EDBT 2026 Demo / reviewers in the wild / expert
Verena Obermüller
dblp:353/7631
· DBLP profile ↗
1ranked-venue papers
0as first author
1since 2021 · last 2023
0000-0001-5417-1364ORCID · reported
Domains — the database's venue-derived domains; a paper can count in several
Graphics, computer vision, multimedia, augmented reality and games · 1 · 1 since 2021
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 |
Visualization and visual analytics · 75% Image and video processing · 25% |
Topics — the 4 heaviest of 4, each with the papers that count most for it
| Topic | Weight | Papers | Last | Evidence papers |
|---|---|---|---|---|
Image and video processing › pattern detection
anomaly detection |
0.7 | 1 | 2023 | Uncover: Toward Interpretable Models for Detecting New Star Cluster Members · IEEE Trans. Vis. Comput. Graph. 2023 |
Visualization and visual analytics › scientific visualization
astronomical visualization |
0.7 | 1 | 2023 | Uncover: Toward Interpretable Models for Detecting New Star Cluster Members · IEEE Trans. Vis. Comput. Graph. 2023 |
Visualization and visual analytics › human-in-the-loop
interactive machine learning |
0.7 | 1 | 2023 | Uncover: Toward Interpretable Models for Detecting New Star Cluster Members · IEEE Trans. Vis. Comput. Graph. 2023 |
Visualization and visual analytics › visual analytics
visual analytics system |
0.7 | 1 | 2023 | Uncover: Toward Interpretable Models for Detecting New Star Cluster Members · IEEE Trans. Vis. Comput. Graph. 2023 |
Methods — techniques the papers use, named apart from their topics
hyperparameter tuning · 0.7dimensionality reduction · 0.7
| Year | Publication | Venue | Position |
|---|---|---|---|
| 2023 | Uncover: Toward Interpretable Models for Detecting New Star Cluster MembersabstractIn this design study, we present Uncover, an interactive tool aimed at astronomers to find previously unidentified member stars in stellar clusters. We contribute data and task abstraction in the domain of astronomy and provide an approach for the non-trivial challenge of finding a suitable hyper-parameter set for highly flexible novelty detection models. We achieve this by substituting the tedious manual trial and error process, which usually results in finding a small subset of passable models with a five-step workflow approach. We utilize ranges of a priori defined, interpretable summary statistics models have to adhere to. Our goal is to enable astronomers to use their domain expertise to quantify model goodness effectively. We attempt to change the current culture of blindly accepting a machine learning model to one where astronomers build and modify a model based on their expertise. We evaluate the tools' usability and usefulness in a series of interviews with domain experts. Sebastian Ratzenböck, Verena Obermüller, Torsten Möller, João Alves 0004, Immanuel M. Bomze |
IEEE Trans. Vis. Comput. Graph. | 2 |