Difference between revisions of "July 29th, 2019 - CIB Lensing: Minimum Mass vs. (Halo) Kappa Reduced Bispectra (Selected Shells & Multipoles)"
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| − | In this post, I have plots showing how <math> b_{\ell} </math> changes by the minimum mass (cut) for selected shells at selected multipoles. The absolute minimum mass the catalog contains is about <math> 1.29 \times 10^{12} M_{\odot} </math>. I have four mass cuts (5e12, 1e13, 5e13, 1e14) and the original total kappa in each of the plots. | + | In this post, I have plots showing how <math> b_{\ell} </math> changes by the minimum mass (cut) for selected shells at selected multipoles. The absolute minimum mass the catalog contains is about <math> 1.29 \times 10^{12} M_{\odot} </math>. I have four mass cuts (5e12, 1e13, 5e13, 1e14) and the original total kappa in each of the plots. The bispectra does not behave with much pattern compared to the power spectra (https://mocks.cita.utoronto.ca/index.php/July_26th,_2019_-_CIB_Lensing:_Minimum_Mass_vs._(Halo)_Kappa_Power_Spectra_(Selected_Shells_%26_Multipoles,_y-axis_set_to_zero,_goes_up_to_higher_mass_cut); for shells that cover less redshifts and at higher <math> \ell </math>, the curves seem to flatten out at low mass cuts. |
'''Shell 3 (0 ~ 1200 Mpcs, Source at 1400 Mpcs) ''' (<math> \ell = 500, 1100, 2100, 3100 </math>) | '''Shell 3 (0 ~ 1200 Mpcs, Source at 1400 Mpcs) ''' (<math> \ell = 500, 1100, 2100, 3100 </math>) | ||
Latest revision as of 23:30, 29 July 2019
In this post, I have plots showing how [math]\displaystyle{ b_{\ell} }[/math] changes by the minimum mass (cut) for selected shells at selected multipoles. The absolute minimum mass the catalog contains is about [math]\displaystyle{ 1.29 \times 10^{12} M_{\odot} }[/math]. I have four mass cuts (5e12, 1e13, 5e13, 1e14) and the original total kappa in each of the plots. The bispectra does not behave with much pattern compared to the power spectra (https://mocks.cita.utoronto.ca/index.php/July_26th,_2019_-_CIB_Lensing:_Minimum_Mass_vs._(Halo)_Kappa_Power_Spectra_(Selected_Shells_%26_Multipoles,_y-axis_set_to_zero,_goes_up_to_higher_mass_cut); for shells that cover less redshifts and at higher [math]\displaystyle{ \ell }[/math], the curves seem to flatten out at low mass cuts.
Shell 3 (0 ~ 1200 Mpcs, Source at 1400 Mpcs) ([math]\displaystyle{ \ell = 500, 1100, 2100, 3100 }[/math])
Shell 7 (0 ~ 2800 Mpcs, Source at 3000 Mpcs) ([math]\displaystyle{ \ell = 500, 1100, 2100, 3100 }[/math])
Shell 12 (0 ~ 4800 Mpcs, Source at 5000 Mpcs) ([math]\displaystyle{ \ell = 500, 1100, 2100, 3100 }[/math])
Shell 17 (0 ~ 6800 Mpcs, Source at 7000 Mpcs) ([math]\displaystyle{ \ell = 500, 1100, 2100, 3100 }[/math])
