Anna is a postdoctoral researcher in the High-Energy Astrophysics group at the Department of Theoretical Physics and Astrophysics, Masaryk University in Brno, Czechia. She obtained her Ph.D. in 2022 from the Jagiellonian University in Cracow, Poland. In her research, Anna focuses on radio galaxies at various stages of their evolution: from the youngest compact-symmetric objects to giant radio galaxies and even sources with intermittent activity. In her research, she utilizes the multi-waveband archival data in an appraoch to investigate the jet production efficiencies and jet duty cycle.
In her spare time Anna enjoys rock climbing and hiking in the mountains.
| 10/2022 | PhD in Astronomy “Radio Emission in early-type galaxies: radio loudness, jet duty cycle and large-scale environment” at the Jagiellonian University in Cracow, Poland; PhD advisors: Assoc. Prof. Dr. Łukasz Stawarz |
| 06/2017 | MSc in Astronomy “The luminosity profile analysis of the host galaxies of the radio sources w X-shape and double-double morphology. ” at the Jagiellonian University in Cracow, Poland; Supervisor: Dr. Dorota Kozieł-Wierzbowska |
| 09/2015 | BSc in Astronomy “Analysis of the optical spectra of radio galaxies with restarting activity. ” at the Jagiellonian University in Cracow, Poland; Supervisor: Dr. Dorota Kozieł-Wierzbowska |
| since 2022 | Postdoctoral researcher in the High-Energy Astrophysics group, Department of Theoretical Physics and Astrophysics at the Masaryk University, Brno, Czech Republic |
Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
(arXiv).
A Novel Method for Estimating the Ambient Medium Density Around Distant Radio Sources from Their Observed Radio Spectra
(arXiv).
Mid-infrared Diagnostics of the Circumnuclear Environments of the Youngest Radio Galaxies
(arXiv).
On the Jet Production Efficiency in a Sample of the Youngest Radio Galaxies
(arXiv).
What Distinguishes the Host Galaxies of Radio-loud and Radio-quiet AGNs?
(arXiv).
For a complete list of publications see here.