Transit analysis¶
Single transit¶
The template notebook begins with a cell initialising the main TransitAnalysis class
ta = TransitAnalysis(target, night, tid=TID, cids=CIDS)
where target is the target name, night is the observing night, tid is the target ID, and cids is a list of IDs of reference stars to be included into the reference star optimisation (marked in the photometry reference frames). The TransitAnalysis class has options to tailor the analysis, but this information should be enough for the basic use cases.
Multiple epochs¶
from muscat2ta..m2mnlpf import M2MultiNightLPF
lpf = M2MultiNightLPF(name, use_opencl=USE_OPENCL)
Secondary eclipse modelling¶
TBD