  The AO327 drift survey for radio pulsars and transients used the Arecibo
telescope from 2010 until its collapse in 2020. AO327 collected ~3100 hours of
data at 327 MHz with a time resolution of 82 us and frequency resolution of 24
kHz. While the main motivation for such surveys is the discovery of new pulsars
and new, even unforeseen, types of radio transients, they also serendipitously
collect a wealth of data on known pulsars. We present an electronic catalog of
data and data products on 206 pulsars whose periodic emission was detected by
AO327 and are listed in the ATNF catalog of all published pulsars. The AO327
data products include dedispersed time series at full time resolution, average
("folded") pulse profiles, Gaussian pulse profile templates, and an absolute
phase reference that allows phase-aligning the AO327 pulse profiles in a
physically meaningful manner with profiles from data taken with other
instruments. We also provide machine-readable tables with uncalibrated flux
measurements at 327 MHz and pulse widths at 50% and 10% of the pulse peak
determined from the fitted Gaussian profile templates. The AO327 catalog data
set can be used in applications like population analysis of radio pulsars,
pulse profile evolution studies in time and frequency, cone and core emission
of the pulsar beam, scintillation, pulse intensity distributions, and others.
It also constitutes a ready-made resource for teaching signal processing and
pulsar astronomy techniques.
