Difference between revisions of "LBNL-2020: Galactic Foreground Modeling"
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* Data challenge paper and next steps (Victor, 10) | * Data challenge paper and next steps (Victor, 10) | ||
| − | * DC06 (Caterina, 10) | + | * [[:File: LBNL-Foreground_modeling-DC06.pdf | DC06]] (Caterina, 10) |
* [https://docs.google.com/presentation/d/13dpTpG9FKBsyMizep_PGGP4Xy6U_cWurcRK-PjB35lA/edit?usp=sharing PySM3] (Andrea, 10) | * [https://docs.google.com/presentation/d/13dpTpG9FKBsyMizep_PGGP4Xy6U_cWurcRK-PjB35lA/edit?usp=sharing PySM3] (Andrea, 10) | ||
* [[Media:3D-filaments-CMB-S4-2020.pdf|Filament-based models]] (Carlos, 15) | * [[Media:3D-filaments-CMB-S4-2020.pdf|Filament-based models]] (Carlos, 15) | ||
Revision as of 10:37, 1 April 2020
Contents
Connection details
Parallels 5 and 6, Session D. Wednesday April 1, 11:30 AM to 1:30 PM pacific.
https://lbnl.zoom.us/j/676588242
Monitor: Ben
Scribe: Brandon
Charge
- Presentation / discussion of new developments in simulation techniques, codes, since the last meeting.
- Identify the other working groups with science cases relying on Galactic foreground modeling (low-ell / BB, extragalactic foregrounds, etc)
- What are the conclusions of the previous data challenges for these groups, in what direction does the foreground modeling require more complexity.
- Are we prepared to provide the simulations that will be required to answer outstanding science questions for CD1.
- What trade off studies are being looked at, will these require new foreground modeling efforts?
- Are existing simulations sufficient for the next data challenge?
Agenda
- Data challenge paper and next steps (Victor, 10)
- DC06 (Caterina, 10)
- PySM3 (Andrea, 10)
- Filament-based models (Carlos, 15)
- Frequency decorrelation (Brandon, 15)
Break
- Neural Net Models, Dust (Ben, 15)
- Neural Net Models, Synchrotron (Giuseppe, 15)
Discussion
Notes
On this Google Doc for now, to be transferred to Wiki after session
