  We present timing solutions and analyses of 11 pulsars discovered by the
Five-hundred-meter Aperture Spherical radio Telescope (FAST). These pulsars
were discovered using an ultra-wide bandwidth receiver in drift-scan
observations made during the commissioning phase of FAST, and were then
confirmed and timed using the 64-m Parkes Radio Telescope. Each pulsar has been
observed over a span of at least one year. Highlighted discoveries include PSR
J0344-0901, which displays mode-changing behaviour and may belong to the class
of so-called `swooshing' pulsars (alongside PSRs B0919+06 and B1859+07); PSR
J0803-0942, whose emission is almost completely linearly polarised; and PSRs
J1900-0134 and J1945+1211, whose well defined polarisation angle curves place
stringent constraints on their emission geometry. We further discuss the
detectability of these pulsars by earlier surveys, and highlight lessons
learned from our work in carrying out confirmation and monitoring observations
of pulsars discovered by a highly sensitive telescope, many of which may be
applicable to next-generation pulsar surveys. This paper marks one of the first
major releases of FAST-discovered pulsars, and paves the way for future
discoveries anticipated from the Commensal Radio Astronomy FAST Survey
(CRAFTS).
