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June 16, 20260 citationsOpen Access

Mass Dependence of the RECT Parameter C: Results from SPARC and NSA Galaxy Samples

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DFDaniel Fang

Key Result

This is an astrophysics paper analyzing the mass-dependent response of the RECT parameter C in galaxy populations, containing no clinical data.

Key Points

  • To investigate how the RECT parameter C varies with mass in spiral and mixed galaxy populations.
  • Utilized random samples from SPACE and NSA galaxies for analysis.
  • Included core Python scripts to reproduce key tables and figures from the study.
  • Implemented the empirical relation C_eff = Σ_star^(-0.6) for NSA-related codes.
  • Presented evidence of mass-dependent variation in RECT parameter C among galaxy types.
  • Provided reproducible findings through shared analysis scripts, enhancing transparency in results.

Structured PICO

P
Population
Spiral and mixed galaxy populations from SPACE and NSA random samples

The paper provides analysis code and a preprint investigating the mass-dependent response of RECT parameter C in galaxy populations.

Abstract

This upload contains the preprint and supporting analysis code for the paper: "Mass-Dependent Response of RECT Parameter C in Spiral and Mixed Galaxy Populations: Evidence from SPACE and NSA Random Samples" The repository includes: - The full preprint PDF - Core Python scripts to reproduce Table 1 and the main figures - Additional analysis scripts for the SPACE and NSA samples All NSA-related codes use Cₑff = Σₛtar^ (-0. 6), following the empirical relation observed in the SPACE sample.

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Daniel Fang (2026) studied this question. This is an astrophysics paper analyzing the mass-dependent response of the RECT parameter C in galaxy populations, containing no clinical data.

synapsesocial.com/papers/6a31572eaf7cf7f8256b3dadhttps://doi.org/10.5281/zenodo.20701202
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