Campuses:
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| - | * | + | * Working to make a visual we have needed. |
| + | * This made by Josquin. | ||
| + | * left vertical axis is noise levels. right vertical axis is signals (CMB, dust, synchrotron) | ||
| + | * AK: Not a fan of uK_CMB above ~300 GHz. The upper range makes synchtron, dust, etc look odd. | ||
| + | * AK: Like everything in Janskies or W/ | ||
| + | * SH: Understood. This figure works for CMB community, but maybe a second product to use in a more general context. | ||
| + | * HH: Al's point is good. Reach broader groups. | ||
| + | * AT: Yes, more general units good. | ||
| + | * SH: Al can send unit suggestion to Josquin. | ||
| + | * SH: Also planning to color code bands by pixel type. | ||
| + | * AT: Error in band location? SH: yes, iterating with Josquin. | ||
| Noise Requirements vs < | Noise Requirements vs < | ||
| * AT: standard NASA term is current best estimate (CBE) | * AT: standard NASA term is current best estimate (CBE) | ||
| * starting from r is awkward as foreground limits aren't well understood. so r values don't set a noise requirement. | * starting from r is awkward as foreground limits aren't well understood. so r values don't set a noise requirement. | ||
| - | * we'll adopt this empirical noise requirement and iterate that with science case. | + | * we'll adopt this empirical noise requirement and iterate that with science case. Then we see if this pushes us off any cliffs in terms of achievable science. |
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