Exoplanetary Disk Vertical Structure Model Parameters from ARKS III

Machine-readable tables contain fiducial parametric model values for astronomical sources and scale height aspect ratios derived from parametric modeling, frank, and rave. The data was produced by Brianna Zawadzki as part of the ALMA survey to Resolve exoKuiper belt Substructures (ARKS). It was last updated in January 2026.

Use Cases

• Analyze the distribution of scale height aspect ratios across different sources to study disk vertical structure.
• Compare fiducial parametric model values with outputs from the frank and rave modeling methods.
• Use the fiducial model parameters as inputs for simulations of exoplanetary disk dynamics.

Strengths

• Data is directly associated with the published ARKS III survey results, providing model values referenced in its tables.
• The dataset was updated in January 2026, indicating recent maintenance.

Limitations

• The number of rows, columns, and file size are unknown, preventing assessment of dataset scale.
• The specific column names and data formats are not provided, complicating initial analysis.

Provenance

Source

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

Collection Method

Parametric modeling of astronomical sources, including methods named frank and rave.

Freshness

Last updated on 2026-01-19.