mwhite.berkeley.edu

Data Repository: Martin White

Research group home page is here. And my research interests are summarized here. My home page is here. The following data are available to the community:. Simulated thermal SZ maps and cluster catalogues. Simulated weak lensing maps. Resources for baryon acoustic oscillations. Code for computing Fisher matrices. For redshift space distortions. Package for cosmological perturbation theory. Convolution Lagrandian Perturbation Theory (package for cosmological perturbation theory). Martin White's Home Page.

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Data Repository: Martin White | mwhite.berkeley.edu Reviews

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Research group home page is here. And my research interests are summarized here. My home page is here. The following data are available to the community:. Simulated thermal SZ maps and cluster catalogues. Simulated weak lensing maps. Resources for baryon acoustic oscillations. Code for computing Fisher matrices. For redshift space distortions. Package for cosmological perturbation theory. Convolution Lagrandian Perturbation Theory (package for cosmological perturbation theory). Martin White's Home Page.

<META> KEYWORDS

1 data repository

2 sph cluster archive

3 halo m sigma data

4 catalogues and plots

5 research

6 ly a data

7 for acoustic oscillations

8 copter

9 clpt

10 box remapping

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data repository,sph cluster archive,halo m sigma data,catalogues and plots,research,ly a data,for acoustic oscillations,copter,clpt,box remapping,cosmoxi2d,litemangle,fitstablewriter,some selected talks/lectures,apex sz experiment,boss numbers,kinetic sz

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Data Repository: Martin White | mwhite.berkeley.edu Reviews

https://mwhite.berkeley.edu

Research group home page is here. And my research interests are summarized here. My home page is here. The following data are available to the community:. Simulated thermal SZ maps and cluster catalogues. Simulated weak lensing maps. Resources for baryon acoustic oscillations. Code for computing Fisher matrices. For redshift space distortions. Package for cosmological perturbation theory. Convolution Lagrandian Perturbation Theory (package for cosmological perturbation theory). Martin White's Home Page.

INTERNAL PAGES

mwhite.berkeley.edu

1

Martin White Data Repository: CLPT

http://mwhite.berkeley.edu/CLPT

Convolution Lagrangian Perturbation Theory. The links below provide a tar-ball and README file for CLPT. A C code written by Lile Wang to compute predictions for the halo and matter clustering using Convolution Lagrangian Perturbation Theory; described in Carlson, Reid and White [MNRAS 429(2013)1674, arxiv:1209:0780. It also has extensions for the Gaussian streaming model, described in described in Reid and White [MNRAS 417(2013)1913, arxiv:1105:4165. Return to Martin's home page.

2

Martin White Data Repository: Intrinsic

http://mwhite.berkeley.edu/Intrinsic

These data are for collaborators only. Halo angular momentum data. This directory contains simulated weak lensing convergence maps made from an N-body simulation using the Born approximation. In addition we have catalogs of halos within the field of view and their angular momenta. The "location" of the halo is a somewhat fuzzy concept. I have chosen to use the location of the most bound particle, which also closely corresponds to the position of the densest particle in most of the halos. This see...

3

Martin White Data Repository: BOSS

http://mwhite.berkeley.edu/BOSS

These data are for collaborators only. Return to Martin's home page. Last modified Wed Apr 14 11:39:19 2010.

4

Martin White Data Repository: Sigma

http://mwhite.berkeley.edu/Sigma

The data files herein give the relation between the velocity dispersion and/or temperature and the mass of halos in some of my simulations. Each file is labelled by a name describing the cosmology (see below) and an output time (only a=1.0000 for now, but a summary of the redshift evolution can be found in sigmaM vs z.dat and sigmaM vs z.ps). M/10 {15}Msun/h) = (sigma/sigma15) 3. M/10 {15}Msun/h) = (kT/kT15) (3/2). Concordance150 1 1.0000.sig. Concordance150 3 1.0000.sig. Lcdm128A 1.0000.sig.

5

Hydrodynamic Simulations of Galaxy Clusters

http://mwhite.berkeley.edu/ClusterArchive

Hydrodynamic Simulations of Galaxy Clusters. A page discussing the formation of a cluster of galaxies as seen in different wavebands, along with a QuickTime movie, can be reached by following this link. More discussion of clusters, along with numerous links to other sites, can be found by by following this link. Or you can find my talk on this topic, complete with audio, at the ITP web site. A movie of structure formation in this model is here. The gas and dark matter profiles. Back to Home Page.

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cdm.berkeley.edu

Lensing: Data Repository: Martin White

http://cdm.berkeley.edu/Lensing

We have several lensing-related projects from which the data is available to the community. First is the multi-plane ray-tracing maps that were made as part of. C Vale and M. White, ApJ. Which are available by following this link. And second is the grid of models (with group and galaxy catalogues) made as part of. M White and C. Vale, Astroparticle Physics. Which are available by following this link. MWhite, Astroparticle Physics. 2005)349, [ astro-ph/0502003. Which are available by following this link.

cdm.berkeley.edu

Martin White: Selected talks

http://cdm.berkeley.edu/Talks

2013 Planck cosmology results Overview. The 10 minute version). 2013 Planck cosmology results. Slides from talk at LBNL). 2013 Planck cosmology results. Audio slides from talk at SLAC). Cosmic Sound: Near and Far. Cosmological results from Planck 2015. Slides from talk at Yale). 2012 Santa Fe cosmology workshop. Talk on non-BAO science with BOSS. 2007 Santa Fe cosmology workshop. On Redshift surveys and large-scale structure in Beijing. 2010 Santa Fe cosmology workshop. Notes for lecture(s) given in 2004.

cdm.berkeley.edu

Hydrodynamic Simulations of Galaxy Clusters

http://cdm.berkeley.edu/ClusterArchive

Hydrodynamic Simulations of Galaxy Clusters. A page discussing the formation of a cluster of galaxies as seen in different wavebands, along with a QuickTime movie, can be reached by following this link. More discussion of clusters, along with numerous links to other sites, can be found by by following this link. Or you can find my talk on this topic, complete with audio, at the ITP web site. A movie of structure formation in this model is here. The gas and dark matter profiles. Back to Home Page.

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Data Repository: Martin White

Research group home page is here. And my research interests are summarized here. My home page is here. The following data are available to the community:. Simulated thermal SZ maps and cluster catalogues. Simulated weak lensing maps. Resources for baryon acoustic oscillations. Code for computing Fisher matrices. For redshift space distortions. Package for cosmological perturbation theory. Convolution Lagrandian Perturbation Theory (package for cosmological perturbation theory). Martin White's Home Page.

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