Difference between revisions of "CIB lensing"
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[[File:Cib totalfield powerspectrum err norm.png|200px]] | [[File:Cib totalfield powerspectrum err norm.png|200px]] | ||
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| + | and smoothed : | ||
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| + | [[File:Cib totalfield powerspectrum sm.png|200px]] | ||
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| + | This was done with field only, Cal_sky was not working with halos cutout. | ||
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| + | Here is the fractional difference : | ||
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| + | [[File:Cib totalfield powerspectrum reldiff.png|200px]] | ||
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| + | With smoothing and Planck data : | ||
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| + | |||
| + | [[File:Cib totalfield powerspectrum reldiff err.png|200px]] | ||
Latest revision as of 19:35, 24 August 2018
Final picture, the CIB is divided in slices,each slice is lensed by the appropriate kappa shell. Then all the slices are added up
and smoothed :
This was done with field only, Cal_sky was not working with halos cutout.
Here is the fractional difference :
With smoothing and Planck data :
