Hu ZZhu WGould AUdalski ASumi TChen PCalchi Novati SYee JCBeichman CABryden GCarey SFausnaugh MScott Gaudi BHenderson CBShvartzvald YWibking BMroz PSkowron JPoleski RSzymanski MKSoszynski IPietrukowicz PKozłowski SUlaczyk KRybicki KAIwanek PWrona MGromadzki MGAbe FBarry RBennett DPBhattacharya ABond IAFujii HFukui AHamada RHirao YSilva SIItow YKirikawa RKoshimoto NMatsubara YMiyazaki SMuraki YOlmschenk GRanc CRattenbury NJSatoh YSuzuki DTomoyoshi MTristram PJVandorou AYama HYamashita K2024-10-202024-10-202024-09-01Hu Z, Zhu W, Gould A, Udalski A, Sumi T, Chen P, Calchi Novati S, Yee JC, Beichman CA, Bryden G, Carey S, Fausnaugh M, Scott Gaudi B, Henderson CB, Shvartzvald Y, Wibking B, Mroz P, Skowron J, Poleski R, Szymanski MK, Soszynski I, Pietrukowicz P, Kozłowski S, Ulaczyk K, Rybicki KA, Iwanek P, Wrona M, Gromadzki M, Abe F, Barry R, Bennett DP, Bhattacharya A, Bond IA, Fujii H, Fukui A, Hamada R, Hirao Y, Silva SI, Itow Y, Kirikawa R, Koshimoto N, Matsubara Y, Miyazaki S, Muraki Y, Olmschenk G, Ranc C, Rattenbury NJ, Satoh Y, Suzuki D, Tomoyoshi M, Tristram PJ, Vandorou A, Yama H, Yamashita K. (2024). OGLE-2015-BLG-0845L: a low-mass M dwarf from the microlensing parallax and xallarap effects. Monthly Notices of the Royal Astronomical Society. 533. 2. (pp. 1991-2004).0035-8711https://mro.massey.ac.nz/handle/10179/71771We present the analysis of the microlensing event OGLE-2015-BLG-0845, which was affected by both the microlensing parallax and xallarap effects. The former was detected via the simultaneous observations from the ground and Spitzer, and the latter was caused by the orbital motion of the source star in a relatively close binary. The combination of these two effects led to a mass measurement of the lens object, revealing a low-mass (0.14 ± 0.05 M) M dwarf at the bulge distance (7.6 ± 1.0 kpc). The source binary consists of a late F-type subgiant and a K-type dwarf of ∼ 1.2 and ∼ 0.9M, respectively, and the orbital period is 70 ± 10 d. OGLE-2015-BLG-0845 is the first single-lens event in which the lens mass is measured via the binarity of the source. Given the abundance of binary systems as potential microlensing sources, the xallarap effect may not be a rare phenomenon. Our work thus highlights the application of the xallarap effect in the mass determination of microlenses, and the same method can be used to identify isolated dark lenses.(c) The author/shttps://creativecommons.org/licenses/by/4.0/gravitational lensingmicro – methodsdata analysis – binariesgeneralJournal article10.1093/mnras/stae19061365-2966CC BYjournal-article1991-2004