KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with $\theta_{\rm E}$ measurements
Youn Kil Jung, Kyu-Ha Hwang, Hongjing Yang, Andrew Gould, Jennifer C., Yee, Cheongho Han, Michael D. Albrow, Sun-Ju Chung, Yoon-Hyun Ryu, In-Gu, Shin, Yossi Shvartzvald, Weicheng Zang, Sang-Mok Cha, Dong-Jin Kim, Seung-Lee, Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee

TL;DR
This paper reports the detection of a ninth free-floating planet candidate through microlensing, measuring its Einstein radius and timescale, and discusses the potential for future high-resolution imaging to find possible host stars.
Contribution
It presents the identification and characterization of a new free-floating planet candidate with precise measurements of its Einstein radius, and explores methods to detect potential host stars.
Findings
First measurement of $ heta_{E}$ for this candidate.
No strong evidence of a host star in the light curve.
Potential for high-resolution imaging to detect wide-separation hosts.
Abstract
We report a free-floating planet (FFP) candidate identified from the analysis of the microlensing event KMT-2023-BLG-2669. The lensing light curve is characterized by a short duration and a small amplitude . From the analysis, we find the Einstein timescale of and the Einstein radius of . These measurements enable us to infer the lens mass as , where is the relative lens-source parallax. The inference implies that the lens is a sub-Neptune- to Saturn-mass object depending on its unknown distance. This is the ninth isolated planetary-mass microlens with , which (as shown by \citealt{gould22}) is a useful threshold for a FFP candidate. We…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Solar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies
