Right now, if I want to get model magnification at a specific time stamp, I have to add a time array to a telescope, add it to a pyLIMA event, add model parameters, and assign them to a pyLIMA model, and then finally, I can call the mag = model.magnification(pyLIMA_paramaters, telescope). While it makes sense to go through a telescope, it may be cumbersome at times, especially if the initial telescope already exists, but for whatever reason, I want to find what is the model magnification at a time for which the telescope doesn't have observations.
It would be nice if there were an easier way to get model magnification.
Right now, if I want to get model magnification at a specific time stamp, I have to add a time array to a telescope, add it to a pyLIMA event, add model parameters, and assign them to a pyLIMA model, and then finally, I can call the
mag = model.magnification(pyLIMA_paramaters, telescope). While it makes sense to go through a telescope, it may be cumbersome at times, especially if the initial telescope already exists, but for whatever reason, I want to find what is the model magnification at a time for which the telescope doesn't have observations.It would be nice if there were an easier way to get model magnification.