Terry SKBeaulieu J-PBennett DPBhattacharya AHulberg JHuston MJKoshimoto NBlackman JWBond IACole AALu JRRanc CRektsini NEVandorou A2025-03-122025-03-122025-03Terry SK, Beaulieu JP, Bennett DP, Bhattacharya A, Hulberg J, Huston MJ, Koshimoto N, Blackman JW, Bond IA, Cole AA, Lu JR, Ranc C, Rektsini NE, Vandorou A. (2025). A Candidate High-velocity Exoplanet System in the Galactic Bulge. Astronomical Journal. 169. 3.0004-6256https://mro.massey.ac.nz/handle/10179/72617We present an analysis of adaptive optics images from the Keck I telescope of the microlensing event MOA-2011-BLG-262. The original discovery paper by Bennett et al. reports two possibilities for the lens system: a nearby gas giant lens with an exomoon companion or a very low-mass star with a planetary companion in the Galactic bulge. The ∼10 yr baseline between the microlensing event and the Keck follow-up observations allows us to detect the faint candidate lens host (star) at K = 22.3 mag and confirm the distant lens system interpretation. The combination of the host star brightness and light curve parameters yields host star and planet masses of Mhost = 0.19 ± 0.03 M⊙ and mp = 28.92 ± 4.75 M⊕ at a distance of DL = 7.49 ± 0.91 kpc. We perform a multiepoch cross reference to Gaia Data Release 3 and measure a transverse velocity for the candidate lens system of vL = 541.31 ± 65.75 km s−1. We conclude this event consists of the highest-velocity exoplanet system detected to date, and also the lowest-mass microlensing host star with a confirmed mass measurement. The high-velocity nature of the lens system can be definitively confirmed with an additional epoch of high-resolution imaging at any time now. The methods outlined in this work demonstrate that the Roman Galactic Exoplanet Survey will be able to securely measure low-mass host stars in the bulge.(c) 2025 The Author/sCC BY 4.0https://creativecommons.org/licenses/by/4.0/. Unified Astronomy Thesaurus concepts: Exoplanets (498); Gravitational microlensing (672); High-resolution microlensing event imaging (2138); Adaptive optics (2281)ExoplanetsGravitational microlensingHigh-resolution microlensing event imagingAdaptive opticsJournal article10.3847/1538-3881/ad9b0f1538-3881journal-article131