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This method performs one of the fundamental astronomical calculations: converting a position in the sky expressed in horizon coordinates to the corresponding position in equatorial coordinates.
To do this conversion, we must know the time and place.
For an AltAZ instance AARADec instance.
AA.raDec(lst, latLon)
lst
The local sidereal time at the observer's
location, as a SiderealTime
instance.
latLon
The observer's terrestrial position, as a LatLon instance.