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 14:50
      COSMOLOGY
      • 14:00
        Hyeonmo's Report 10m
        Speaker: Hyeonmo Koo (University of Seoul)

        Brief Introduction of the Calculation inside GADGET2 Simulation & Plotting

        • Smoothing length hi would be decided from: N (0 < r < 2hi) = 30.
          • Number of particles inside r < 2hi graph
          • ρCalculated - ρData
        • Number of particles per each halo = 20000 → x 50 collision samples → Superposition → Number of particles per each halo = 1000000 → N (0 < r < 2hi) can be roughly given as 30 x 50 = 1500
          • pynbody.config['sph']['smooth-particles'] = 1500 ≈ 1200
        • Displacement 5 pc → Superposition
        • Used vi_render.pyx
        • Initial → (O)
        • Statistical → (X)
        • One grid size: 170 pc
        • Solve for how many sigma differences.
      • 14:10
        Young's report. FoF and MST algorithm 10m
        Speaker: Young Ju

        FoF and MST Algorithm

        • Comparison of density calculation
          • MGS calculates density before finding neighbors.
            • Density threshold : 10 Mpc/h
            • Density threshold : 5 Mpc/h
            • Using Voronoi method
            • No kink
        • MGS for python version
          • Use 'Numba', it takes about 2 minutes.
          • C++ code → Python code
          • Loop three times → Loop once
        • We need the optimization.
      • 14:20
        Hannah's Report 10m

        See the slides from 8p

        Speaker: Hannah Jhee (University of Seoul)

        Axionyx

        • Test on multi-level grids
        • Possible caveats
          • Initial soliton profile
          • Boundary condition: Outflow?
          • Periodic boundary condition (X)
          • → Free streaming
          • → Good boundary condition
          • → Halo condition simulation
          • Give plenty of time → Relaxation
          • r1/2 → Fixed
          • r0 → Random
          • Halo has zero centroid velocity and is at rest.
      • 14:30
        Sumi's report 10m
        Speaker: Sumi Kim (University of Seoul)

        Plan for IAU Poster

        • No progress
      • 14:40
        Dr.Sabiu's Report 10m
        Speaker: Dr Cristiano Sabiu (University of Seoul)

        Deep Learning the Deep Sky: Recovering Low Surface Brightness Objects with Machine Learning

        • No progress
    • 14:50 15:00
      Discussion 10m