Difference between revisions of "Wish List and Existing Capability for Simulated Maps"

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+ Models
 
+ Models
  
* The tSZ and kSZ maps use halo profiles obtained from hydrodynamical simulations ([[[http://adsabs.harvard.edu/abs/2012ApJ...758...75B | BBPS 2012]]] and [[[http://adsabs.harvard.edu/abs/2016JCAP...08..058B | Battaglia 2016]]])
+
* The tSZ and kSZ maps use halo profiles obtained from hydrodynamical simulations ([http://adsabs.harvard.edu/abs/2012ApJ...758...75B | BBPS 2012] and [http://adsabs.harvard.edu/abs/2016JCAP...08..058B | Battaglia 2016])
* So far the current CIB maps designed only for cross correlation work with clusters. The SED and profiles come from [[[http://adsabs.harvard.edu/abs/2014A%26A...571A..30P |Planck CIB model]]]
+
* So far the current CIB maps designed only for cross correlation work with clusters. The SED and profiles come from [http://adsabs.harvard.edu/abs/2014A%26A...571A..30P |Planck CIB model]
* The current optical HOD model is analogous to the one used for [[[http://adsabs.harvard.edu/abs/2013MNRAS.428.1036M |BOSS mocks ]]]
+
* The current optical HOD model is analogous to the one used for [http://adsabs.harvard.edu/abs/2013MNRAS.428.1036M |BOSS mocks ]
  
 
+ Figures
 
+ Figures
[[image tSZ_panels.png width="1000px"]]
+
[[File:[[[image tSZ_panels.png width="1000px"]]]]]
 
Figure 1 - 504 full-sky Compton y-maps generated with our simulation pipeline
 
Figure 1 - 504 full-sky Compton y-maps generated with our simulation pipeline
[[image All_sky_multi.png width="1000px"]]
+
[[File:Example.jpg]]
 
Figure 2 - Montage of a single multi-wavelength realization of the extragalactic sky
 
Figure 2 - Montage of a single multi-wavelength realization of the extragalactic sky
  
+ Data files
+
+ Data files  
40 fullsky healpix y maps of nside=4096. 
+
On Nersc?
[[[http://www.cita.utoronto.ca/~gstein/data/tSZ_hidden/ | tSZ y-maps]]]
 

Revision as of 15:00, 16 November 2016

This page is meant to be a clearinghouse for requirements (desires?) for simulated maps and existing resources/capabilities for producing such maps

Created, 18Oct16

Wish List

  • Full-sky Healpix-pixelized maps at NSIDE=8192 (~0.4 arcmin resolution)
  • At least 8 frequency bands
  • Lensed CMB, Unlensed CMB, Kappa maps
  • Lots more...

Existing Resources / Capabilities

Nov 16 2016 CITA group (Dick, Marcelo, & George ) + Nick

We have developed a massively parallel LSS simulation pipeline for forecasting and application to upcoming experiments and surveys such as CMB-S4, DESI, and LSST.

The pipeline produces light cone halo catalogs and full-sky simulated observations suitable for data covariance determination by direct Monte Carlo, and includes beyond standard model (BSM) effects such as non-Gaussian initial conditions and evolving dark energy and undergoing continuous development for BSM effects.

+ Current data products and capabilities

++ 500 simulated full sky light cones (Healpix format)

++ Full sky maps:

  • Cluster/Group tSZ Effect (500 Compton y-maps)
  • Cluster/Group kSZ Effect (500 dT/T maps)

++ Can be simulated given specs (e.g. nu, flux cut, cosmo parameters):

  • Optical galaxy redshift catalogs for a given survey HOD
  • CIB maps at 100-2000 GHz for various models in literature
  • Light cones with specified resolution and survey geometries

+ Performance and computational resources

  • Full-sky catalogs take ~10 min each on 128 Scinet-GPC nodes, or ~20 node-hours
  • Full suite of 500 runs took ~1e4 node-hours, or ~2 days wall-clock
  • Map projection is a negligible fraction of computational cost

+ Models

  • The tSZ and kSZ maps use halo profiles obtained from hydrodynamical simulations (| BBPS 2012 and | Battaglia 2016)
  • So far the current CIB maps designed only for cross correlation work with clusters. The SED and profiles come from |Planck CIB model
  • The current optical HOD model is analogous to the one used for |BOSS mocks

+ Figures [[File:[[[image tSZ_panels.png width="1000px"]]]]] Figure 1 - 504 full-sky Compton y-maps generated with our simulation pipeline Example.jpg Figure 2 - Montage of a single multi-wavelength realization of the extragalactic sky

+ Data files On Nersc?