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
        Hyeonmo's Report
        Speaker: Hyeonmo Koo (University of Seoul)

        Planar System Generation

        • We have created the ellipsoid+ satellite galaxy.
        • We discuss setting the initial conditions more precisely.
        • We imple Professor Jaeweon Lee code with MATLAB.
        • We are currently in the process of seeking a direction for research.
        • We study gas dynamics code.
        • Cold Dark Matter (CDM): Gas separation is important., collisionless
          • Collisionless
            • Cross section is very small.
            • CDM has the property of passing through.
            • Under gravity, there is no interaction other than gravity.
            • The trajectory changes.
        • Fuzzy Dark Matter (FDM): Velocity changes., the dispersion represents., FDM is described as waves.
          • FDM is described as waves.: Interference, the property of waves, represents.
          • Cooling principle: The interaction between the two
      • 2
        Young's report. FoF and MST algorithm
        Speaker: Young Ju

        FoF and MST algorithm

        • We check Mulguisin code.
        • We make switch of 'voronoi+local+weight'.
        • We set radius = 10 (dimensionless)
        • We add errors.
      • 3
        Hannah's Report
        Speaker: Hannah Jhee (University of Seoul)

        Halos infalling a cluster through filaments

        • Decomposition of halo velocity
        • Problem: How did you set up the filament?
          • All time filament: Remove the unnecessary things (physically low-density things) and collect the important things.
          • Filament fix: Reduce the noise.
          • Finding the filament structure.: Merger tree.
          • 500 times smoothed
            • Readjust one position of the filament as the mean.
          • Review vpararell.
          • Setting the criteria for the merger tree well.
          • Filament is curved.
        • Participate in KITP workshop (program).: Feb 5th ~ Feb 16th
      • 4
        Seyeon's Report - CLML
        Speaker: Se Yeon Hwang (Universe of Seoul)

        Cosmology with Large scale structure using Machine Learning (CLML)

        • We predict parameters as Convolution Neural Network (CNN).
      • 5
        Sumi's report
        Speaker: Sumi Kim (University of Seoul)

        Cosmology of High-Order Statistics (CHOA) & Dark Energy Spectroscopic Instrument (DESI)

        • A joint study with Professor Ena Choi: Satellite Galaxy Distribution
      • 6
        Dr.Sabiu's Report
        Speaker: Dr Cristiano Sabiu (University of Seoul)

        Deep Learning the Deep Sky: Recovering low surface brightness objects with machine learning

        • No progress
    • 7
      Discussion