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The coordinates are fixed.
The coordinates are recorded.
The coordinates are in Talairach space.
Basically, the coordinates are given in inches.
The coordinates are then derived by numerical integration.
For algebraic simplicity, the coordinates are transformed for individual layers.
As viewers swivel the telescope to survey the scenery, the coordinates are sent to a computer embedded in the base.
When an event is registered, the coordinates are stored internally as a (x,y) coordinate pair.
The coordinates are in the reciprocal lattice basis, and so they are integers.
The celfmt=hms is used to indicate that the coordinates are provided in sexagesimal format.
If not specified, the coordinates are returned in the current coordinate system for the window.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com