Michael J.I. Brown and R. L. Webster, PASA, 15 (2), 176
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Conclusions
A search of 
near the ecliptic to a limiting magnitude of 
has been conducted for bright Kuiper belt objects. This search and other surveys constrain the number of Kuiper belt objects brighter than our limiting magnitude to 
. Surveys with the planned 
CCD on the Siding Spring 40-inch telescope should provide an improved estimate of the population of bright Kuiper Belt Objects and further constrain the bright end of the luminosity function.
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