Campuses:
This shows you the differences between two versions of the page.
| Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
| private:teleconsnotes20170503 [2017/05/19 16:09] – hanany | private:teleconsnotes20170503 [2017/05/19 16:16] (current) – hanany | ||
|---|---|---|---|
| Line 3: | Line 3: | ||
| Legend: **Bold face** encodes 'need more information'; | Legend: **Bold face** encodes 'need more information'; | ||
| - | Telecon Notes by Al Kogut | + | Telecon Notes by Al Kogut (with extra SH edits) |
| - | Shaul has put an Excel spreadsheet onto the wiki executive area with bands used by previous imagers (concepts or flight missions). Need to look at previous literature on band optimization. **__Action**: Will set up smaller working group to propose bands for Probe.__ | + | * Shaul has put an Excel spreadsheet onto the wiki executive area with bands used by previous imagers (concepts or flight missions). Need to look at previous literature on band optimization. **__Action__**: __Will |
| - | + | | |
| - | -- List currently contains only bands from bolometer missions, | + | |
| - | not to be taken as dismissing lower frequencies. | + | |
| - | + | | |
| - | + | * __**Action:** to contact Kris Gorski for trades on scan strategy__ | |
| - | General agreement on wording of E-mail for community participation | + | * __**Action: |
| - | in working groups. | + | |
| - | working group including non-inflationary fundamental physics (neutrino mass, | + | * __**Action** to review paper, see if this is worth looking into for Probe.__ |
| - | N_eff). | + | |
| - | + | ||
| - | + | ||
| - | Question for data challenge: What units should we use? Thermodynamic | + | |
| - | temperature units will pose a problem when trying to combine with | + | |
| - | channels above 1 THz from a spectrometer. | + | |
| - | is already in units mK thermodynamic temperature. | + | |
| - | massive rework, but don't want to prevent analysis of potential benefits | + | |
| - | from spectrometer data from higher frequencies. | + | |
| - | + | ||
| - | + | ||
| - | Amy reviewed initial aperture analysis. | + | |
| - | which has 4.6 m usable fairing diameter. | + | |
| - | aperture is 1.2 m to 1.4 m unless we go to deployables. | + | |
| - | significantly larger than CoRE will require significant cost savings | + | |
| - | from some other subsystem. | + | |
| - | that strongly pushes case for apertures significantly larger than 1.2 meters? | + | |
| - | o Action to contact Kris Gorski for trades on scan strategy | + | |
| - | o Can we distribute studies done for CoRE and LiteBIRD to Probe EC? | + | |
| - | + | ||
| - | + | ||
| - | Cluster science: Adding space mission (CoRE) to ground_based (CMB-S4) | + | |
| - | significnantly enhances number of identified clusters. | + | |
| - | improved foregrounds from space mission. | + | |
| - | for specific assumptions. | + | |
| - | o Action to review paper, see if this is worth looking into for Probe. | + | |