Difference between revisions of "LBNL-2020: Galactic Foreground Modeling"

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== Agenda ==
 
== Agenda ==
  
* Data challenge paper and next steps (Victor, 10)
+
* [https://docs.google.com/presentation/d/1SNdXrNwx0NOHkv0f7IbvPrV5cDeTu-weyIeP1Sp5pcg/edit#slide=id.g726b394445_0_261 Data challenge paper and next steps] (Victor, 10)
 
* [[:File: LBNL-Foreground_modeling-DC06.pdf | 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)

Revision as of 10:58, 1 April 2020

Connection details

Parallels 5 and 6, Session D. Wednesday April 1, 11:30 AM to 1:30 PM pacific.

https://lbnl.zoom.us/j/659092332

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

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