no code implementations • 8 Apr 2024 • Y. Wang, A. Gao, Y. Gong, Y. Zeng
In this paper, we consider the stylization of sparse-view scenes in terms of disentangling content semantics and style textures.
no code implementations • 30 Nov 2023 • Y. Wang, J. Xu, Y. Zeng, Y. Gong
In this paper, we propose an anisotropic neural representation learning method that utilizes learnable view-dependent features to improve scene representation and reconstruction.
no code implementations • 24 Sep 2023 • Y. Li, X. Qin, J. Geng, R. Chen, Y. Hou, Y. Gong, M. Pan, P. Zhang
REW AFL introduces a novel PS utility function that jointly considers global FL training utilities and local energy utility, which integrates energy consumption and residual battery energy of candidate mobile devices.
no code implementations • 30 Jul 2022 • Y. Gong, X. Ma
Smoke detection has become a significant task in associated industries due to the close relationship between the petrochemical industry's smoke emission and its safety production and environmental damage.
no code implementations • 10 Mar 2021 • Rohit Dokara, A. Brunthaler, K. M. Menten, S. A. Dzib, W. Reich, W. D. Cotton, L. D. Anderson, C. -H. R. Chen, Y. Gong, S. -N. X. Medina, G. N. Ortiz-León, M. Rugel, J. S. Urquhart, F. Wyrowski, A. Yang, H. Beuther, S. J. Billington, T. Csengeri, C. Carrasco-González, N. Roy
We aim to identify SNR candidates using continuum images from the Karl G. Jansky Very Large Array GLObal view of the STAR formation in the Milky Way (GLOSTAR) survey.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
no code implementations • 7 Jan 2021 • A. M. Jacob, K. M. Menten, Y. Gong, P. Bergman, M. Tiwari, S. Bruenken, A. O. H. Olofsson
This analysis confirms our hypothesis that CH2 originates in warm and dilute PDR layers.
Astrophysics of Galaxies
no code implementations • 22 Dec 2020 • Y. Gong, A. Belloche, F. J. Du, K. M. Menten, C. Henkel, G. X. Li, F. Wyrowski, R. Q. Mao
We performed $^{13}$CO (1--0), C$^{18}$O (1--0), C$^{17}$O (1--0), $^{13}$CO (2--1), C$^{18}$O (2--1), and C$^{17}$O (2--1) imaging observations toward the Serpens filament with the Institut de Radioastronomie Millim{\'e}trique 30-m (IRAM-30 m) and Atacama Pathfinder EXperiment (APEX) telescopes.
Astrophysics of Galaxies
no code implementations • 3 Aug 2020 • O. A. Ansari, S. M. Mazhari, Y. Gong, C. Y. Chung
Moreover, further simulation results indicate the impacts of uncertainties of wind generation and load demand on short-term reliability indices.