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We produce light curves for all ~34,000 targets observed with K2 in Campaign17 (C17), identifying 34 planet candidates, 184 eclipsing binaries, and 222other periodic variables. The location of the C17 field means follow-up canbegin immediately now that the campaign has concluded and interesting targetshave been identified. The C17 field has a large overlap with C6, so this latestcampaign also offers a rare opportunity to study a large number of targetsalready observed in a previous K2 campaign. The timing of the C17 data release,shortly before science operations begin with the Transiting Exoplanet SurveySatellite (TESS), also lets us exercise some of the tools and methods developedfor identification and dissemination of planet candidates from TESS. We findexcellent agreement between these results and those identified using onlyK2-based tools. Among our planet candidates are several planet candidates withsizes < 4 R_E and orbiting stars with KepMag < 10 (indicating good RV targetsof the sort TESS hopes to find) and a Jupiter-sized single-transit event arounda star already hosting a 6 d planet candidate.

A TESS Dress Rehearsal: Planetary Candidates and Variables from K2 Campaign 17