The Astrophysical Journal (Jan 2025)

Observations of Microlensed Images with Dual-field Interferometry: On-sky Demonstration and Prospects

  • Przemek Mróz,
  • Subo Dong,
  • Antoine Mérand,
  • Jinyi Shangguan,
  • Julien Woillez,
  • Andrew Gould,
  • Andrzej Udalski,
  • Frank Eisenhauer,
  • Yoon-Hyun Ryu,
  • Zexuan Wu,
  • Zhuokai Liu,
  • Hongjing Yang,
  • —,
  • Guillaume Bourdarot,
  • Denis Defrère,
  • Antonia Drescher,
  • Maximilian Fabricius,
  • Paulo Garcia,
  • Reinhard Genzel,
  • Stefan Gillessen,
  • Sebastian F. Hönig,
  • Laura Kreidberg,
  • Jean-Baptiste Le Bouquin,
  • Dieter Lutz,
  • Florentin Millour,
  • Thomas Ott,
  • Thibaut Paumard,
  • Jonas Sauter,
  • T. Taro Shimizu,
  • Christian Straubmeier,
  • Matthias Subroweit,
  • Felix Widmann,
  • (The GRAVITY+ Collaboration),
  • Michał K. Szymański,
  • Igor Soszyński,
  • Paweł Pietrukowicz,
  • Szymon Kozłowski,
  • Radosław Poleski,
  • Jan Skowron,
  • Krzysztof Ulaczyk,
  • Mariusz Gromadzki,
  • Krzysztof Rybicki,
  • Patryk Iwanek,
  • Marcin Wrona,
  • Mateusz J. Mróz,
  • (The OGLE Collaboration),
  • Michael D. Albrow,
  • Sun-Ju Chung,
  • Cheongho Han,
  • Kyu-Ha Hwang,
  • Youn Kil Jung,
  • In-Gu Shin,
  • Yossi Shvartzvald,
  • Jennifer C. Yee,
  • Weicheng Zang,
  • Sang-Mok Cha,
  • Dong-Jin Kim,
  • Seung-Lee Kim,
  • Chung-Uk Lee,
  • Dong-Joo Lee,
  • Yongseok Lee,
  • Byeong-Gon Park,
  • Richard W. Pogge,
  • (KMTNet Collaboration)

DOI
https://doi.org/10.3847/1538-4357/ad9b14
Journal volume & issue
Vol. 980, no. 1
p. 47

Abstract

Read online

Interferometric observations of gravitational microlensing events offer an opportunity for precise, efficient, and direct mass and distance measurements of lensing objects, especially those of isolated neutron stars and black holes. However, such observations have previously been possible for only a handful of extremely bright events. The recent development of a dual-field interferometer, GRAVITY Wide, has made it possible to reach out to significantly fainter objects and increase the pool of microlensing events amenable to interferometric observations by 2 orders of magnitude. Here, we present the first successful observation of a microlensing event with GRAVITY Wide and the resolution of microlensed images in the event OGLE-2023-BLG-0061/KMT-2023-BLG-0496. We measure the angular Einstein radius of the lens with subpercent precision, θ _E = 1.280 ± 0.009 mas. Combined with the microlensing parallax detected from the event light curve, the mass and distance to the lens are found to be 0.472 ± 0.012 M _⊙ and 1.81 ± 0.05 kpc, respectively. We present the procedure for the selection of targets for interferometric observations and discuss possible systematic effects affecting GRAVITY Wide data. This detection demonstrates the capabilities of the new instrument, and it opens up completely new possibilities for the follow-up of microlensing events and future routine discoveries of isolated neutron stars and black holes.

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