Demo Data from VLDB 2026 / reviewers in the wild / expert
Akshaya Athawale
dblp:241/5319
· DBLP profile ↗
1ranked-venue papers
0as first author
0since 2021 · last 2019
—ORCID · none
Domains — the database's venue-derived domains; a paper can count in several
Artificial intelligence and machine learning · 1Graphics, computer vision, multimedia, augmented reality and games · 1
Expertise — from the expertise taxonomy: the topics of the expert's papers under the CCF categories. A weight counts papers with recency: 1 for a paper about the topic, 0.3 when the topic is its context, halved every five years.
| Artificial intelligence
1 paper |
3D vision · 100% | |
| Computer graphics and multimedia
1 paper |
Rendering · 50% Visual content generation and editing · 50% |
Topics — the 4 heaviest of 4, each with the papers that count most for it
| Topic | Weight | Papers | Last | Evidence papers |
|---|---|---|---|---|
Computer vision › 3D vision › inverse rendering
illumination estimation |
0.4 | 1 | 2019 | Deep Sky Modeling for Single Image Outdoor Lighting Estimation · CVPR 2019 |
Computer vision › 3D vision › inverse rendering
outdoor lighting estimation |
0.4 | 1 | 2019 | Deep Sky Modeling for Single Image Outdoor Lighting Estimation · CVPR 2019 |
Rendering
image-based rendering |
0.1 | 1 | 2019 | Deep Sky Modeling for Single Image Outdoor Lighting Estimation · CVPR 2019 |
Visual content generation and editing › image editing › image compositing
object insertion |
0.1 | 1 | 2019 | Deep Sky Modeling for Single Image Outdoor Lighting Estimation · CVPR 2019 |
Methods — techniques the papers use, named apart from their topics
deep learning · 0.8convolutional neural network · 0.8
| Year | Publication | Venue | Position |
|---|---|---|---|
| 2019 | Deep Sky Modeling for Single Image Outdoor Lighting EstimationabstractWe propose a data-driven learned sky model, which we use for outdoor lighting estimation from a single image. As no large-scale dataset of images and their corresponding ground truth illumination is readily available, we use complementary datasets to train our approach, combining the vast diversity of illumination conditions of SUN360 with the radiometrically calibrated and physically accurate Laval HDR sky database. Our key contribution is to provide a holistic view of both lighting modeling and estimation, solving both problems end-to-end. From a test image, our method can directly estimate an HDR environment map of the lighting without relying on analytical lighting models. We demonstrate the versatility and expressivity of our learned sky model and show that it can be used to recover plausible illumination, leading to visually pleasant virtual object insertions. To further evaluate our method, we capture a dataset of HDR 360° panoramas and show through extensive validation that we significantly outperform previous state-of-the-art. Yannick Hold-Geoffroy, Akshaya Athawale, Jean-François Lalonde |
CVPR | 2 |