DP
Douglas Potter
University of Zurich
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Cosmology and Gravitation Theories
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Education
Education history is unavailable.
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Publications (122)
- Euclid Save
- Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations Save
- Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength Save
- Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. I. Hydrodynamics Save
- Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation Save
- Euclid preparation. Far-infrared predictions for Euclid galaxy catalogues: cluster, protocluster, and field Save
- Euclid preparation. Simulated galaxy catalogues for non-standard cosmological models Save
- Euclid preparation: LXXIX. Using mock low surface brightness dwarf galaxies to probe Euclid Wide Survey detection capabilities Save
- Euclid preparation: LXXVIII. Full-shape modelling of two-point and three-point correlation functions in real space Save
- Euclid preparation: LXXX. Overview of Euclid infrared detector performance from ground tests Save
- Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images Save
- Euclid preparation: LXXXII. Predicting star-forming galaxy scaling relations with the spectral stacking code SpectraPyle Save
- Euclid preparation: LXXXIII. The impact of redshift interlopers on the two-point correlation function analysis Save
- Euclid preparation: LXXXIV. The flat-sky approximation for the clustering of Euclid's photometric galaxies Save
- Euclid preparation: LXXXV. Toward a DR1 application of higher-order weak lensing statistics Save
- Euclid preparation: XXVII. The NISP spectroscopy channel: Ground performance and calibration Save
- Euclid: VI. NISP-P optical ghosts Save
- Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength Save
- Euclid preparation: LXXVI. Simulating thousands of Euclid spectroscopic skies Save
- Euclid preparation: LXXIII. Spatially resolved stellar populations of local galaxies with Euclid: A proof of concept using synthetic images with the TNG50 simulation Save