Dust grain size distributions evolve from large-grain dominated at high redshift to MRN-like at low redshift, driven primarily by shattering and ISM accretion after stars supply initial large grains, reproducing z=0 dust masses and Milky Way extinction properties.
The impact of binary stars on the dust and metal evolution of galaxies
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Different SED fitting techniques and data types produce stellar parameters and xi_ion values differing by up to 1.1 dex even for a homogeneous sample of z=3 EoR-analog galaxies, with apparent redshift evolution of xi_ion appearing only under consistent methodology.
A unified JSONL/CSV corpus merges photometric, kinematic, dynamical, and chemical parameters for all 174 Milky Way globular clusters from Harris, Gaia EDR3, Baumgardt N-body, and APOGEE DR17 surveys.
The paper reviews dust production, destruction and growth processes in galaxies, compiles literature data on comoving dust mass density, presents evidence for and against interstellar dust growth, and identifies the high-redshift dust budget as needing further study.
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A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications
A unified JSONL/CSV corpus merges photometric, kinematic, dynamical, and chemical parameters for all 174 Milky Way globular clusters from Harris, Gaia EDR3, Baumgardt N-body, and APOGEE DR17 surveys.