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Disambiguation of "Tanaka, Masayuki"

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3D visualization of aurora considering the physical characteristics.

, , , , , , , and . SIGGRAPH Asia Posters, page 52. ACM, (2016)

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Masayuki Hirosue

Masao Tanaka

Masafumi Tanaka

Masayuki Maenishi

Masayuki Yamamoto

 

Other publications of authors with the same name

Direct spatio-spectral datacube reconstruction from raw data using a spatially adaptive spatio-spectral basis., , and . Digital Photography, volume 8660 of SPIE Proceedings, page 866003. SPIE/IS&T, (2013)A Practical One-Shot Multispectral Imaging System Using a Single Image Sensor., , , and . IEEE Trans. Image Processing, 24 (10): 3048-3059 (2015)Adaptive Residual Interpolation for Color and Multispectral Image Demosaicking., , , and . Sensors, 17 (12): 2787 (2017)Centered Subset Kernel PCA for Denoising., and . ACCV Workshops (2), volume 6469 of Lecture Notes in Computer Science, page 354-363. Springer, (2010)Liquid Diffusion Model that Accounts for a Variety of Dyeing Parameters., , , and . Eurographics (Short Papers), page 85-88. Eurographics Association, (2007)Monochrome And Color Polarization Demosaicking Using Edge-Aware Residual Interpolation., , , and . ICIP, page 2571-2575. IEEE, (2020)Minimized-Laplacian residual interpolation for color image demosaicking., , , and . Digital Photography, volume 9023 of SPIE Proceedings, page 90230L. SPIE/IS&T, (2014)An optically-selected cluster catalog at redshift 0.1<z<1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1701.00818Comment: 16 pages, 15 figures, cluster catalogs will be made available after the paper is accepted.Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1704.06004Comment: 28 pages, 11 figures, submitted to a special issue of PASJ.First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. I. The role of group or cluster environment in star formation quenching from z = 0.2 to 1.1, , , , , , , , and . (2017)cite arxiv:1704.06219Comment: 14 pages, 9 figures.