Dan Hu received her PhD in 2021 at Shanghai Jiao Tong University, China. Her research focuses on studying the galaxy
clusters and groups, particularly in the areas of the merger dynamics, chemical enrichment, and diffuse radio structures,
by utilising the multi-wavelength (X-ray, radio and optical) observations and the smoothed particle hydrodynamic (SPH) simulations.
| 6/2021 | PhD in Astronomy “An X-ray Study of Galaxy Cluster Mergers and Their Effects on the ICM Chemical Evolution” at Shanghai Jiao Tong University, Shanghai, China; PhD advisor: Dr. H.G. Xu |
| since 2021 | Postdoctoral Researcher in the Department of Theoretical Physics and Astrophysics at Masaryk University, Brno, Czech Republic |
Ram-pressure stripped radio tail and two ULXs in the spiral galaxy HCG 97b
(arXiv).
The Merger Dynamics of the Galaxy Cluster A1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a Wide-angle Tail and a Narrow-angle Tail Radio Source (arXiv).
A Study of the Merger History of the Galaxy Group HCG 62 Based on X-Ray Observations and Smoothed Particle Hydrodynamic Simulations (arXiv).
A Study of Gas Entropy Profiles of 47 Galaxy Clusters and Groups out to the Virial Radius (arXiv).
Contribution of Radio Halos to the Foreground for SKA EoR Experiments
(arXiv).
A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best-Heckman Sample
(arXiv).
For a complete list of publications see here.