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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Global canopy height regression and uncertainty estimation from GEDI LIDAR waveforms with deep ensembles. Remote Sensing of Environment, 268:112760.
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An upper limit on late accretion and water delivery in the TRAPPIST-1 exoplanet system. Nature Astronomy, 6(1):80-88.
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The Compositions and Interior Structures of Terrestrial Planets and Water-Worlds. 2022, University of Zurich, Mathematisch-naturwissenschaftliche Fakultät.
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The growth of supermassive black holes and their host galaxies in cosmological simulations. 2022, University of Zurich, Faculty of Science.
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Dominant-feature identification in data from Gaussian processes applied to Finnish forest inventory records. ArXiv.org 2203.03322, Cornell University.
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BiasBed -- Rigorous Texture Bias Evaluation. ArXiv.org 2211.13190, Cornell University.
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On the orthogonality of zero-mean Gaussian measures: Sufficiently dense sampling. ArXiv.org 2212.10239, Cornell University.
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Theory and applications of multivariate conditional transformation models. 2022, University of Zurich, Medizinische Fakultät.
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Identifying features in spatial data on different scales of variation with ecological applications. 2022, University of Zurich, Mathematisch-naturwissenschaftliche Fakultät.
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Quantification of sensitivity and empirical determinancy in Bayesian hierarchical models. 2022, University of Zurich, Mathematisch-naturwissenschaftliche Fakultät.
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Eccentricity driving of pebble accreting low-mass planets. Monthly Notices of the Royal Astronomical Society, 509(4):5622-5635.
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A wide-orbit giant planet in the high-mass b Centauri binary system. Nature, 600(7888):231-234.
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Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations. Monthly Notices of the Royal Astronomical Society, 501(2):1591-1602.
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Mixed dark matter: matter power spectrum and halo mass function. Journal of Cosmology and Astroparticle Physics, 2021(12):044.
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Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data. Journal of Cosmology and Astroparticle Physics, 2021(12):046.
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Cosmological simulations of number counts. Journal of Cosmology and Astroparticle Physics, 2021(12):021.
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Digital taxonomist: Identifying plant species in community scientists’ photographs. ISPRS Journal of Photogrammetry and Remote Sensing, 182:112-121.
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From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning. Monthly Notices of the Royal Astronomical Society, 509(1):1323-1341.
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The baryon cycle of Seven Dwarfs with superbubble feedback. ArXiv.org 06646, Cornell University.
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Euclid preparation : XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses. Astronomy and Astrophysics, 655:A44.
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Hidden Water in Magma Ocean Exoplanets. Astrophysical Journal Letters, 922:L4.
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General relativistic effects in weak lensing angular power spectra. Physical review D, 104:083548.
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Robust Damage Estimation of Typhoon Goni on Coconut Crops with Sentinel-2 Imagery. Remote Sensing, 13(21):4302.
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Pure Lorentz spin connection theories and uniqueness of general relativity. Classical and quantum gravity, 38(20):205009.
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Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations. Monthly Notices of the Royal Astronomical Society, 508(2):2979-3008.
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A compositional link between rocky exoplanets and their host stars. Science, 374(6565):330-332.
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Decaying dark matter: simulations and weak-lensing forecast. Journal of Cosmology and Astroparticle Physics, 2021(10):040.
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The Hessigheim 3D (H3D) benchmark on semantic segmentation of high-resolution 3D point clouds and textured meshes from UAV LiDAR and Multi-View-Stereo. ISPRS Open Journal of Photogrammetry and Remote Sensing, 1:100001.
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Applying deep neural networks to predict incidence and phenology of plant pests and diseases. Ecosphere, 12(10):e03791.
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TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet. Monthly Notices of the Royal Astronomical Society, 507(2):2782-2803.
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Euclid Preparation : XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3. Astrophysical Journal Supplement Series, 256(1):9.
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TESS and HARPS reveal two sub-Neptunes around TOI 1062. Astronomy and Astrophysics, 653:A105.
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Synthetic evolution tracks of giant planets. Monthly Notices of the Royal Astronomical Society, 507(2):2094-2102.
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Combining heterogeneous spatial datasets with process-based spatial fusion models: A unifying framework. Computational Statistics & Data Analysis, 161:107240.
