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Verena Obermüller

dblp:353/7631 · DBLP profile ↗
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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

TopicWeightPapersLastEvidence papers
Image and video processing › pattern detection
anomaly detection
0.712023
Uncover: Toward Interpretable Models for Detecting New Star Cluster Members · IEEE Trans. Vis. Comput. Graph. 2023
Visualization and visual analytics › scientific visualization
astronomical visualization
0.712023
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
0.712023
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
0.712023
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
YearPublicationVenuePosition
2023 Uncover: Toward Interpretable Models for Detecting New Star Cluster Members
abstract
In 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