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lomb-scargle-periodogram

Lomb-Scargle periodogram for finding periodic signals in unevenly sampled time series data. Use when analyzing light curves, radial velocity data, or any astronomical time series to detect periodic variations. Works for stellar rotation, pulsation, eclipsing binaries, and general periodic phenomena. Based on lightkurve library.

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Installation

Follow the repository instructions for this skill and your agent. Review the files and dependencies before adding it to your workflow.

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Skill instructions

Lomb-Scargle Periodogram

The Lomb-Scargle periodogram is the standard tool for finding periods in unevenly sampled astronomical time series data. It's particularly useful for detecting periodic signals in light curves from space missions like Kepler, K2, and TESS.

Overview

The Lomb-Scargle periodogram extends the classical periodogram to handle unevenly sampled data, which is common in astronomy due to observing constraints, data gaps, and variable cadences.

Basic Usage with Lightkurve

import lightkurve as lk
import numpy as np

# Create a light curve object
lc = lk.LightCurve(time=time, flux=flux, flux_err=error)

# Create periodogram (specify maximum period to search)
pg = lc.to_periodogram(maximum_period=15)  # Search up to 15 days

# Find strongest period
strongest_period = pg.period_at_max_power
max_power = pg.max_power

print(f"Strongest period: {strongest_period:.5f} days")
print(f"Power: {max_power:.5f}")

Plotting Periodograms

import matplotlib.pyplot as plt

pg.plot(view='period')  # View vs period (not frequency)
plt.xlabel('Period [days]')
plt.ylabel('Power')
plt.show()

Important: Use view='period' to see periods directly, not frequencies. The default view='frequency' shows frequency (1/period).

Period Range Selection

Choose appropriate period ranges based on your science case:

  • Stellar rotation: 0.1 - 100 days
  • Exoplanet transits: 0.5 - 50 days (most common)
  • Eclipsing binaries: 0.1 - 100 days
  • Stellar pulsations: 0.001 - 1 day
# Search specific period range
pg = lc.to_periodogram(minimum_period=2.0, maximum_period=7.0)

Interpreting Results

Power Significance

Higher power indicates stronger periodic signal, but be cautious:

  • High power: Likely real periodic signal
  • Multiple peaks: Could indicate harmonics (period/2, period*2)
  • Aliasing: Very short periods may be aliases of longer periods
Common Patterns
  1. Single strong peak: Likely the true period
  2. Harmonics: Peaks at period/2, period*2 suggest the fundamental period
  3. Aliases: Check if period*2 or period/2 also show signals

Model Fitting

Once you find a period, you can fit a model:

# Get the frequency at maximum power
frequency = pg.frequency_at_max_power

# Create a model light curve
model = pg.model(time=lc.time, frequency=frequency)

# Plot data and model
import matplotlib.pyplot as plt
lc.plot(label='Data')
model.plot(label='Model')
plt.legend()
plt.show()

Dependencies

pip install lightkurve numpy matplotlib

References

When to Use This vs. Other Methods

  • Lomb-Scargle: General periodic signals (rotation, pulsation, eclipsing binaries)
  • Transit Least Squares (TLS): Specifically for exoplanet transits (more sensitive)
  • Box Least Squares (BLS): Alternative transit detection method

For exoplanet detection, consider using TLS after Lomb-Scargle for initial period search.

Examples

Read the usage examples in the source repository.

View source ↗

Source history

Indexed on
2026-01-20
Index updated
2026-02-02
Branch
main

Index and sync dates describe this directory. View the source repository for code history.

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