Annalisa Pillepich

Max Planck Institute for Astronomy — Germany

Physics and Astronomy · Physical Sciences

70h-index27.2kcitations328works7.72yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(250), Astronomy and Astrophysical Research(187), Stellar, planetary, and galactic studies(80), Astrophysics and Star Formation Studies(59), Astrophysical Phenomena and Observations(41)

Publications324 total

The temperature and metallicity distributions of the ICM: insights with TNG-Cluster for <i>XRISM</i> -like observations
Monthly Notices of the Royal Astronomical Society·2026· 1 citedOpen Access
Magnetic fields in the intracluster medium with TNG-Cluster: Properties, morphology, and tangential anisotropy
Astronomy and Astrophysics·2025· 2 citedOpen Access
Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters
arXiv (Cornell University)·2025Open Access
X-ray shocks in the cool cores of galaxy clusters: insights from TNG-Cluster
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
Exploring the statistical properties of double radio relics in the TNG-Cluster and TNG300 simulations
arXiv (Cornell University)·2025Open Access
Mass proxy quality of massive halo properties in the <scp>illustrisTNG</scp> and <scp>flamingo</scp> simulations: I. Hot gas
Monthly Notices of the Royal Astronomical Society·2025· 2 citedOpen Access
The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
Astronomy and Astrophysics·2025· 1 citedOpen Access
Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
The Astrophysical Journal·2025· 1 citedOpen Access
Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
ArXiv.org·2025Open Access
What drives cluster cool-core transformations? A population-level analysis using TNG-Cluster
Astronomy and Astrophysics·2025· 3 citedOpen Access
Jellyfish galaxies with the IllustrisTNG simulations – Supermassive black hole activity in dense environments with ram-pressure stripped satellites
Monthly Notices of the Royal Astronomical Society·2025· 3 citedOpen Access
Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
ArXiv.org·2025Open Access
Extragalactic stellar tidal streams: Observations meet simulation
Astronomy and Astrophysics·2025· 5 citedOpen Access
Mass Proxy Quality of Massive Halo Properties in the IllustrisTNG and FLAMINGO Simulations: I. Hot Gas
arXiv (Cornell University)·2025Open Access
Photometric analysis of the intracluster light in the TNG300 simulation and wide-field observations
Monthly Notices of the Royal Astronomical Society·2025· 2 citedOpen Access
Modelling the selection of galaxy groups with end-to-end simulations
Astronomy and Astrophysics·2025· 2 citedOpen Access
Intra-cluster light as a dynamical clock for galaxy clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea, and Horizon-AGN simulations
Astronomy and Astrophysics·2025· 4 citedOpen Access
The diverse physical origins of stars in the dynamically hot bulge: CALIFA versus IllustrisTNG
Astronomy and Astrophysics·2025· 4 citedOpen Access
Introducing the AIDA-TNG project: Galaxy formation in alternative dark matter models
Astronomy and Astrophysics·2025· 13 citedOpen Access
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Frequent Co-authors

Mark Vogelsberger(44), Dylan Nelson(43), Lars Hernquist(43), Volker Springel(34), Shy Genel(34), Federico Marinacci(32), Paul Torrey(31), Rainer Weinberger(27), Rüdiger Pakmor(23), Jill Naiman(13), Vicente Rodríguez-Gómez(13), Laura V. Sales(9), Debora Sijacki(6), Gregory F. Snyder(6), Benedikt Diemer(5), Chung‐Pei Ma(5), Sandro Tacchella(4), Martina Donnari(4), Sarah Wellons(3), Jennifer M. Lotz(3)