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The current model for the slew timing just uses the angular separation between two fields. In reality, the Blanco is an Alt/Az telescope, which means that slews in RA will should take a long time near the poll. Also we should be aware of the RA = 360 discontinuity.
The text was updated successfully, but these errors were encountered:
The current model for the slew timing just uses the angular separation between two fields. In reality, the Blanco is an Alt/Az telescope, which means that slews in RA will should take a long time near the poll. Also we should be aware of the RA = 360 discontinuity.
The text was updated successfully, but these errors were encountered: