Researcher · Astrophysics & Scientific Computing
Dr. Arman Khalatyan
Leibniz Institute for Astrophysics Potsdam (AIP)
Building the data infrastructure for precision astrophysics — from 400 million-star catalogues to the HPC, ML and AI systems that fit, benchmark and ship them.
01 On this site
02 Research & Work
Full stellar-parameter and dust-extinction posteriors for hundreds of millions of stars (StarHorse / SHBoost), chrono-chemical mapping of the Milky Way disc, bulge and bar with Gaia DR3, APOGEE and 4MOST, and the 4MIDABLE survey design for 4MOST.
High-resolution cosmological simulations of the Local Group and early galaxy assembly — from the first thin discs at z > 4 to AGN feedback in galaxy evolution (MareNostrum, Hestia). Earlier work on the QCD phase diagram and compact stars.
03 Technical Expertise
HPC & Cluster Computing
400+ node SLURM clusters, fault-tolerant large-scale jobs, NUMA/RDMA, throughput optimization.
Data Engineering
PyArrow, Dask, Parquet, S3/MinIO, 210 GB full-catalogue pipelines, end-to-end checksum verification.
Machine Learning & MLOps
vLLM inference, LoRA fine-tuning, model quantization, evaluation harnesses, agentic orchestration.
Astrophysics Research
Stellar parameter estimation, extinction mapping, galaxy formation, N-body simulation, spectroscopic surveys.
DevOps & Systems
Docker, Kubernetes, CI/CD, HAProxy, monitoring, Proxmox, secure multi-host infrastructure.
Languages & Tooling
Python (primary), Bash, C/C++ (simulation, OpenGL), LaTeX, Git, Jupyter, Matplotlib.
04 Recent Publications
The five most recent — the full record lives on the publications page.
- 2026 The Nineteenth Data Release of the Sloan Digital Sky Survey DOI ↗
- 2026 The spheroidal bulge of the Milky Way: Chemodynamically distinct from the inner-thick disc and bar DOI ↗
- 2025 Latest Developments of the PUNCH4NFDI Compute and Storage Infrastructures DOI ↗
- 2024 Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS DOI ↗
- 2024 Insights from super-metal-rich stars: Is the Milky Way bar young? DOI ↗