Campuses:
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=== Notes === | === Notes === | ||
- | Discussion | + | Discussion of status of report |
- | * have to look at the science impacts | + | * Raphael put text in for inflation, non-Guassianity, |
- | * start with sensitivity --- r is in "first place" scientifically | + | * **Raphael will contact Levon and Vera to contribute text about primordial magnetic field and birefringence, |
- | * look at the high frequency bands | + | * Question about the final formats of Figures 1 and 2; Shaul says: TBD |
- | * different technology, | + | * Question about our 2 \sigma values. Shaul suggest that Raphael will recalculate given the requirements and CBE, just so that we have the basic values, like we did many months ago. **Raphael agrees |
- | + | * Raphael points out that foreground subtraction performance from the foregrounds group still needs to come together and fold into the predictions. | |
- | * what drives | + | * Question: what noise values and what r is Clem using in his simulations. We would want to use the ' |
- | * data rate | + | * Colin talks about his ' |
- | * spin rate | + | * The key question is: are we happy with the science objectives as listed in the STM? We all agree about the reionization objective. Do we have one more? two more? **Nick and Colin will discuss and finalize the entry(ies?) in the STM. Colin will restructure the ' |
- | | + | * Nick reminds us that the strengths of space are in the full sky coverage and the high frequencies which are important |
- | | + | * Laura describes the state with Galactic Science; good progress with the STM through iterations with Shaul and Amy. Folks are working on overleaf. 3 pg. material will be ported by the end of August. |
- | | + | * **Shaul will communicate with Gianfranco and request 2 pages for 'extra science' |
- | + | * **Shaul will communicate with Charles Lawrence and Marcel Schmittfull about ' | |
- | * Shaul - get risk list from Amy | + | |
+ | * Systematics section is well along. Shaul is working with Brendan on the section. |