Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H\(\alpha\) and [O III] emitters
Shuntov et al. 2025, A&A 699, A231
CV
Education
- Ph.D in Astrophysics, Sorbonne Université / Institut d’Astrophysique de Paris, 2022
- M.S. in Physics, University of Zagreb, 2018
- B.S. in Physics, University of Zagreb, 2016
Work experience
- 2022 – present: Postdoctoral Researcher
- Cosmic DAWN Center, Niels Bohr Institute / University of Copenhagen
- Galaxy formation and evolution, multi-band imaging surveys, machine learning
Publications
COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging
Shuntov et al. 2025, A&A subm
The COSMOS-Web ring: Spectroscopic confirmation of the background source at \(z = 5.1\)
Shuntov et al. 2025, A&A 696, L14
COSMOS-Web: Stellar mass assembly in relation to dark matter halos across \(0.2 < z < 12\) of cosmic history
Shuntov et al. 2025 A&A 695, A20
COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z ∼ 5
Shuntov et al. 2022 A&A 664, A61
PhotoWeb redshift: boosting photometric redshift accuracy with large spectroscopic surveys
Shuntov et al. 2025, A&A 636, A90
Talks
Galaxy growth in dark matter halos – insights from COSMOS-Web and FRESCO
Talk at 40th IAP Symposium, Institut d'Astrophysique de Paris, Paris, France
Tutorial 1 on Relevant Topic in Your Field
Tutorial at UC-Berkeley Institute for Testing Science, Berkeley CA, USA