July 26th, 2019 - CIB Lensing: Halo vs. Field Kappa Power Spectra (All Shells)
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In this post, I am attaching plots that compare the field and halo kappa power spectra for each kappa shell.
Shell # and Corresponding Comoving Distances for Kappa Shell 1 : 0 ~ 400 Mpcs (Source at 600) Shell 2 : 0 ~ 800 Mpcs (Source at 1000) Shell 3 : 0 ~ 1200 Mpcs (Source at 1400) Shell 4 : 0 ~ 1600 Mpcs (Source at 1800) Shell 5 : 0 ~ 2000 Mpcs (Source at 2200) Shell 6 : 0 ~ 2400 Mpcs (Source at 2600) Shell 7 : 0 ~ 2800 Mpcs (Source at 3000) Shell 8 : 0 ~ 3200 Mpcs (Source at 3400) Shell 9 : 0 ~ 3600 Mpcs (Source at 3800) Shell 10 : 0 ~ 4000 Mpcs (Source at 4200) Shell 11 : 0 ~ 4400 Mpcs (Source at 4600) Shell 12 : 0 ~ 4800 Mpcs (Source at 5000) Shell 13 : 0 ~ 5200 Mpcs (Source at 5400) Shell 14 : 0 ~ 5600 Mpcs (Source at 5800) Shell 15 : 0 ~ 6000 Mpcs (Source at 6200) Shell 16 : 0 ~ 6400 Mpcs (Source at 6600) Shell 17 : 0 ~ 6800 Mpcs (Source at 7000) Shell 18 : 0 ~ 7200 Mpcs (Source at 7200)
For the first three (or four) shells, the field dominates over most [math]\displaystyle{ \ell }[/math]'s; there are two intersecting points between the field and halo. In the subsequent shells, there is a certain [math]\displaystyle{ \ell }[/math] where the halo starts dominating over the field; this occurs at around [math]\displaystyle{ \ell = 500 }[/math] for closer shells, but increases as the shell number increases. For the last few shells, this point is at around [math]\displaystyle{ \ell = 1500 }[/math] or larger. In other words, as the shell number increases, the field dominates over larger [math]\displaystyle{ \ell }[/math] ranges.
Shell # Increasing from Left to Right, Top to Bottom (See Distance in Legend)