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Linking Uranus’ temperature profile to wind-induced magnetic fields. Monthly Notices of the Royal Astronomical Society, 507(1):1485-1490.
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Which AGN jets quench star formation in massive galaxies?. Monthly Notices of the Royal Astronomical Society, 507(1):175-204.
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Maximum accretion rate of supermassive stars. Astronomy and Astrophysics, 652:L7.
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Maximum accretion rate of supermassive stars. ArXiv.org 13373, Cornell University.
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Compositional Diversity of Rocky Exoplanets. Elements (Quebec), 17(4):235-240.
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Mapping oil palm density at country scale: An active learning approach. Remote Sensing of Environment, 261:112479.
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Domain Adaptation for Semantic Segmentation of Historical Panchromatic Orthomosaics in Central Africa. ISPRS International Journal of Geo-Information, 10(8):523.
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Why do more massive stars host larger planets?. Astronomy and Astrophysics, 652:A110.
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Discussion on competition for spatial statistics for large datasets. Journal of agricultural, biological, and environmental statistics, (26):599-603.
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Remotely sensed between‐individual functional trait variation in a temperate forest. Ecology and Evolution, 11(16):10834-10867.
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Galaxy formation across scales : from small vortices to large discs. 2021, University of Zurich, Faculty of Science.
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Improved gravitational radiation time-scales II: Spin–orbit contributions and environmental perturbations. Monthly Notices of the Royal Astronomical Society, 506(1):1007-1018.
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Light, medium-weight, or heavy? The nature of the first supermassive black hole seeds. Monthly Notices of the Royal Astronomical Society, 506(1):613-632.
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Revisiting Dynamical Friction: The Role of Global Modes and Local Wakes. The Astrophysical Journal, 916(1):55.
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Bayesian spatial modelling of terrestrial radiation in Switzerland. Journal of Environmental Radioactivity, 233:106571.
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3D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging. Monthly Notices of the Royal Astronomical Society, 505(3):4586-4607.
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Association between environmental and climatic risk factors and the spatial distribution of cystic and alveolar echinococcosis in Kyrgyzstan. PLoS Neglected Tropical Diseases, 15(6):e0009498.
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Euclid preparation : IX. EuclidEmulator2 – power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations. Monthly Notices of the Royal Astronomical Society, 505(2):2840-2869.
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The EOS/resolution conspiracy: convergence in proto-planetary collision simulations. Monthly Notices of the Royal Astronomical Society, 505(2):1806-1816.
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Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy, 51(3):1333-1383.
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Toward a Collective Agenda on AI for Earth Science Data Analysis. Proceedings of the IEEE, 9(2):88-104.
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TOI-269 b: an eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA. Astronomy and Astrophysics, 650:A145.
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rasterdiv—An Information Theory tailored R package for measuring ecosystem heterogeneity from space: To the origin and back. Methods in Ecology and Evolution, 12(6):1093-1102.
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The bursty origin of the Milky Way thick disc. Monthly Notices of the Royal Astronomical Society, 505(1):889-902.
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An N-body population synthesis framework for the formation of moons around Jupiter-like planets. Monthly Notices of the Royal Astronomical Society, 504(4):5455-5474.
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GRAINet: mapping grain size distributions in river beds from UAV images with convolutional neural networks. Hydrology and Earth System Sciences, 25(5):2567-2597.
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Dark acoustic oscillations: imprints on the matter power spectrum and the halo mass function. Monthly Notices of the Royal Astronomical Society, 504(3):3773-3786.
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Observing relativistic features in large-scale structure surveys – II. Doppler magnification in an ensemble of relativistic simulations. Monthly Notices of the Royal Astronomical Society, 504(3):3534-3543.
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Growing Mars fast: High-resolution GPU simulations of embryo formation. Icarus, 359:114305.
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The Alfvénic nature of chromospheric swirls. Astronomy and Astrophysics, 649:A121.
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Formation of intermediate-mass planets via magnetically controlled disk fragmentation. Nature Astronomy, 5(5):440-444.
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Halo model approach for the 21-cm power spectrum at cosmic dawn. Physical review D, 103(8):083025.
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Deformations of GR, geometrodynamics and reality conditions. Classical and quantum gravity, 38(8):085009.
