OGLE-2018-BLG-0022: First Prediction of an Astrometric Microlensing Signal from a Photometric Microlensing Event
Abstract
In this work, we present the analysis of the binary microlensing event OGLE-2018-BLG-0022 that is detected toward the Galactic bulge field. The dense and continuous coverage with the high-quality photometry data from ground-based observations combined with the space-based Spitzer observations of this long timescale event enables us to uniquely determine the masses M_1 = 0.40 ± 0.05 M⊙ and M_2 = 0.13 ± 0.01 M⊙ of the individual lens components. Because the lens-source relative parallax and the vector lens-source relative proper motion are unambiguously determined, we can likewise unambiguously predict the astrometric offset between the light centroid of the magnified images (as observed by the Gaia satellite) and the true position of the source. This prediction can be tested when the individual-epoch Gaia astrometric measurements are released.
Additional Information
© 2019 The American Astronomical Society. Received 2019 February 3; revised 2019 March 29; accepted 2019 April 2; published 2019 May 7. Work by C.H. was supported by the grant (2017R1A4A1015178) of the National Research Foundation of Korea. Work by A.G. was supported by US NSF grant AST-1516842. Work by I.G.S. and A.G. were supported by JPL grant 1500811. A.G. received support from the European Research Council under the European Union's Seventh Framework Programme (FP 7) ERC grant Agreement No. [321035]. The MOA project is supported by JSPS KAKENHI grant No. JSPS24253004, JSPS26247023, JSPS23340064, JSPS15H00781, and JP16H06287. Y.M. acknowledges the support by the grant JP14002006. D.P.B., A.B., and C.R. were supported by NASA through grant NASA-80NSSC18K0274. The work by C.R. was supported by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by USRA through a contract with NASA. N.J.R. is a Royal Society of New Zealand Rutherford Discovery Fellow. The OGLE project has received funding from the National Science Centre, Poland, grant MAESTRO 2014/14/A/ST9/00121 to A.U.. This research has made use of the KMTNet system operated by the Korea Astronomy and Space Science Institute (KASI) and the data were obtained at three host sites of CTIO in Chile, SAAO in South Africa, and SSO in Australia. We acknowledge the high-speed Internet service (KREONET) provided by Korea Institute of Science and Technology Information (KISTI).Attached Files
Published - Han_2019_ApJ_876_81.pdf
Submitted - 1904.00139.pdf
Files
1904.00139.pdf
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Additional details
Identifiers
- Eprint ID
- 95343
- Resolver ID
- CaltechAUTHORS:20190508-094203825
Related works
- Describes
- https://arxiv.org/abs/1904.00139 (URL)
Funding
- National Research Foundation of Korea
- 2017R1A4A1015178
- NSF
- AST-1516842
- JPL
- 1500811
- European Research Council (ERC)
- 321035
- Japan Society for the Promotion of Science (JSPS)
- JSPS24253004
- Japan Society for the Promotion of Science (JSPS)
- JSPS26247023
- Japan Society for the Promotion of Science (JSPS)
- JSPS23340064
- Japan Society for the Promotion of Science (JSPS)
- JSPS15H00781
- Japan Society for the Promotion of Science (JSPS)
- JP16H06287
- Japan Society for the Promotion of Science (JSPS)
- JP14002006
- NASA
- 80NSSC18K0274
- NASA Postdoctoral Program
- Royal Society
- National Science Centre (Poland)
- MAESTRO 2014/14/A/ST9/00121
Dates
- Created
-
2019-05-08Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field