Difference between revisions of "UCSD-2019: Science Theme: Matter Mapping"
From CMB-S4 wiki
Jump to navigationJump to search (→Agenda) |
|||
| Line 16: | Line 16: | ||
* Giulio Fabbian [remote]: NG lensing biases | * Giulio Fabbian [remote]: NG lensing biases | ||
* Alex van Engelen: thermal-kinetic SZ (tkSZ) [https://cmb-s4.org/wiki/index.php/File:Tksz_vanengelen_S4_oct2019.key.pdf Slides] | * Alex van Engelen: thermal-kinetic SZ (tkSZ) [https://cmb-s4.org/wiki/index.php/File:Tksz_vanengelen_S4_oct2019.key.pdf Slides] | ||
| − | * Nick Battaglia: SZ systematics | + | * Nick Battaglia: SZ systematics [[File:S4_SZ_systematics.pdf]] |
- Focused discussions: [~1 hr] | - Focused discussions: [~1 hr] | ||
Revision as of 13:33, 17 October 2019
Contents
Charge
Review science goals
Review/update/prioritize questions to be answered regarding measurement requirements
Identify priorities for science case development, if any
Agenda
- Review of previous work and science case(s) [10 min]
- Presentations on additional science and new ideas [5+2 min each]
- Srini Raghunathan: CMB-cluster lensing and tSZ counts
- Siavash Yasini: Birkinshaw-Gull effect
- Selim Hotinli: Rees-Sciama and/or moving lens effect
- Giulio Fabbian [remote]: NG lensing biases
- Alex van Engelen: thermal-kinetic SZ (tkSZ) Slides
- Nick Battaglia: SZ systematics File:S4 SZ systematics.pdf
- Focused discussions: [~1 hr]
- Further developing science cases: deep survey at the Pole -- e.g., overlap with deep satellite observations, possibilities for cross-correlations
- Galactic Science
- Review/update/prioritize questions to be answered regarding measurement requirements -- what needs to be done for CD-1? what needs to be done better than it was in the DSR?
Remote attendance
Notes
Please comment as you see fit. here