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Mars' Formation Can Constrain the Primordial Orbits of the Gas Giants. Astrophysical Journal Letters, 910(2):L16.
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Virialization of the Inner CGM in the FIRE Simulations and Implications for Galaxy Disks, Star Formation, and Feedback. The Astrophysical Journal, 911(2):88.
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Searching for gravitational waves via Doppler tracking by future missions to Uranus and Neptune. Monthly Notices of the Royal Astronomical Society. Letters, 503(1):L73-L79.
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Monopole fluctuation of the CMB and its gauge invariance. Physical review D, 103(6):063516.
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From zero to infinity: Minimum to maximum diversity of the planet by spatio‐parametric Rao’s quadratic entropy. Global Ecology and Biogeography, 30(5):1153-1162.
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Out of sight, out of mind? The impact of correlated clustering in substructure lensing. Monthly Notices of the Royal Astronomical Society, 502(4):6064-6079.
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Cutting out the cosmological middle man: general relativity in the light-cone coordinates. Classical and quantum gravity, 38(5):055011.
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The Origin and Evolution of Lyα Blobs in Cosmological Galaxy Formation Simulations. The Astrophysical Journal, 909(2):119.
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The Star Formation History of Eridanus II: On the Role of Supernova Feedback in the Quenching of Ultrafaint Dwarf Galaxies. The Astrophysical Journal, 909(2):192.
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Euclid preparation : XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography. Astronomy and Astrophysics, 647:A117.
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Connecting the Gravity Field, Moment of Inertia, and Core Properties in Jupiter through Empirical Structural Models. The Astrophysical Journal, 910(1):38.
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Identification of dominant features in spatial data. Spatial Statistics, 41:100483.
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30 Years of space–time covariance functions. Wiley Interdisciplinary Reviews: Computational Statistics, 13(2):e1512.
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A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113. Monthly Notices of the Royal Astronomical Society, 502(4):4842-4857.
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The IRX–β relation of high-redshift galaxies. Monthly Notices of the Royal Astronomical Society, 502(3):3210-3241.
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Old and new major mergers in the SOSIMPLE galaxy, NGC 7135. Monthly Notices of the Royal Astronomical Society, 502(2):2296-2307.
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Could Uranus and Neptune form by collisions of planetary embryos?. Monthly Notices of the Royal Astronomical Society, 502(2):1647-1660.
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BEAST begins: Sample characteristics and survey performance of the B-star Exoplanet Abundance Study. ArXiv.org 02043, Cornell University.
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Internal water storage capacity of terrestrial planets and the effect of hydration on the M-R relation. Astronomy and Astrophysics, 646:A162.
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Science Goals and Mission Objectives for the Future Exploration of Ice Giants Systems: A Horizon 2061 Perspective. Space Science Reviews, 217(1):3.
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Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides. Planetary Science Journal, 2:1.
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Observing relativistic features in large-scale structure surveys – I. Multipoles of the power spectrum. Monthly Notices of the Royal Astronomical Society, 501(2):2547-2561.
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The influence of infall on the properties of protoplanetary discs. Astronomy and Astrophysics, 645:A43.
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The Evolution of Giant Planets – Towards a Better Understanding of Gas Giants in- and outside the Solar System. 2021, University of Zurich, Faculty of Science.
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Advances in Giant Planet Formation Theory. 2021, University of Zurich, Faculty of Science.
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General Relativistic Effects in Cosmological Weak Lensing. 2021, University of Zurich, Faculty of Science.
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Asymptotic analysis of ML-covariance parameter estimators based on covariance approximations. ArXiv.org 2112.12317, Cornell University.
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Blinded study: prospectively defined high-frequency oscillations predict seizure outcome in individual patients. Brain Communications, 3(3):fcab209.
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Neptune and Uranus: ice or rock giants?. Philosophical Transactions of the Royal Society of London, Series A: Mathematical, Physical and Engineering Sciences, 378(2187):20190489.
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The interiors of Uranus and Neptune: current understanding and open questions. Philosophical Transactions of the Royal Society of London, Series A: Mathematical, Physical and Engineering Sciences, 378(2187):20190474.
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The role of ice lines in the formation of Uranus and Neptune. Philosophical Transactions of the Royal Society of London, Series A: Mathematical, Physical and Engineering Sciences, 378(2187):20200107.