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We present timing solutions and analyses of 11 pulsars discovered by theFive-hundred-meter Aperture Spherical radio Telescope (FAST). These pulsarswere discovered using an ultra-wide bandwidth receiver in drift-scanobservations made during the commissioning phase of FAST, and were thenconfirmed and timed using the 64-m Parkes Radio Telescope. Each pulsar has beenobserved over a span of at least one year. Highlighted discoveries include PSRJ0344-0901, which displays mode-changing behaviour and may belong to the classof so-called `swooshing' pulsars (alongside PSRs B0919+06 and B1859+07); PSRJ0803-0942, whose emission is almost completely linearly polarised; and PSRsJ1900-0134 and J1945+1211, whose well defined polarisation angle curves placestringent constraints on their emission geometry. We further discuss thedetectability of these pulsars by earlier surveys, and highlight lessonslearned from our work in carrying out confirmation and monitoring observationsof pulsars discovered by a highly sensitive telescope, many of which may beapplicable to next-generation pulsar surveys. This paper marks one of the firstmajor releases of FAST-discovered pulsars, and paves the way for futurediscoveries anticipated from the Commensal Radio Astronomy FAST Survey(CRAFTS).

An in-depth investigation of 11 pulsars discovered by FAST