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pro vyhledávání: '"Weber, Mark"'
Recent advancements in generative models have highlighted the crucial role of image tokenization in the efficient synthesis of high-resolution images. Tokenization, which transforms images into latent representations, reduces computational demands co
Externí odkaz:
http://arxiv.org/abs/2406.07550
Autor:
Bellei, Claudio, Xu, Muhua, Phillips, Ross, Robinson, Tom, Weber, Mark, Kaler, Tim, Leiserson, Charles E., Arvind, Chen, Jie
Subgraph representation learning is a technique for analyzing local structures (or shapes) within complex networks. Enabled by recent developments in scalable Graph Neural Networks (GNNs), this approach encodes relational information at a subgroup le
Externí odkaz:
http://arxiv.org/abs/2404.19109
Autor:
Weber, Mark1 (AUTHOR) weber@uni-bremen.de
Publikováno v:
Atmospheric Measurement Techniques. 2024, Vol. 17 Issue 11, p3597-3604. 8p.
Autor:
Toker, Aysim, Kondmann, Lukas, Weber, Mark, Eisenberger, Marvin, Camero, Andrés, Hu, Jingliang, Hoderlein, Ariadna Pregel, Şenaras, Çağlar, Davis, Timothy, Cremers, Daniel, Marchisio, Giovanni, Zhu, Xiao Xiang, Leal-Taixé, Laura
Earth observation is a fundamental tool for monitoring the evolution of land use in specific areas of interest. Observing and precisely defining change, in this context, requires both time-series data and pixel-wise segmentations. To that end, we pro
Externí odkaz:
http://arxiv.org/abs/2203.12560
Autor:
Weber, Mark1, Cunningham, Emily1, Beck, Diane M.1, Sadaghiani, Sepideh1, Wang, Ranxiao Frances1 wang18@illinois.edu
Publikováno v:
Memory & Cognition. May2024, Vol. 52 Issue 4, p984-997. 14p.
Autor:
Weber, Mark1,2 (AUTHOR) mark.edward.weber@gmail.com, Zrnic, Dusan2 (AUTHOR), Zhang, Pengfei2,3 (AUTHOR), Mansell, Edward2 (AUTHOR)
Publikováno v:
Journal of Applied Meteorology & Climatology. Mar2024, Vol. 63 Issue 3, p455-469. 15p.
Autor:
Li, Z. F., Cheng, X., Ding, M. D., Reeves, Katharine K., Kittrell, DeOndre, Weber, Mark, McKenzie, David E.
Solar flares are rapid energy release phenomena that appear as bright ribbons in the chromosphere and high-temperature loops in the corona, respectively. Supra-arcade Downflows (SADs) are plasma voids that first come out above the flare loops and the
Externí odkaz:
http://arxiv.org/abs/2107.09215