About
About the group
The energy output of actively accreting supermassive black holes (active galactic nuclei, AGN) has become a critical ingredient in modern galaxy formation theories and is widely considered a main driver in regulating the growth of massive galaxies. This energy typically exceeds the binding energy of a galaxy, so that even if only a few percent couples to the surrounding gas, that gas may be heated and driven out of the galaxy, effectively quenching star formation. The critical role of AGN in galaxy formation was hypothesised two decades ago, but specific observational evidence of AGN-driven feedback has been surprisingly hard to come by.
The group's research focuses on finding concrete observational evidence for the self-regulation of supermassive black holes and their host galaxies, on understanding the power, reach and impact of feedback processes exerted by AGN, and on the role of AGN in galaxy evolution across cosmic time. We aim to characterise the internal structure and multi-phase nature of AGN feedback signatures, determine outflow masses and energetics, and inventory the sources of gas excitation, using data from state-of-the-art ground- and space-based telescopes — including integral field unit observations from the JWST Early Release Science program Q3D and large spectroscopic surveys such as SDSS-V.
The group started its work in September 2020, initially funded through an Emmy Noether Grant of the Deutsche Forschungsgemeinschaft (DFG), with additional support from the Daimler und Benz Stiftung, the MERAC Foundation, the DLR and the BMBF/BMFTR.
Team
Team members
Group Lead & Science Staff
Prof. Dr. Dominika Wylezalek
Dr. Robert Schmidt
Postdocs
Dr. Caroline Bertemes
Dr. Pranav Kukreti
Dr. Bruno Dall’Agnol de Oliveira
Dr. Lara Gatto
Master Students
Delvin Demke
Virginia Lenk
Kalina Georgieva
Eleni Koustiona
Matthias Kuntz
Seraphin Bücklers
Bachelor Students
Theodor Brosi
Guests
Prof. Vivek Mariappan
Dr. Francisco Pozo-Núñez
Former Group Members
- Prof. Daniel Wik — visited on sabbatical, now back at the University of Utah
- Prof. David Rupke (Rhodes College, Tennessee, USA) — spent a one-year sabbatical in the group
- Daniela Müller-Trefzer, MSc
- Marco Albán, PhD — now postdoc at the Max Planck Institute for Radio Astronomy (MPIfR)
- Rodrigo Freitas, MSc — now PhD student at Universidade Federal do Rio Grande do Sul, Brazil
- Kolja Reuter, BSc & MSc
- Daniel Götz, MSc
- Stella Himmelsbach, BSc
- Naomi Tokar, BSc
- Greique Valk
- Eren Arici, BSc — now MSc student at Heidelberg University
- Julian Groth, MSc — now PhD student at Stockholm University
- Benjamin Beckmann, MSc
- Jelena Ritter, MSc — now PhD student at MPA Garching
- Dr. Wuji Wang — now postdoc at Caltech / IPAC
- Jan Beckmann, MSc
- Yu-Ruei Wang, BSc
- Payel Nandi, MSc — PhD student at IIA, Bangalore
- Simon Flesch, BSc — now PhD student at MPE
- Chuanming Mao — now MSc student at MPIA Heidelberg
News
Latest updates
Publications
Selected publications
Recent highlights (2025–2026)
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Exploring the gaseous halos of z > 3 radio galaxies with UVES and JWST/NIRSpec
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The eJWST active galactic nucleus observation catalogue
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SDSS-V Black Hole Mapper: the index diagram as a tool to disentangle the influence of the host galaxy in quasar spectra
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Optical emission line properties of eROSITA-selected SDSS-V galaxies
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JWST Q3D Program: Active Galactic Nucleus Photoionization and Shock Ionization in a Red Quasar at z = 0.4
Earlier selected publications
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JWST ERS Program Q3D: The pitfalls of virial BH mass constraints shown in a z = 3 quasar with an ultramassive host
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JWST discovers an AGN ionization cone but only weak radiatively driven feedback in a powerful z ≈ 3.5 radio-loud AGN
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3D tomography of the giant Lyα nebulae of z ≈ 3–5 radio-loud AGN
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Classifying the full SDSS-IV MaNGA Survey using optical diagnostic diagrams: presentation of AGN catalogs in flexible apertures
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MASCOT: molecular gas depletion times and metallicity gradients — evidence for feedback in quenching active galaxies
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First results from the JWST Early Release Science Program Q3D: Turbulent times in the life of a z ∼ 3 extremely red quasar revealed by NIRSpec IFU
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MASCOT — An ESO-ARO legacy survey of molecular gas in nearby SDSS-MaNGA galaxies: I. First data release, and global and resolved relations between H2 and stellar content
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Mapping the invisible circumgalactic medium around a z ~ 4.5 radio galaxy with MUSE
Contact
For questions, please contact
Dominika Wylezalek
Email: dominika.wylezalek@uni-heidelberg.de