Returns an array of 3 fractions of a day, representing respectively the local times of rising, transit and
setting for the given latitude and refraction offset (h0 = -0.5667 for stars and planets, -0.8333 for the
Sun, +0.125 for the Moon).
This class is concerned with distance calibration which should be done before measuring an image, in order to
measure in real physical units rather than in pixels.
This class is concerned with distance calibration which should be done before measuring an image, in order to
measure in real physical units rather than in pixels.
This adjusts the fields of the current object to the given new equinox (eg, J2000) and epoch (eg, JD now)
by first applying proper motion for the new epoch
and then calling SkyPoint.changeEpoch (equinox) on the resulting position.
This class is for adjusting a pair of corresponding points on two images interactively by showing a portion of
each image at full scale around the points and dragging each image with a mouse.