Difference between revisions of "UCSD-2019: Cross-Cut: Simulations for Measurement Requirements"

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== Remote attendance ==
== Remote attendance ==
[https://ucsd.zoom.us/j/973144732 Zoom link]
[https://ucsd.zoom.us/j/814488334 Zoom link]
== Notes ==
== Notes ==
[https://hackmd.io/o1KtRAHXSliAP-sfL73r8A Collaborative note taking on hackMD]
[https://hackmd.io/o1KtRAHXSliAP-sfL73r8A Collaborative note taking on hackMD]

Revision as of 15:00, 18 October 2019

Link back to agenda


  • How do we coordinate the production of a unified sky model with enough realism and flexibility for the AWGs?
  • What simulations do we need for clusters and what cross-checks will be available with data?


Please add your name below the agenda if you plan to participate in the session, contact User:Zonca

  • 10 min - introductions by everyone in the room: who? where? what is your current/future involvement in simulations?
  • 5 min - Andrea Zonca: PySM 3, simulation tools developed for Simons Observatory
  • 5 min - Brandon Hensley: Integration of physical and MHD based dust models into PySM 3
  • 5 min - Marcelo Alvarez: Extragalactic modeling integration in PySM 3, Simulations requirements for cluster finding
  • 5 min - Reijo Keskitalo: Scanning strategy for S4
  • 5 min - Ben Racine: Noise simulations for PGW analysis
  • 25 min - Discussion:
    • Unified sky model
    • How to gather requirements from AWG
    • Clusters
    • Plans for map-based simulations

Other participants: Raphael Flauger, Kimmy Wu

Remote attendance

Zoom link


Collaborative note taking on hackMD