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Where are the low mass Pop III stars ?

, , , , , and . (2016)cite arxiv:1602.00465Comment: submitted to ApJ, 11 pages, 8 figures.

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24.77 Pflops on a Gravitational Tree-Code to Simulate the Milky Way Galaxy with 18600 GPUs., , , , , and . SC, page 54-65. IEEE Computer Society, (2014)High Performance Gravitational N-body Simulations on Supercomputer Fugaku., , and . HPC Asia, page 10-17. ACM, (2022)Supercomputer simulations of structure formation in the Universe.. Astroinformatics, volume 12 of Proceedings of the International Astronomical Union, page 10-16. Cambridge University Press, (2016)Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium, , , , and . (2019)cite arxiv:1909.07034Comment: 9 pages, 8 figures, submitted to MNRAS.SILVERRUSH. VI. A simulation of Ly$\alpha$ emitters in the reionization epoch and a comparison with Subaru Hyper Suprime-Cam survey early data, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1801.00067Comment: Submitted to PASJ, 29 pages, 20 figures.Quasar clustering in a galaxy and quasar formation model based on ultra high-resolution N-body simulations, , , , , and . (2015)cite arxiv:1512.00458Comment: 6 pages, 3 figures, to appear in MNRAS Letters.Simulating the Universe on an Intercontinental Grid., , , , , , , , , and . Computer, 43 (8): 63-70 (2010)Where are the low mass Pop III stars ?, , , , , and . (2016)cite arxiv:1602.00465Comment: submitted to ApJ, 11 pages, 8 figures.4.45 Pflops astrophysical N-body simulation on K computer: the gravitational trillion-body problem., , and . SC, page 5. IEEE/ACM, (2012)