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OPAL
OPAL (Observatoire Pluridisciplinaire des ALpes-maritimes) is a research facility providing High-Performance Computing (HPC), artificial intelligence (AI) computing facilities, data storage and computing, as well as visualization resources and testbeds. OPAL is a joint effort of Université Côte d'Azur, Observatoire de la Côte d'Azur, Inria Sophia Antipolis and Mines ParisTech à Sophia Antipolis. It is built on the sharing of the computational resources of these four institutions through an unified access. OPAL provides computing services to the members of Université Côte d'Azur and their industry and society partners for research, education and development.
Last Deposits
Documents in Full Text
254
Notices
20
Statistics by Discipline
Keywords
Méthodes directes
Astrophysics - Solar and Stellar Astrophysics
$p$-robustness
Planets and satellites dynamical evolution and stability
Turbulence
Event camera
Computer Graphics
Planet-disk interactions
Controlled source seismology
Appearance capture
Reconstruction
Methods observational
GANs
Federated Learning
Atherosclerosis
Sketching
Image processing
EEG
Stars abundances
Multiple Sclerosis
Protoplanetary disks
Gaunt Coefficients
Marked point process
Gravitation
Relighting
Point process
Action Detection
Inverse theory
Alps
Inversion de formes d'ondes
Galaxy evolution
Non-photorealistic rendering
Multi-View
Domain adaptation
Image-Based Rendering
Remote Sensing
MEG
Stars activity
CNN
Convolutional neural network
Lithosphérique
Plasmas
A posteriori estimate
Line drawing
Full-waveform inversion
Saliency
GM-PHD
Densité
Generative adversarial networks
Hydrodynamics
Catastrophic forgetting
Planets and satellites detection
Deep learning
Dense labeling
Machine learning
Stars atmospheres
Deep Learning
Alzheimer's disease
Astrophysics - Earth and Planetary Astrophysics
Finite element method
Methods numerical
Multigrid method
Attention
Semantic segmentation
Small object detection
Spherical Harmonics
Material capture
3D reconstruction
Object detection
Neural Rendering
SVBRDF
Convolutional neural networks
Density
Minor planets
Segmentation
OPAL-Meso
Mean-field limit
Radiative transfer
Seismic imaging
Stable decomposition
3D Gaussian Splatting
Schwarz method
Galaxy disk
Diffusion MRI
Planets and satellites formation
Methods statistical
Tomographie
Neural networks
Lithospheric
Compound regularization
Remote sensing
Imagerie sismique
Alpes
Tractography
Neuromorphic
Gaussian Process
PET Imaging
Sketch-based modeling
Instabilities
Galaxy abundances