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Ryan Maas
Ryan Maas
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Geverifieerd e-mailadres voor cs.washington.edu
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The causes of halo shape changes induced by cooling baryons: disks versus substructures
VP Debattista, B Moore, T Quinn, S Kazantzidis, R Maas, L Mayer, J Read, ...
The Astrophysical Journal 681 (2), 1076, 2008
2142008
The Myria Big Data Management and Analytics System and Cloud Services.
J Wang, T Baker, M Balazinska, D Halperin, B Haynes, B Howe, ...
CIDR, 2017
972017
The role of the radial orbit instability in dark matter halo formation and structure
JM Bellovary, JJ Dalcanton, A Babul, TR Quinn, RW Maas, CG Austin, ...
The Astrophysical Journal 685 (2), 739, 2008
552008
Gaussian mixture models use-case: in-memory analysis with myria
R Maas, J Hyrkas, OG Telford, M Balazinska, A Connolly, B Howe
Proceedings of the 3rd VLDB Workshop on In-Memory Data Mangement and …, 2015
122015
Probing Halo Substructure With Rr Lryae From Multi-epoch Sdss Data.
OJ Fraser, SH Grammer, DP Morgan, AZ Welch, EW Bullock, ...
American Astronomical Society Meeting Abstracts 211, 60.09, 2007
2007
The Role of the Radial Orbit Instability in Dark Matter Halo Formation and Structure
JM Meyer, JJ Dalcanton, TR Quinn, LLR Williams, EI Barnes, A Babul, ...
Proceedings of the International Astronomical Union 2 (S235), 124-124, 2006
2006
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Artikelen 1–6