pyspac 0.1.0

A library for fitting and analyzing asteroid phase curves.

pySPAC: Solar Phase curve Analysis and Characterization

pySPAC (python Solar Phase curve Analysis and Characterization) is a library for analyzing and fitting astronomical phase curves of asteroids and other small solar system bodies. It provides an object-oriented interface to bridge observational photometric data with standard theoretical models.

The primary function of pySPAC is to determine the absolute magnitude (H) and other phase function parameters from a set of phase angle (α) and reduced magnitude observations.

Documentation

📖 Full documentation is available at: https://rcboufleur.github.io/pySPAC/

Features

• Object-oriented interface via the PhaseCurve class
• Standard IAU photometric models: (H, G), (H, G₁, G₂), (H, G₁₂), (H, G₁₂) Penttilä calibration, and linear fit
• Weighted least-squares fitting with observational uncertainties
• Monte Carlo uncertainty analysis
• Multiple optimization methods with automatic constraint validation
• Model generation from fitted parameters
• Data persistence - save and load object state to/from JSON
• Comprehensive error handling and validation

Installation

From PyPI

pip install pyspac

From GitHub

pip install git+https://github.com/rcboufleur/pySPAC.git

Quick Start

import numpy as np
from pyspac import PhaseCurve

# Observational data
angles = np.array([0.17, 0.63, 0.98, 1.62, 4.95, 9.78,
                  12.94, 13.27, 13.81, 17.16, 18.52, 19.4])
mags = np.array([6.911, 7.014, 7.052, 7.105, 7.235, 7.341,
                7.425, 7.427, 7.437, 7.511, 7.551, 7.599])
errors = np.array([0.02, 0.02, 0.03, 0.03, 0.04, 0.04,
                   0.02, 0.02, 0.03, 0.03, 0.04, 0.04])

# Create object and fit model
pc = PhaseCurve(angle=angles, magnitude=mags, magnitude_unc=errors)
pc.fitModel(model="HG", method="trust-constr")
pc.summary()

# Monte Carlo uncertainties
pc.monteCarloUncertainty(n_simulations=500, model="HG", method="trust-constr")
pc.summary()

For detailed examples and tutorials, see the full documentation.

Available Models

Model	Parameters	Description
LINEAR	H, β	Linear phase function
HG	H, G	IAU standard (H, G) system
HG12	H, G₁₂	Simplified (H, G₁₂) system
HG12PEN	H, G₁₂	Penttilä et al. (2016) calibration
HG1G2	H, G₁, G₂	Three-parameter (H, G₁, G₂) system

Model-Method Compatibility

• Constrained models (HG, HG12, HG12PEN, HG1G2): Must use trust-constr, SLSQP, or COBYLA
• Unconstrained models (LINEAR): Can use any optimization method

pySPAC automatically validates model-method compatibility and provides clear error messages.

Monte Carlo Uncertainty Analysis

Two Monte Carlo methods for different scientific cases:

• .monteCarloUncertainty(): Based on observational uncertainties
• .monteCarloUnknownRotation(): Includes rotational scatter modeling

Data Requirements

Model	Min Points	Recommended
All 2-parameter models	3	5+
HG1G2 (3-parameter)	3*	5+

*Due to mathematical constraint 1-G₁-G₂=0

Contributing

Contributions are welcome! Please:

1. Fork the repository on GitHub
2. Create a new branch for your feature or bug fix
3. Make your changes and commit them
4. Submit a pull request to the main branch

Feel free to open an issue to report bugs or suggest new features.

References

If you use pySPAC in your research, please cite this repository and the relevant papers for the models you employ:

• HG System: Bowell, E., et al. (1989). "Application of photometric models to asteroids." In Asteroids II (pp. 524-556).
• HG1G2 & HG12 Systems: Muinonen, K., et al. (2010). "A three-parameter magnitude phase function for asteroids." Icarus, 209(2), 542-555.
• HG12PEN System: Penttilä, A., et al. (2016). "Asteroid H, G1, G2 and H, G12 phase function performance with sparse data." Planetary and Space Science, 123, 117-122.

License

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