CPLUOS Astrophysics team meeting

Asia/Seoul
물리학과

물리학과

Zoom Meeting https://uos-ac-kr.zoom.us/j/8264902652 Meeting ID: 826 490 2652
Description

https://uos-ac-kr.zoom.us/j/8264902652

    • 14:00 15:00
      COSMOLOGY
      • 14:00
        Hyeonmo's Report - Head-on Collsion of FDM/CDM Halos(Writing Paper) 10m
        Speaker: Hyeonmo Koo (University of Seoul)

        Head-on Collsion of FDM/CDM Halos(Writing Paper)

        • Figure 1 : Snapshots of FDM halo collision for v_i = 112.776km/s and v_i = 225.552km/s. For the last two snapshots of each v_i, the COM of each halos should be located on the dotted line if any other interactions are excluded.
        • The comparison of two figure in FDM and CDM
      • 14:10
        Young's report. FoF and MST algorithm 10m
        Speaker: Young Ju

        Mulguisin Clustering Algorithm 1

        Comparison of Clustering Algorithms for Study of Cosmic Structure Finding

        • According to step 5, schematic idea of MGS
        • MGS performance test
          • Ratio = (returned member)/(original member)
          • For MST, there is no link with distance larger than about 10. So even if I increase the linking-length, the number of cluster does not change.
          • MST → flat → because of algorithm
        • There is fault
          • Check the hierarchical clustering and DBSCAN again
          • Hierarchical clustering : there are two criteria
          • 1. Single : calculate euclidean distance
          • 2. Ward : calculate variance of distance
          • Single : distance_threshold = 1.0
          • Ward : distance_threshold = 1.0
          • DBSCAN : eps = 1.0, min_sample = 3
          • When min_sample is very small, the result of DBSCAN return the same result of hierarchical
      • 14:20
        Hannah's Report 10m
        Speaker: Hannah Jhee (University of Seoul)

        Filament

        • DisPerSE : from Morse Theory
        • T-ReX : from MLE on MST
        • Running DisPerSE
        • Create 2D Mock Data
        • Create 3D Mock Data
      • 14:30
        CHOA(Cosmology of High-Order Statistics) 10m
        Speaker: Sumi Kim (University of Seoul)
      • 14:40
        CLML 10m

        Cosmology with Large scale structure using Machine Learning

        Speaker: Se Yeon Hwang

        Cosmology with Large scale structure using Machine Learning(CLML)

        • Preparing for the KAS
        • DATA
        • Basic model
        • DATA normalization
        • How to get this contour?
          • Ω_m = 0.3072
          • σ_8 = 0.8288
        • Epoch : 200, learning rate = 0.0005
          • Predict one : use same model & some input data, but the output is only one.(Ω_m or σ_8)
      • 14:50
        Dr.Sabiu's Report - N-PCF 10m
        Speaker: Dr Cristiano Sabiu (University of Seoul)
    • 15:00 15:10
      Discussion 10m