Difference between revisions of "Argonne-2018:P2-3"

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Minutes
 
Minutes
JC - We want to identify what’s unique and who’s going to do it. Think about writing white papers.
+
*JC - We want to identify what’s unique and who’s going to do it. Think about writing white papers.
SA - X-ray measurements will be very precise and high-resolution, we need to make sure we emphasize the strength of the kSZ, high redshift, low mass, large radii.
+
*SA - X-ray measurements will be very precise and high-resolution, we need to make sure we emphasize the strength of the kSZ, high redshift, low mass, large radii.
JC - Need to get buy in from Galaxy Formation people, have them sign on to white papers
+
*JC - Need to get buy in from Galaxy Formation people, have them sign on to white papers
LB,SA,AS - We should be strategic how we talk about baryonic effects on cosmic shear and LSS  
+
*LB,SA,AS - We should be strategic how we talk about baryonic effects on cosmic shear and LSS  
JK,LN - Advertisement / Outreach to broker community through conferences, talks, etc.
+
*JK,LN - Advertisement / Outreach to broker community through conferences, talks, etc.
JB - Should we have have one set of simulations. Many opinions…
+
*JB - Should we have have one set of simulations. Many opinions…
  
 
List of topics
 
List of topics
  
-Galaxy evolution and feedback (kSZ and tSZ)
+
*Galaxy evolution and feedback (kSZ and tSZ)
-Synergies with imaging surveys (kSZ)
+
*Synergies with imaging surveys (kSZ)
-Growth of Structure as function of redshift
+
*Growth of Structure as function of redshift
-Add Cluster constraints into neutrino and Dark energy chapters
+
*Add Cluster constraints into neutrino and Dark energy chapters
-Legacy catalog and High-redshift galaxy formation
+
*Legacy catalog and High-redshift galaxy formation

Latest revision as of 15:24, 6 March 2018

Back to Argonne 2018 main page

Parallel session P2-3: Forecasting - the extended science case for the Decadal (chairs: N. Battaglia and C. Hill)

Notes from session (Tuesday, March 6, 09:45-10:45)

Extending The science Case (ETC) P1-3, P2-3

Minutes

  • JC - We want to identify what’s unique and who’s going to do it. Think about writing white papers.
  • SA - X-ray measurements will be very precise and high-resolution, we need to make sure we emphasize the strength of the kSZ, high redshift, low mass, large radii.
  • JC - Need to get buy in from Galaxy Formation people, have them sign on to white papers
  • LB,SA,AS - We should be strategic how we talk about baryonic effects on cosmic shear and LSS
  • JK,LN - Advertisement / Outreach to broker community through conferences, talks, etc.
  • JB - Should we have have one set of simulations. Many opinions…

List of topics

  • Galaxy evolution and feedback (kSZ and tSZ)
  • Synergies with imaging surveys (kSZ)
  • Growth of Structure as function of redshift
  • Add Cluster constraints into neutrino and Dark energy chapters
  • Legacy catalog and High-redshift galaxy formation