Difference between revisions of "Notes from May 31 telecon on science requirements for clusters/high-ell"

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(Created page with "Telecon on 31 May 2017 * Fisher predictions: Nick and Mat. Will provide by Friday constraints for decoupled redshift bins, i.e., where the scaling relation parameters are i...")
 
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Telecon on 31 May 2017
 
Telecon on 31 May 2017
  
* Fisher predictions:
+
* General information
Nick and Mat.  Will provide by Friday constraints for decoupled redshift bins, i.e., where the scaling relation parameters are independently determined in each bin (DONE).
+
** CDT face-to-face meeting June 12 and 13, 2017 at NSF.
 +
** AAA meeting June 22, 2017
  
* Simulations:
+
* Fisher predictions
 +
** Nick and Mat will provide constraints by Friday for decoupled redshift bins, i.e., where the scaling relation parameters are independently determined in each bin (DONE).
 +
 
 +
* Simulations
 +
** Argonne: maps with tSZ, CMB, extragalactic sources and uncorrelated CIB from light cones next week; correlated CIB in progress.  Based on SPT-SZ noise at 90, 150 and 220 GHz (Nick's configuration for Fisher).
 +
** CITA: peak-patch approach.  Ongoing interaction between Argonne and CITA to compare peak-patch and N-body using same initial conditions.
 +
** NERSC:
 +
*** Simulation capability for all experiments.
 +
*** Now have SO atmospheric simulations.
 +
*** Marcelo is about to deliver a complete set of maps (CITA) with tSZ, kSZ, uncorrelated CIB, lensing for z<4.5.  Frequency range: 10 -  270 GHz.
 +
** Discussion of simulating higher frequency channels, e.g., CCAT-prime.  NERSC will do so.
 +
** Decided to dedicate an upcoming telecon to simulation effort; to be led by Julian.

Revision as of 10:47, 11 June 2017

Telecon on 31 May 2017

  • General information
    • CDT face-to-face meeting June 12 and 13, 2017 at NSF.
    • AAA meeting June 22, 2017
  • Fisher predictions
    • Nick and Mat will provide constraints by Friday for decoupled redshift bins, i.e., where the scaling relation parameters are independently determined in each bin (DONE).
  • Simulations
    • Argonne: maps with tSZ, CMB, extragalactic sources and uncorrelated CIB from light cones next week; correlated CIB in progress. Based on SPT-SZ noise at 90, 150 and 220 GHz (Nick's configuration for Fisher).
    • CITA: peak-patch approach. Ongoing interaction between Argonne and CITA to compare peak-patch and N-body using same initial conditions.
    • NERSC:
      • Simulation capability for all experiments.
      • Now have SO atmospheric simulations.
      • Marcelo is about to deliver a complete set of maps (CITA) with tSZ, kSZ, uncorrelated CIB, lensing for z<4.5. Frequency range: 10 - 270 GHz.
    • Discussion of simulating higher frequency channels, e.g., CCAT-prime. NERSC will do so.
    • Decided to dedicate an upcoming telecon to simulation effort; to be led by Julian.