opticam.fitting.routines
Functions
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Iteratively fit a straight line (in log space) to the RMS vs flux plots for each catalog. This can be used to |
Module Contents
- opticam.fitting.routines.fit_rms_vs_flux(data)
Iteratively fit a straight line (in log space) to the RMS vs flux plots for each catalog. This can be used to identify variable sources and good comparison sources.
Parameters
- dataDict
The RMS vs flux data.
Returns
- Dict[str, Dict[str, NDArray]]
The power law fits for each filter {filter: {‘flux’: NDArray, ‘rms’: NDArray}}.
- Parameters:
data (Dict)
- Return type:
Dict[str, Dict[str, numpy.typing.NDArray]]