Knowing the Luminosity and Temperature of am observed star or cluster we can place them on the HRD and find which BPASS HRD bin they fall into. From this we can plot the probabilities of that particular bin being filled at each time step and normalise, giving us an age probability distribution.
Feature Requirements
Given an observed luminosity and temperature, the age pdf should be returned.
Given a table of observed luminosities and temperature the age pdfS should be returned
=> This will probably be best done in a pandas data frame where the ages bins are columns and the rows are a set of L and T, i.e. individual objects.
Context
Knowing the Luminosity and Temperature of am observed star or cluster we can place them on the HRD and find which BPASS HRD bin they fall into. From this we can plot the probabilities of that particular bin being filled at each time step and normalise, giving us an age probability distribution.
Feature Requirements
Given an observed luminosity and temperature, the age pdf should be returned. Given a table of observed luminosities and temperature the age pdfS should be returned
=> This will probably be best done in a pandas data frame where the ages bins are columns and the rows are a set of L and T, i.e. individual objects.