Cosmology Data Analysis
FoF catalog interpretation, Python analysis, and visualization
Institution
PNU Cosmology Group, Pusan National University
Collaboration
Prof. Junsup Shim
Timeline
Apr 2026 - Jun 2026
Overview
During a supporting-research internship in the PNU Cosmology Group, advised by Prof. Junsup Shim, I read FoF halo catalogs produced by his Fortran simulations and connected them to Python analysis and visualization. My role did not include developing the simulation itself.
My work
- Interpreted particle counts, centers, and second-moment blocks in binary catalogs and converted coordinate units.
- Worked with the halo mass function (HMF) and two-point correlation function (2pCF), learning volume and bin-width normalization and pair counting with periodic boundaries.
- Implemented interactive visualization using eigenvalues and eigenvectors of second-moment matrices. Display sizes are catalog-specific RMS scales, not halo boundary radii.
Public materials
FoF_Simulation_Plot is the public project repository. The repository-content description here is pinned to youngjinphys/FoF_Simulation_Plot@c059a7934d78c2e5798798b797ab3754ae9d48dd (2026-09-13). That revision contains a public subset of catalog-parsing, coordinate-conversion, and visualization code. It excludes the original catalogs and quantitative results and does not reproduce the complete HMF and 2pCF analysis.
I thank Prof. Junsup Shim for his guidance and the opportunity to work with research data.
Method references
Bias and variance of angular correlation functions
S. D. Landy & A. S. Szalay
The Astrophysical Journal 412, 64–71 (1993)
The evolution of large-scale structure in a universe dominated by cold dark matter
M. Davis, G. Efstathiou, C. S. Frenk & S. D. M. White
The Astrophysical Journal 292, 371–394 (1985)