Publications
ADS
For a list of Publications from the Astrophysics Data System, 2014 - present, click here: ADS search
ZORA
Publications are displayed in reverse chronological order. ICS Publications begin in 2014.
In 2024 our affiliation changed to Department of Astrophysics.
Earlier publications from the Institute for Theoretical Physics can be found here.
ZORA Publication List
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Publications
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Non-isotropic feedback from accreting spinning black holes Monthly Notices of the Royal Astronomical Society, 500(4):4788-4800.
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Generation of gravitational waves and tidal disruptions in clumpy galaxies Monthly Notices of the Royal Astronomical Society, 500(4):4628-4638.
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Clustering dark energy imprints on cosmological observables of the gravitational field Monthly Notices of the Royal Astronomical Society, 500(4):4514-4529.
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Parametric instability in a free-evolving warped protoplanetary disc Monthly Notices of the Royal Astronomical Society, 500(3):4248-4256.
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Black hole spin evolution in warped accretion discs Monthly Notices of the Royal Astronomical Society, 500(3):3719-3727.
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Deep, wide lensing surveys can measure the dark matter halos of dwarf galaxies Physics of the Dark Universe, 30:100719.
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Euclid preparation : X. The Euclid photometric-redshift challenge Astronomy and Astrophysics, 644:A31.
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Machine learning applied to simulations of collisions between rotating, differentiated planets Computational Astrophysics and Cosmology, 7(1):2.
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Fingerprints of a second order critical line in developing neural networks Communications Physics, 3(1):13.
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The link between star formation and gas in nearby galaxies Communications Physics, 3:226.
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Galaxy power spectrum in general relativity Journal of Cosmology and Astroparticle Physics, 2020(11):064.
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No Evidence for [C ii] Halos or High-velocity Outflows in z gsim 6 Quasar Host Galaxies The Astrophysical Journal, 904(2):131.
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Bifurcation in the history of Uranus and Neptune: the role of giant impacts Monthly Notices of the Royal Astronomical Society, 492(4):5336-5353.
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Stellar and weak lensing profiles of massive galaxies in the Hyper-Suprime Cam survey and in hydrodynamic simulations Monthly Notices of the Royal Astronomical Society, 500(1):432-447.
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Theoretical versus Observational Uncertainties: Composition of Giant Exoplanets The Astrophysical Journal, 903(2):147.
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Earth as an Exoplanet. I. Time Variable Thermal Emission Using Spatially Resolved Moderate Imaging Spectroradiometer Data Astronomical Journal, 160(6):246.
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The influence of bulk composition on the long-term interior-atmosphere evolution of terrestrial exoplanets Astronomy and Astrophysics, 643:A44.
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Disk dominated galaxies retain their shapes below z=1.0 ArXiv.org 13845, Cornell University.
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Formation of satellites in circumplanetary discs generated by disc instability Monthly Notices of the Royal Astronomical Society, 499(1):1023-1036.
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Positive feedback at the disc–halo interface Monthly Notices of the Royal Astronomical Society, 498(1):1140-1158.
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Constraining the depth of the winds on Uranus and Neptune via Ohmic dissipation Monthly Notices of the Royal Astronomical Society, 498(1):621-638.
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Reproducing the CO-to-H2 conversion factor in cosmological simulations of Milky-Way-mass galaxies Monthly Notices of the Royal Astronomical Society, 499(1):837-850.
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Advancing texture metrics to model landscape heterogeneity In: IGARSS 2020 - 2020 IEEE International Geoscience and Remote Sensing Symposium, Waikoloa, HI, USA, 26 September 2020 - 2 October 2020, 2735-2738.
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Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies Monthly Notices of the Royal Astronomical Society, 497(4):4051-4065.
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Understanding dense hydrogen at planetary conditions Nature Reviews. Physics, 2(10):562-574.
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The impact of AGN wind feedback in simulations of isolated galaxies with a multiphase ISM Monthly Notices of the Royal Astronomical Society, 497(4):5292-5308.
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Ice Giant Systems: The scientific potential of orbital missions to Uranus and Neptune Planetary and Space Science, 191:105030.
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The relativistic galaxy number counts in the weak field approximation Journal of Cosmology and Astroparticle Physics, 2020(09):058.
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Towards a polarization prediction for LISA via intensity interferometry Monthly Notices of the Royal Astronomical Society, 498(3):4577-4589.
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Tight constraints on the excess radio background at z = 9.1 from LOFAR. Monthly Notices of the Royal Astronomical Society, 498(3):4178-4191.
