Instruction

Analyze transit photometry data by processing light curves to identify periodic dips in stellar brightness.
Utilize transit fitting models (e.g., Batman, PyTransit) to estimate planetary parameters such as radius ratio and orbital period.
Conduct atmosphere characterization workflows by synthesizing transmission spectra to detect molecular markers like $H_2O$ or $CO_2$.
Implement data cleaning steps, such as detrending stellar variability and removing instrumental noise from space-based observations.
Follow best practices for radial velocity analysis to determine planetary mass and eccentricity.
Establish a cross-validation pipeline to confirm candidate planets and rule out false positives (e.g., eclipsing binaries).

When to Use

When performing light curve analysis for exoplanet discovery or characterization.
When modeling planetary atmospheres or determining physical parameters from astronomical data.
When planning scientific workflows for high-precision photometry or spectroscopy in exoplanetary science.

Support exoplanet workflows with clear steps and best practices.

Analyze transit photometry data by processing light curves to identify periodic dips in stellar brightness.
Utilize transit fitting models (e.g., Batman, PyTransit) to estimate planetary parameters such as radius ratio and orbital period.
Conduct atmosphere characterization workflows by synthesizing transmission spectra to detect molecular markers like $H_2O$ or $CO_2$.
Implement data cleaning steps, such as detrending stellar variability and removing instrumental noise from space-based observations.
Follow best practices for radial velocity analysis to determine planetary mass and eccentricity.
Establish a cross-validation pipeline to confirm candidate planets and rule out false positives (e.g., eclipsing binaries).

When performing light curve analysis for exoplanet discovery or characterization.
When modeling planetary atmospheres or determining physical parameters from astronomical data.
When planning scientific workflows for high-precision photometry or spectroscopy in exoplanetary science.