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Revision 2 as of 2019-02-01 07:22:51
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Editor: JosephMohr
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Revision 3 as of 2019-02-01 08:06:23
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Editor: JosephMohr
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== 9:00 - 10:30 Tuesday == == 9:00 - 10:30 Tuesday: How do we create the cluster catalog? ==
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== 11:00 - 12:30 Tuesday ==  * Goals and status of the CFC (cluster finding challenge)
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== 14:30 - 16:00 Tuesday ==  * MCMF overview with focus on lessons learned from RASS+DES
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== 16:30 - 18:00 Tuesday ==  * Status of the DECam surveys and the PS region of the eROSITA-DE sky
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== 9:00 - 10:30 Wednesday ==  * Discussion and plans going forward
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== 11:00 - 12:30 Wednesday == == 11:00 - 12:30 Tuesday: What is a cluster selection function? ==

 * Review of the selection function modeling in SPT-SZ and MARD-Y3, implications for eROSITA

 * Modeling of the selection function using sky simulations within a fixed cosmology

 * Scaling relations, scatter and sky simulations- what are the connections and complementarity?

 * Discussions and plans going forward

== 14:30 - 16:00 Tuesday: How do we cross-compare and then combine mass calibration information? ==

 * Review of the available sources of dynamical and weak lensing mass calibration information

 * Strategy for the incorporation of mass calibration information within the eROSITA-DE cluster analyses

 * New ideas and new directions- importance of strong lensing, relevance of CMB lensing, etc

 * Discussion and plans going forward

== 16:30 - 18:00 Tuesday: What is our plan for the cluster cosmology analysis? ==

 * Cluster cosmology context and competition, the eROSITA-DE perspective

 * Empirical mass calibration and cosmological studies using the Grandis+ code

 * Cosmological studies using other codes (add short title/description)

 * Discussion and plans going forward

== 9:00 - 10:30 Wednesday: HSC+eROSITA planning with eFEDS and eRASS1 ==

 * Review of the four eFEDS key projects

 * Plans for the eRASS1 coverage of the HSC survey

 * Presentation of the proposed leads for the key projects

 * Discussion and plans going forward

== 11:00 - 12:30 Wednesday: What are our plans for non-cosmology cluster science? ==

 * Review of PV phase observations and science goals

 * Presentation of additional science ideas together with comment on timescale and resources

 * Discussion and plan going forward

Potsdam Meeting CWG Splinter Session Agenda

9:00 - 10:30 Tuesday: How do we create the cluster catalog?

  • Goals and status of the CFC (cluster finding challenge)
  • MCMF overview with focus on lessons learned from RASS+DES
  • Status of the DECam surveys and the PS region of the eROSITA-DE sky
  • Discussion and plans going forward

11:00 - 12:30 Tuesday: What is a cluster selection function?

  • Review of the selection function modeling in SPT-SZ and MARD-Y3, implications for eROSITA
  • Modeling of the selection function using sky simulations within a fixed cosmology
  • Scaling relations, scatter and sky simulations- what are the connections and complementarity?
  • Discussions and plans going forward

14:30 - 16:00 Tuesday: How do we cross-compare and then combine mass calibration information?

  • Review of the available sources of dynamical and weak lensing mass calibration information
  • Strategy for the incorporation of mass calibration information within the eROSITA-DE cluster analyses
  • New ideas and new directions- importance of strong lensing, relevance of CMB lensing, etc
  • Discussion and plans going forward

16:30 - 18:00 Tuesday: What is our plan for the cluster cosmology analysis?

  • Cluster cosmology context and competition, the eROSITA-DE perspective
  • Empirical mass calibration and cosmological studies using the Grandis+ code
  • Cosmological studies using other codes (add short title/description)
  • Discussion and plans going forward

9:00 - 10:30 Wednesday: HSC+eROSITA planning with eFEDS and eRASS1

  • Review of the four eFEDS key projects
  • Plans for the eRASS1 coverage of the HSC survey
  • Presentation of the proposed leads for the key projects
  • Discussion and plans going forward

11:00 - 12:30 Wednesday: What are our plans for non-cosmology cluster science?

  • Review of PV phase observations and science goals
  • Presentation of additional science ideas together with comment on timescale and resources
  • Discussion and plan going forward

14:30 - 16:00 Wednesday

No CWG splinter. Attend AGN or Calibration WG splinters.

16:30 - 18:00 Wednesday

Joint discussion of multi-lambda followup plans with AGN WG.

EROSITAwiki: CWG Splinters (last edited 2019-02-01 08:16:50 by JosephMohr)