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Weak-lensing observables in relativistic N-body simulations Monthly Notices of the Royal Astronomical Society, 497(2):2078-2095.
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Giant Planet Formation Models with a Self-consistent Treatment of the Heavy Elements The Astrophysical Journal, 900(2):133.
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TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert Astronomical Journal, 160(4):153.
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Steady Wind-blown Cavities within Infalling Rotating Envelopes: Application to the Broad Velocity Component in Young Protostars The Astrophysical Journal, 900(1):15.
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Lithologic Controls on Silicate Weathering Regimes of Temperate Planets ArXiv.org 11620, Cornell University.
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Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe Monthly Notices of the Royal Astronomical Society, 498(3):3601-3615.
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Cosmic Dawn II (CoDa II): a new radiation-hydrodynamics simulation of the self-consistent coupling of galaxy formation and reionization Monthly Notices of the Royal Astronomical Society, 496(4):4087-4107.
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Origin of star-forming rings around massive centres in massive galaxies at z < 4 Monthly Notices of the Royal Astronomical Society, 496(4):5372-5398.
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Galactic ionizing photon budget during the epoch of reionization in the Cosmic Dawn II simulation Monthly Notices of the Royal Astronomical Society, 496(4):4342-4357.
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Predicting dark matter halo formation in N-body simulations with deep regression networks Monthly Notices of the Royal Astronomical Society, 496(4):5116-5125.
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The Erratic Path to Coalescence of LISA Massive Black Hole Binaries in Subparsec-resolution Simulations of Smooth Circumnuclear Gas Disks The Astrophysical Journal, 899(2):126.
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Detailed Calculations of the Efficiency of Planetesimal Accretion in the Core-accretion Model The Astrophysical Journal, 899(1):45.
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Tools21cm: A python package to analyse the large-scale 21-cm signal from the Epoch of Reionization and Cosmic Dawn Journal of Open Source Software, 5(52):2363.
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The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuIGG$\vec{L}$E Survey Astrophysical Journal Letters, 899(1):L9.
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Numerical solutions to Einstein’s equations in a shearing-dust universe: a code comparison Classical and quantum gravity, 37(15):154001.
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Rapid Filamentary Accretion as the Origin of Extended Thin Discs Monthly Notices of the Royal Astronomical Society, 487(4):43464-4356.
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TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet Astronomical Journal, 160(2):96.
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Updated Equipotential Shapes of Jupiter and Saturn Using Juno and Cassini Grand Finale Gravity Science Measurements JGR: Planets, 125(8):e2019JE006354.
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Impact of the measured parameters of exoplanets on the inferred internal structure Astronomy and Astrophysics, 640:A135.
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Modeling relativistic contributions to the halo power spectrum dipole Journal of Cosmology and Astroparticle Physics, 2020(07):048.
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Generation and application of river network analogues for use in ecology and evolution Ecology and Evolution, 10(14):7537-7550.
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A remnant planetary core in the hot-Neptune desert Nature, 583(7814):39-42.
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General and consistent statistics for cosmological observations Physical review research, 2(3):033004.
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The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies Monthly Notices of the Royal Astronomical Society, 495(3):3002-3013.
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Vortices evolution in the solar atmosphere Astronomy and Astrophysics, 639:A118.
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The challenge of forming a fuzzy core in Jupiter Astronomy and Astrophysics, 638:A121.
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Dynamical friction with radiative feedback – II. High-resolution study of the subsonic regime Monthly Notices of the Royal Astronomical Society, 495(2):2063-2074.
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Euclid: Reconstruction of weak-lensing mass maps for non-Gaussianity studies Astronomy and Astrophysics, 638:A141.
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Formation of the First Stars and Black Holes Space Science Reviews, 216(4):48.
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Estimating the integrated bispectrum from weak lensing maps Journal of Cosmology and Astroparticle Physics, 2020(05):043.
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Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources Monthly Notices of the Royal Astronomical Society, 495(2):2321-2331.
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Report from the Tri-Agency Cosmological Simulation Task Force ArXiv.org 2005-07281, Cornell University.
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Second-order phase transition in phytoplankton trait dynamics Chaos (Woodbury, N.Y.), 30(5):053109.
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TW Hya: an old protoplanetary disc revived by its planet Monthly Notices of the Royal Astronomical Society, 495(1):285-304.
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Parametrising non-linear dark energy perturbations Journal of Cosmology and Astroparticle Physics, 2020(04):039.
