What question did this study set out to answer?

To investigate how the RECT parameter C varies with mass in spiral and mixed galaxy populations.

June 16, 20260 citationsOpen Access

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

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

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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