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This repository has been archived by the owner on Oct 26, 2022. It is now read-only.
We'll need the function bjd2utc(), as the input FITS images will use Barycentric Julian Date while LEMON works internally with seconds after the Unix epoch.
The biggest source of confusion comes from the fact that time standards and reference frames are independent from one another, even though there are many overlapping concepts between the two. We will use the following terminology: “reference frame” will refer to the geometric location from which one could measure time – different reference frames differ by the light-travel time between them; “time standard” will refer to the way a particular clock ticks and its arbitrary zero point, as defined by international standards; and “time stamp” is the combination of the two, and determines the timing accuracy of the event.
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This is the
BJD_TDB
FITS keyword. It's a non-standard keyword but commonly used for exoplanets.More information on:
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