The Astrophysical Journal (Jan 2024)

Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia Predictions

  • Krzysztof A. Rybicki,
  • Yossi Shvartzvald,
  • Jennifer C. Yee,
  • Sebastiano Calchi Novati,
  • Eran O. Ofek,
  • Ian A. Bond,
  • Charles Beichman,
  • Geoff Bryden,
  • Sean Carey,
  • Calen Henderson,
  • Wei Zhu,
  • Michael M. Fausnaugh,
  • Benjamin Wibking,
  • The Spitzer Team,
  • Andrzej Udalski,
  • Radek Poleski,
  • Przemek Mróz,
  • Michał K. Szymański,
  • Igor Soszyński,
  • Paweł Pietrukowicz,
  • Szymon Kozłowski,
  • Jan Skowron,
  • Krzysztof Ulaczyk,
  • Patryk Iwanek,
  • Marcin Wrona,
  • The OGLE Collaboration,
  • Yoon-Hyun Ryu,
  • Michael D. Albrow,
  • Sun-Ju Chung,
  • Andrew Gould,
  • Cheongho Han,
  • Kyu-Ha Hwang,
  • Youn Kil Jung,
  • In-Gu Shin,
  • Hongjing Yang,
  • Weicheng Zang,
  • Sang-Mok Cha,
  • Dong-Jin Kim,
  • Hyoun-Woo Kim,
  • Seung-Lee Kim,
  • Chung-Uk Lee,
  • Dong-Joo Lee,
  • Yongseok Lee,
  • Byeong-Gon Park,
  • Richard W. Pogge,
  • The KMTNet Collaboration,
  • Fumio Abe,
  • Richard Barry,
  • David P. Bennett,
  • Aparna Bhattacharya,
  • Akihiko Fukui,
  • Ryusei Hamada,
  • Shunya Hamada,
  • Naoto Hamasaki,
  • Yuki Hirao,
  • Stela Ishitani Silva,
  • Yoshitaka Itow,
  • Rintaro Kirikawa,
  • Naoki Koshimoto,
  • Yutaka Matsubara,
  • Shota Miyazaki,
  • Yasushi Muraki,
  • Tutumi Nagai,
  • Kansuke Nunota,
  • Greg Olmschenk,
  • Clement Ranc,
  • Nicholas J. Rattenbury,
  • Yuki K. Satoh,
  • Takahiro Sumi,
  • Daisuke Suzuki,
  • Paul. J. Tristram,
  • Aikaterini Vandorou,
  • Hibiki Yama,
  • MOA collaboration,
  • Łukasz Wyrzykowski,
  • Kornel Howil,
  • Katarzyna Kruszyńska

DOI
https://doi.org/10.3847/1538-4357/ad7bb1
Journal volume & issue
Vol. 975, no. 2
p. 216

Abstract

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In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of ∼950 microlensing events observed by the Spitzer Space Telescope between 2014 and 2019. In this study we focus on a subsample of nine microlensing events, selected based on their long timescales, small microlensing parallaxes, and joint observations by the Gaia mission, to increase the probability that the chosen lenses are massive and the mass is measurable. Among the selected events we identify lensing black holes and neutron star candidates, with potential confirmation through forthcoming release of the Gaia time-series astrometry in 2026. Utilizing Bayesian analysis and Galactic models, along with the Gaia Data Release 3 proper-motion data, four good candidates for dark remnants were identified: OGLE-2016-BLG-0293, OGLE-2018-BLG-0483, OGLE-2018-BLG-0662, and OGLE-2015-BLG-0149, with lens masses of ${3.0}_{-1.3}^{+1.8}\,{M}_{\odot }$ , ${4.7}_{-2.1}^{+3.2}\,{M}_{\odot }$ , ${3.15}_{-0.64}^{+0.66}\,{M}_{\odot }$ and ${1.40}_{-0.55}^{+0.75}\,{M}_{\odot }$ , respectively. Notably, the first two candidates are expected to exhibit astrometric microlensing signals detectable by Gaia, offering the prospect of validating the lens masses. The methodologies developed in this work will be applied to the full Spitzer microlensing sample, populating and analyzing the timescale ( t _E ) versus parallax ( π _E ) diagram to derive constraints on the population of lenses in general and massive remnants in particular.

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