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/ | + | [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 16:00, 18 October 2019
Contents
Charge
- 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?
Agenda
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
