Demo Data from VLDB 2026 / reviewers in the wild / expert
Hilda Faraji
dblp:40/3530
· DBLP profile ↗
2ranked-venue papers
2as first author
0since 2021 · last 2006
—ORCID · none
Domains — the database's venue-derived domains; a paper can count in several
Graphics, computer vision, multimedia, augmented reality and games · 2 · 2 first-author
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.
| Computer graphics and multimedia
1 paper |
Image and video processing · 67% Computational photography and imaging · 33% |
Topics — the 3 heaviest of 3, each with the papers that count most for it
| Topic | Weight | Papers | Last | Evidence papers |
|---|---|---|---|---|
Computational photography and imaging › camera characterization
camera noise modeling |
0.1 | 1 | 2006 | CCD noise removal in digital images · IEEE Trans. Image Process. 2006 |
Image and video processing › image restoration
image denoising |
0.1 | 1 | 2006 | CCD noise removal in digital images · IEEE Trans. Image Process. 2006 |
Image and video processing
image restoration |
0.1 | 1 | 2006 | CCD noise removal in digital images · IEEE Trans. Image Process. 2006 |
Methods — techniques the papers use, named apart from their topics
light space denoising · 0.1camera response function · 0.1adaptive filtering · 0.1
| Year | Publication | Venue | Position |
|---|---|---|---|
| 2006 | CCD noise removal in digital imagesabstractIn this work, we propose a denoising scheme to restore images degraded by CCD noise. The CCD noise model, measured in the space of incident light values (light space), is a combination of signal-independent and signal-dependent noise terms. This model becomes more complex in image brightness space (normal camera output) due to the nonlinearity of the camera response function that transforms incoming data from light space to image space. We develop two adaptive restoration techniques, both accounting for this nonlinearity. One operates in light space, where the relationship between the incident light and light space values is linear, while the second method uses the transformed noise model to operate in image space. Both techniques apply multiple adaptive filters and merge their outputs to give the final restored image. Experimental results suggest that light space denoising is more efficient, since it enables the design of a simpler filter implementation. Results are given for real images with synthetic noise added, and for images with real noise. Hilda Faraji, W. James MacLean |
IEEE Trans. Image Process. | 1 |
| 2004 | Adaptive suppression of CCD signal-dependent noise in light spaceabstractWe propose a denoising scheme to restore images degraded by CCD noise. Typically, restoration algorithms assume a linear mapping between the incident light space and image space. However, in practice, a camera response function performs a non-linear mapping on the sensor output and, as a result, the sensor noise model becomes more complex in the image space. We correct for non-linearity by mapping the corrupted image into "light space", where the relationship between the incident light and light space values is linear. To reduce the sensor noise we accurately model the CCD sensor noise by using the photon transfer curve. We then develop a combination of adaptive filters based on the estimated noise model in light space. Our adaptive system demonstrates efficient noise removal performance in uniform regions, while preserving edges and fine details. Hilda Faraji, W. James MacLean |
ICASSP (3) | 1 |