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Complex distribution and velocity field of molecular gas in NGC 1316 as revealed by Morita Array of ALMA, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1905.11085Comment: 16 pages, 8 figures, 3 tables, accepted for publication in PASJ.The formation of UCDs and massive GCs: Quasar-like objects for testing for a variable stellar initial mass function (IMF), , , , and . (2017)cite arxiv:1708.07127Comment: Accepted for publication in A&A, 12 pages, 10 figures + appendix.Coevolution of dust, gas, and stars in galaxies - I. Spatial distributions and scaling-relations of dust and molecular hydrogen. (2013)cite arxiv:1304.1633Comment: 29 pages, 23 figures, accepted for publication in MNRAS.The AIverse project: Simulating, analyzing, and describing galaxies and star clusters with artificial intelligence., , and . Astron. Comput., (2019)Evolution of the high-mass end of the stellar initial mass functions in starburst galaxies, and . (2013)cite arxiv:1301.7128Comment: 14pages, 5figures, accepted for publication in ApJL.Estimating galaxy masses from kinematics of globular cluster systems: a new method based on deep learning., , , and . CoRR, (2021)Choirs, HI Galaxy Groups: Catalogue and Detection of Star-forming Dwarf Group Members, , , , , , , , , and 17 other author(s). (2013)cite arxiv:1304.7938Comment: To be published in MNRAS. 21 pages, 27 figures.