Common-Envelope Light-Curve Fitting
Develop common-envelope model light curves and fitting workflows for Rubin transient candidates.
The common-envelope tooling models stellar inspirals using a primary-star profile and companion mass, producing predicted light curves in Rubin filters. Model grids, candidate filtering and parameter inference are being developed to connect these predictions with transient-broker workflows.
Maturity
Not specified
Access
Public
No portal sign-in is required.
Maintainers
Nikki Noughani
What it supports
Use cases
- Stellar inspiral light curves
- Rubin-band model grids
- Candidate identification
- Parameter inference
Where it runs
Runtime homes
Runtime, inputs & outputs
- Distributions
- Runtime
- not-applicable
- Access
- public
- Inputs
- Not specified
- Outputs
- Not specified
Names & abbreviations
- CADC
- Canadian Astronomy Data Centre
- CanDIAPL
- Canadian Data Intensive Astrophysics Platform
- CE
- Common Envelope
Connected work
Related science context
Common-envelope transient modelsPredicted light curves and model grids support development of common-envelope candidate identification and parameter inference.