eclipsebin 0.1.3

A specialized binning scheme for eclipsing binary star light curves

Binning Eclipsing Binary Star Light Curves

Overview

This Python package provides a specialized binning scheme designed to more effectively capture the features of eclipsing binary star light curves. Unlike traditional uniform binning (middle panel), which can dilute the crucial details of eclipses, this non-uniform binning method (right panel) prioritizes the accurate representation of eclipse events.

Key Features

• Eclipse-Focused Binning: The binning algorithm identifies the eclipse phases and allocates up to half of the total bins to these critical periods. The remaining bins are distributed across the out-of-eclipse regions.

• Optimized Data Distribution: Using the pandas qcut function, the package ensures that each bin within the eclipse and out-of-eclipse segments contains approximately the same number of data points, maintaining the integrity of the light curve's structure.

• Enhanced Accuracy: By concentrating bins around the brief, narrow eclipse phases, the method improves the resolution of these events, which are essential for deriving accurate parameters of the binary system.

Why Use This Binning Scheme?

Eclipses in binary star systems contain vital information about the system's properties, such as the relative sizes, masses, and orbital parameters of the stars. Standard uniform binning can obscure these details, especially when the eclipse duration is short relative to the orbital period. This package mitigates that issue by adaptively placing more bins where they matter most—during the eclipses—thereby preserving the fidelity of the light curve and improving the subsequent analysis.

How it Works

Getting Started

To start using the package, install it via pip:

pip install eclipsebin

Usage

import eclipsebin as ebin

# Example usage
binner = EclipsingBinaryBinner(phases, fluxes, fluxerrs, nbins=200, fraction_in_eclipse=0.2)
bin_centers, bin_means, bin_stds = binner.bin_light_curve(plot=True)

Refer to the documentation for more detailed usage instructions and examples.

Contributing

Contributions are welcome! Please refer to the Contributing Guide for guidelines on how to help improve this project.

License

This project is licensed under the MIT License - see the LICENSE file for details.