Dec 13, 2018 - Resolving low redshift CIB

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After pointing out CIB power (unlensed) from lowest redshift is weird, George and Jason went and found out that some nearby particles were given unnaturally large flux. After dropping particles up to 100 Mpc, we have somewhat more sensible power spectra. There is still a lot of point source power, but the level is notably smaller what was before (so at ell = 5000 we are no longer dominated by the lowest shell.

Second pavel 02 power spectra.png

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