{"arxiv_id":"0709.0292","incoming":{"papers":22,"sentences":26,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":13,"sentences":15,"quotes":[{"arxiv_id":"2605.11083","title":"FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics","url":"/paper/2605.11083","section":"simulations","sentence":"The simulations include radiative cooling and heating [ref] , star formation and evolution [ref] , black hole growth [ref] , feedback from young stars and supernovae [ref] , and AGN feedback [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"1601.04707","title":"Simulated Milky Way analogues: implications for dark matter direct searches","url":"/paper/1601.04707","section":"Simulations","sentence":"The project combines a state-of-the-art hydrodynamical SPH implementation nicknamed anarchy [ref] – built on top of an optimized version of the gadget SPH code, last described by [ref] – and a 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IMF."},{"p":0.89,"quote":null,"citing":[{"self":false,"year":2024,"title":"Interplay of Stellar and Gas-Phase Metallicities: Unveiling Insights for Stellar Feedback Modeling with Illustris, IllustrisTNG, and EAGLE","arxiv_id":"2401.12310"}],"verified":true,"paraphrase":"Treated the dense unresolved ISM with a sub-grid equation of state much like that of this paper."},{"p":0.98,"quote":null,"citing":[{"self":false,"year":2018,"title":"The impact of assembly bias on the halo occupation in hydrodynamical simulations","arxiv_id":"1805.06938"}],"verified":true,"paraphrase":"Followed the pressure-dependent Kennicutt-Schmidt relation from this paper and the metallicity-dependent density threshold of another work."},{"p":0.81,"quote":null,"citing":[{"self":false,"year":2021,"title":"{\\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning","arxiv_id":"2101.04687"}],"verified":true,"paraphrase":"Converted gas particles into star particles at a pressure-dependent, gas temperature and density limited rate, following another work and this paper."},{"p":0.99,"quote":null,"citing":[{"self":false,"year":2019,"title":"The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy","arxiv_id":"1903.00485"}],"verified":true,"paraphrase":"Governed gas above a density threshold by an effective equation of state and formed stars following a Kennicutt-Schmidt relation, while at lower densities it followed an isothermal equation of state as in this paper."},{"p":0.99,"quote":null,"citing":[{"self":false,"year":2021,"title":"On the variation in stellar $\\alpha$-enhancements of star-forming galaxies in the EAGLE simulation","arxiv_id":"2102.04561"}],"verified":true,"paraphrase":"Implemented star formation according to this paper with a star formation rate following the empirical Kennicutt-Schmidt relation."},{"p":0.99,"quote":null,"citing":[{"self":false,"year":2022,"title":"Globular cluster metallicity distributions in the E-MOSAICS 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galaxies","arxiv_id":"1703.10907"}],"verified":true,"paraphrase":"Implemented star formation as a pressure law from this paper, subject to a metallicity-dependent density threshold from another work."},{"p":0.97,"quote":null,"citing":[{"self":true,"year":2024,"title":"The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST","arxiv_id":"2402.17819"}],"verified":true,"paraphrase":"Stochastically converted gas particles above a density threshold and pressure into stars to follow the star formation rate of this paper, designed to reproduce the Kennicutt-Schmidt law."},{"p":0.99,"quote":null,"citing":[{"self":true,"year":2015,"title":"Dark matter annihilation radiation in hydrodynamic simulations of Milky Way haloes","arxiv_id":"1509.02166"}],"verified":true,"paraphrase":"Applied a pressure floor in the form of an effective equation of state designed to mimic the mixture of ISM phases as in this paper to cold and dense 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