In Initial Velocity [28.184km/s] - Velocity Decrease [28.184km/s] graph,
0 ~ 42 : FDM Data is higher than CDM Data
42 ~ : FDM Data and CDM data are similar
The Halo with mass M → Scaling of halo with mass M_0 which have initial velocity vM_0/M
Here, set the M_0 = 50, drew the graph comparing velocity of before and after collision.
17:00
Young's report. FoF and MST algorithm15m
Speaker:
Young Ju
FoF and MST algorithm
Check the number of cluster by changing linking-length.
Random data : 50 clusters
Noise : 5,000
In fResolution - Number graph,
MGS
n total
n >= 3
n >= 50
In Linking - Length graph,
FoF
n total
n >= 3
n >= 50
17:15
CHOA(Cosmology of High-Order Statistics)15m
Speaker:
Sumi Kim(University of Seoul)
CosKASI Presentation Summary
Goal : To extract more information from small scales(~50Mpc)
Method : Train some generated simulations with Gaussian Process and using MCMC to recover test simulation parameters.
Result : Using 5 kinds of Correlation functions can predicted with few % error at small scales, improving cosmological parameters precision increase with 15 ~ 25%
Projected : ω_p(r_p)
Monopole : ξ_0(r)
Quadrupole : ξ_2(r)
Underdensity probability : P_U(r)
Marked correlation function : M(r)
Our progress
Considering all possible shapes in 4pcf on our code and working on generalizing issues.
17:30
Dr.Sabiu's Report - Density Reconstruction15m
Speaker:
DrCristiano Sabiu(University of Seoul)
Density Reconstruction
3-point correlation function - all bins (configurations) → How about draw the graph as 3-D instead 2-D?
4-point correlation function - all bins (configurations)