Introduction¶
From a OU-SHE/OU-PHZ catalogue DpdWLShearCatalog, 2D-MASS-WL will provide the following output products:
E/B modes on small patches (noisy maps, monte carlo maps, noise standard deviation maps, weighted density maps and the denoised maps).
E/B modes for the most massive clusters of the output cluster catalogue (noisy maps, noise standard deviation maps, weighted density maps and the denoised maps).
E/B modes on the full sky (noisy maps, noise standard deviation maps, weighted density maps and the denoised maps).
E/B modes on small patches¶
For the production of convergence maps for small fields, an input DpdWLShearCatalog FITS catalogue collecting information from OU-SHE/OU-PHZ is needed, as well as a set of parameters DpdTwoDMassParamsConvergencePatch specifying the location of the patches and running parameters. The noisy/denoised convergence maps and noise standard deviation maps are then obtained after projection of the input region, located on the sphere, and collected in DpdTwoDMassConvergencePatch.
E/B modes for cluster studies¶
For the production of convergence maps for clusters studies, a catalogue DpdLE3clDetClusters of optical clusters with centre position, radius and richness is used as input as well as a set of parameters DpdTwoDMassParamsConvergenceClusters and an input DpdWLShearCatalog FITS catalogue. The output product is a DpdTwoDMassConvergenceClusters containing FITS data arrays with as HDUs the noisy/denoised convergence maps, a map containing the total galaxy weight per pixel and a noise standard deviation map for a patch centred on each detected and sufficiently massive cluster.
E/B modes on the full sky¶
For the production of full-sky maps, an input DpdWLPosShearCatalog FITS catalogue collecting information from OU-SHE/OU-PHZ is needed, as well as a set of parameters DpdTwoDMassParamsConvergenceSphere specifying the HEALPix resolution and other running parameters. The product DpdTwoDMassConvergenceSphere contains as products computed on the sphere (HEALPix maps) the noisy/denoised convergence maps, the total galaxy weight per pixel, Monte-Carlo realisations and noise standard deviation maps.
Inputs/outputs list¶
E/B modes on small patches:
Inputs
DpdTwoDMassParamsConvergencePatch
DpdWLShearCatalog
DpdHealpixVisibilityMaskVMPZ
DpdTomographicBins
Outputs
DpdTwoDMassConvergencePatch
E/B modes for cluster studies:
Inputs
DpdTwoDMassParamsConvergenceClusters
DpdWLShearCatalog
DpdLE3clDetClusters
DpdHealpixVisibilityMaskVMPZ
DpdTomographicBins
Outputs
DpdTwoDMassConvergenceClusters
Spherical E/B modes:
Inputs
DpdTwoDMassParamsConvergenceSphere
DpdWLShearCatalog
DpdHealpixVisibilityMaskVMPZ
DpdTomographicBins
Outputs
DpdTwoDMassConvergenceSphere
Input products 2DMASS
Output products 2DMASS