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

    • COSMOLOGY
      • 1
        Dr.Sangnam Park's Report - FDM_Offset
        Speaker: Sangnam Park
      • 2
        Hyeonmo's report - CDM Halo Evolution for Gadget2 Simulation
        Speaker: Hyeonmo Koo (University of Seoul)
        • CDM Halo Evolution for Gadget2 Simulation
          • Position-box - velocity graph
            • Set M = 50
            • Peak = X-axis 33 position-box
            • M = 50 ➝ 18 ~ 25
            • M = 30 ➝ (18 ~ 25)(5/3)
            • M = 40 ➝ Initial velocity increases more than when M = 50.
      • 3
        Young's report. FoF and MST algorithm
        Speaker: Young Ju
        • FoF and MST algorithm
          • Number density : Add 5000 noise data, minimum member = 50
            • Radius : 3σ = 30, ρ = N/((4π/3)(σ^3))
            • Cluster id - ρ graph
              • MGS's ρ is bigger than MST's ρ.
              • The mean of ρ is about 0.0018.
          • Number density : Add 5000 noise data
            • True density (from random) VS Recovered density (from MGS)
            • True density - Recovered density graph
              • The mean increases proportionally.
          • Number density 2 : Add 5000 noise data, minimum member = 3
            • The number of galaxies in cluster VS The number of clusters.
            • Number of galaxies - Number of Clusters graph
              • The number of Number of clusters in MGS is about twice as high as the number of Number of clusters in MST.
      • 4
        CHOA(Cosmology of High-Order Statistics)
        Speaker: Sumi Kim (University of Seoul)
      • 5
        Dr.Sabiu's Report
        Speaker: Dr Cristiano Sabiu (University of Seoul)
    • 6
      Discussion