  Various observational properties of Ap/Bp stars have been well-established
such as the often-cited 10% incidence rate of strong, organized magnetic fields
amongst all A- and B-type stars. However, these inferences have generally been
drawn fromsurveys biased towards the strongest most easily detectable fields. A
volume-limited spectropolarimetric survey of all intermediate-mass stars within
100 pc was initiated in 2007 in order to avoid the biases inherent in previous
studies. This workyielded the magnetic properties of a large number of Ap/Bp
stars in the sample; however, nearly half of the sample remained either
unobserved or had relatively poor constraints on their field strengths and
geometries. We have recently completed thissurvey using measurements obtained
by ESPaDOnS and NARVAL. We discuss here some of the recent findings of this
survey.
