A catalog and research note by John Timlin of Pennsylvania State University presents the X-ray and HeII equivalent width properties of Radio-loud quasars. The research indicates that X-ray emission from typical RLQs likely originates in the corona rather than from a jet-linked component. The dataset is available under an Open Access (green) license.
Use Cases
- Analyzing the relationship between X-ray emission and HeII equivalent width in radio-loud quasars based on the catalog properties.
- Investigating the origin of X-ray emission in quasars based on the described corona vs. jet-linked component distinction.
- Training models to classify quasar emission mechanisms based on X-ray and HeII EW properties mentioned in the description.
- Conducting comparative studies of radio-loud quasar populations using the presented catalog data.
Strengths
- Dataset is associated with a specific research finding on the origin of X-ray emission in radio-loud quasars.
- Provenance is clear, authored by a researcher at Pennsylvania State University.
- Available under an Open Access (green) license, facilitating reuse.
Limitations
- Column-level documentation is absent; field semantics must be inferred after download.
- Row count is unknown, which may limit suitability assessment.
- Last update date is unknown; freshness unverified.
Provenance
- Source
- John Timlin, Pennsylvania State University
- Collection Method
- Likely compiled from astronomical observations and research analysis, as indicated by the description of a catalog and research note.