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 - Introduction of GALIC code
        Speaker: Hyeonmo Koo (University of Seoul)

        Introduction of GALIC code

        • GALIC head-on collision
          • Colorbar minimum = 5
          • GALIC cord has 10 conditions.
          • Color = density
        • Try Dice code.
      • 2
        Young's report. FoF and MST algorithm
        Speaker: Young Ju

        FoF and MST Algorithm

        • Mulguisin clustering algorithm
        • Polar angles are different.
      • 3
        Seyeon's Report - CLML
        Speaker: Se Yeon Hwang (Universe of Seoul)

        Cosmology with Large scale structure using Machine Learning (CLML)

        • No progress
      • 4
        Sumi's report
        Speaker: Sumi Kim (University of Seoul)

        Cosmology of High-Order Statistics (CHOA)

        • Redshift split → The advice: Using three redshift bins
        • MLPRegressor n = 512
        • Layers = (n, n, 2n, 2n, 2n, 2n, n, n)
        • This week
          • 3 pcf is currently running now (1/3 finished).
          • No making theoretical part slides for KAS presentation
      • 5
        John Suarez's report

        Join Photo+Spect Data

        • Photometric normalized.
          • Epoch: 10
          • Learning rate: 0.01
          • All redshift (including Z > 0.5)
            • (Model, Learning rate, Batch size, Loss (MSE))
              • (resnet50, 0.01, 32, 0.614)
        • Photometric data models
          • Redshifts z < 0.5
          • Resnet +3 linear [512, 256, 1] → Redshift
            • (Model, Learning, Batch size, Epochs, Loss)
              • (resnet50, 0.01, 32, 300, 0.828)
        • To do
          • Spectroscopic data models
          • Photometric data models
          • Data set
            • In progress a data set from GUADALUPE (Last DESI DR)
      • 6
        Hannah's Report
        Speaker: Hannah Jhee (University of Seoul)

        Halos infalling a cluster through filaments

        • Snapshot number
          • Cosine graph
            • Nearest point
            • Most dense
            • Perpendicular method → Red line is mistake. → cos0 ≠ 0
            • The process: Halo → Nearest filament → Nearest+densest (?) filament
      • 7
        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
    • 8
      Discussion