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Elemental abundances of nearby M dwarfs based on high-resolution near-infrared spectra obtained by the Subaru/IRD survey: Proof of concept

, , , , , , , , , , , , , , , , , , , , , , , , , , and . (2021)cite arxiv:2112.00173Comment: 31 pages, 16 figures, accepted for publication in AJ.

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Performance evaluation and tuning of GRAPE-6 - towards 40 "real" Tflops., , and . SC, page 2. ACM, (2003)A 29.5 Tflops simulation of planetesimals in Uranus-Neptune region on GRAPE-6., , , and . SC, page 20:1-20:14. IEEE Computer Society, (2002)Elemental abundances of nearby M dwarfs based on high-resolution near-infrared spectra obtained by the Subaru/IRD survey: Proof of concept, , , , , , , , , and 17 other author(s). (2021)cite arxiv:2112.00173Comment: 31 pages, 16 figures, accepted for publication in AJ.HARP Chip: A.600 Mflops Application-Specific LSI for Astrophysical itN-body Simulations., , , , and . HICSS (1), page 302-311. IEEE Computer Society, (1994)Terrestrial Planet Formation at Home and Abroad, , , , and . (2013)cite arxiv:1312.1689Comment: 27 pages, 9 figures, 2 tables. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C. Dullemond, Th. Henning.HARP-1: A Special-Purpose Computer for itN-body Simulation with the Hermite Integrator., , and . HICSS (1), page 292-301. IEEE Computer Society, (1994)