log scale, right is just a zoom for low frequencies | ||
+ | * a few changes: | ||
+ | * 4 years to 5 years, after Mission study meeting, ~900M, still 10% less than cap | ||
+ | * 10% loss from low-pass filters. Planck had ~15%. There are 3-4 elements, each has ~3% loss. | ||
+ | * Bandwidth, optical efficiencies and temperatures are the main factors that distinguish experiments. | ||
+ | * PICO: 25% top-hat bandwidth, 70% optical efficiency (lenselet+loss+bolo) | ||
+ | * Karl is going to check with Jaques if spillover was included in optical efficiency for CORE; check with Toki if he can bring more numbers here for next week's workshop | ||
+ | * CORE has higher load in high-v, probably due to both warm mirrors (and warm stop) | ||
+ | * LiteBird: data not very available; from 2016 paper. Small pixel size, thus large spillover leads to low efficiency. | ||
+ | * Conclusion: all similar, most difference is high frequency due to mirror temperatures. | ||
+ | * page 3 | ||
+ | * 6K is not totally hypothetical; | ||
+ | * temperature stability at 6K | ||
+ | * Planck' | ||
+ | * Bill: 95% observing time for 5 years may be optimistic. | ||
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