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Constraining the intergalactic medium at z ≈ 9.1 using LOFAR Epoch of Reionization observations Monthly Notices of the Royal Astronomical Society, 493(4):4728-4747.
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Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix Journal of Cosmology and Astroparticle Physics, 2020(04):019.
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Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies Journal of Cosmology and Astroparticle Physics, 2020(04):020.
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Dynamical friction-driven orbital circularization in rotating discs: a semi-analytical description Monthly Notices of the Royal Astronomical Society, 494(2):3053-3059.
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The impact of relativistic effects on the 3D Quasar-Lyman-α cross-correlation Journal of Cosmology and Astroparticle Physics, 2020(04):006.
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Uranus and Neptune: Origin, Evolution and Internal Structure Space Science Reviews, 216(3):38.
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The loss of the intracluster medium in globular clusters Monthly Notices of the Royal Astronomical Society, 493(1):1306-1316.
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Global Simulations of Self-gravitating Magnetized Protoplanetary Disks The Astrophysical Journal, 891(2):154.
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Improved constraints from ultra-faint dwarf galaxies on primordial black holes as dark matter Monthly Notices of the Royal Astronomical Society, 492(4):5247-5260.
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Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures The Astrophysical Journal, 891(2):109.
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Mass determinations of the three mini-Neptunes transiting TOI-125 Monthly Notices of the Royal Astronomical Society, 492(4):5399-5412.
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On the origin of the peak of the stellar initial mass function: exploring the tidal screening theory Monthly Notices of the Royal Astronomical Society, 492(4):4727-4751.
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Bayesian Network Modeling applied to Feline Calicivirus Infection among cats in Switzerland Frontiers in Veterinary Science, 7:73.
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Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation Monthly Notices of the Royal Astronomical Society, 492(1):1385-1398.
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Maximum cosmological information from type Ia supernova observations Physical review D, 101(4):043507.
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Revisited mass-radius relations for exoplanets below 120 M⊕ Astronomy and Astrophysics, 634:A43.
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Jupiter’s heavy-element enrichment expected from formation models Astronomy and Astrophysics, 634:A31.
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Ray tracing the integrated Sachs-Wolfe effect through the light cones of the dark energy universe simulation-full universe runs Physical review D, 101(2):023512.
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EDGE: the mass–metallicity relation as a critical test of galaxy formation physics Monthly Notices of the Royal Astronomical Society, 491(2):1656-1672.
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HD 213885b: a transiting 1-d-period super-Earth with an Earth-like composition around a bright (V = 7.9) star unveiled by TESS Monthly Notices of the Royal Astronomical Society, 491(2):2982-2999.
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Dynamics of Massive Black Hole Binaries in Circumnuclear Discs 2020, University of Zurich, Faculty of Science.
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Emulation of Planetary-Scale Collisions – Artifcially Intelligent Collision Handling in N-body Simulations 2020, University of Zurich, Faculty of Science.
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The Origin of Lyman Alpha Blobs in Cosmological Galaxy Formation Simulations ArXiv.org 08397, Cornell University.
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Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution Astronomy and Astrophysics, 633:A50.
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Monte Carlo permutation tests for assessing spatial dependence at different scales In: La Rocca, Michele; Brunero, Liseo; Salmaso, Luigi . Nonparametric Statistics. ISNPS 2018. Cham, Switzerland, 503-511.
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The Role of Giant Impacts on Mercury, Uranus and Neptune 2020, University of Zurich, Faculty of Science.
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Tetrad Formalism for Exact Cosmological Observables Switzerland: Springer.
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Exploring Models of Lensing Galaxies – On Bridging the Gap between Observations, Models, and Simulations 2020, University of Zurich, Faculty of Science.
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High-Fidelity Emulation of Non-Linear Cosmic Large-Scale Structure 2020, University of Zurich, Faculty of Science.
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The Composition and Internal Structure of Intermediate-mass Exoplanets 2020, University of Zurich, Faculty of Science.
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Asymptotic properties of the maximum likelihood and cross validation estimators for transformed Gaussian processes Electronic Journal of Statistics, 14(1):1962-2008.
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Epidemic cystic and alveolar echinococcosis in Kyrgyzstan: an analysis of national surveillance data The Lancet Global Health, 8(4):e603-e611.
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The origin of the high metallicity of close-in giant exoplanets Astronomy and Astrophysics, 633:A33.
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The Origin of the Stellar Initial Mass Function 2020, University of Zurich, Faculty of Science.