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Spitzer plus VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event
Indexado
WoS WOS:000553812300001
Scopus SCOPUS_ID:85088973774
DOI 10.3847/1538-4357/AB9749
Año 2020
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555 (Kojima-1). We measure the microlens parallax vector pi(E) using Spitzer and ground-based light curves with constraints on the direction of lens-source relative proper motion derived from Very Large Telescope Interferometer (VLTI) GRAVITY observations. Combining this pi(E) determination with the angular Einstein radius theta(E) measured by VLTI-GRAVITY observations, we find that the lens is a star with mass M-L = 0.495 +/- 0.063 M-circle dot at a distance D-L = 429 +/- 21 pc. We find that the blended light basically all comes from the lens. The lens-source proper motion is mu(rel, hel) = 26.55 +/- 0.36 mas yr(-1), so with currently available adaptive-optics instruments, the lens and source can be resolved in 2021. This is the first microlensing event whose lens mass is unambiguously measured by interferometry + satellite-parallax observations, which opens a new window for mass measurements of isolated objects such as stellar-mass black holes.

Revista



Revista ISSN
Astrophysical Journal 0004-637X

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Zang, Weicheng - Tsinghua Univ - China
Tsinghua University - China
2 Dong, Subo - Peking Univ - China
Peking University - China
3 Gould, Andrew - Max Planck Institute for Astronomy - Alemania
The Ohio State University - Estados Unidos
Max Planck Inst Astron - Alemania
4 Novati, Sebastiano Calchi Hombre CALTECH - Estados Unidos
Infrared Processing & Analysis Center - Estados Unidos
5 Chen, P. - Peking Univ - China
Peking University - China
6 Yang, Hongjing - Tsinghua Univ - China
Tsinghua University - China
7 Li, Shun-Sheng - CASSACA - China
Univ Chinese Acad Sci - China
National Astronomical Observatories Chinese Academy of Sciences - China
University of Chinese Academy of Sciences - China
8 Mao, Shude - Tsinghua Univ - China
CASSACA - China
Tsinghua University - China
National Astronomical Observatories Chinese Academy of Sciences - China
9 Alton, K. B. - Desert Blooms Observ - Chile
Desert Blooms Observatory - Chile
10 Brimacombe, J. Hombre Coral Towers Observ - Australia
Coral Towers Observatory - Australia
11 Carey, Sean Hombre CALTECH - Estados Unidos
Spitzer Science Center - Estados Unidos
12 Christie, G. W. - Auckland Observ - Nueva Zelanda
Stardome Observatory, Auckland - Nueva Zelanda
13 Delplancke-Strobele, F. - ESO - Alemania
Observatorio Europeo Austral - Alemania
European Southern Observ - Alemania
14 Feliz, Dax Hombre Vanderbilt Univ - Estados Unidos
Vanderbilt University - Estados Unidos
15 Gaudi, B. Scott - OHIO STATE UNIV - Estados Unidos
The Ohio State University - Estados Unidos
16 Green, J. - Kumeu Observ - Nueva Zelanda
Kumeu Observatory - Nueva Zelanda
17 Hu, Shao-Ming - Shandong Univ - China
Shandong University, Weihai - China
18 Jayasinghe, T. - OHIO STATE UNIV - Estados Unidos
The Ohio State University - Estados Unidos
19 Koff, R. A. - Antelope Hills Observ - Estados Unidos
Antelope Hills Observatory - Estados Unidos
20 Kurtenkov, Alexander Hombre Bulgarian Acad Sci - Bulgaria
Bulgarian Academy of Sciences - Bulgaria
The Bulgarian Academy of Sciences - Bulgaria
21 Merand, Antoine Hombre ESO - Alemania
Observatorio Europeo Austral - Alemania
European Southern Observ - Alemania
22 Minev, M. Hombre Univ Sofia - Bulgaria
Sofia University St. Kliment Ohridski - Bulgaria
Bulgarian Academy of Sciences - Bulgaria
University of Iowa - Bulgaria
23 Mutel, Robert Hombre UNIV IOWA - Estados Unidos
University of Iowa - Estados Unidos
24 Natusch, T. - AUT Univ - Nueva Zelanda
Auckland University of Technology - Nueva Zelanda
24 Gould, Andrew Hombre Max Planck Inst Astron - Alemania
OHIO STATE UNIV - Estados Unidos
Max Planck Institute for Astronomy - Alemania
The Ohio State University - Estados Unidos
25 Roth, Tyler Hombre UNIV IOWA - Estados Unidos
University of Iowa - Estados Unidos
26 Shvartzvald, Yossi Hombre Weizmann Inst Sci - Israel
Weizmann Institute of Science Israel - Israel
27 Espada, Daniel Hombre UNIV ARIZONA - Estados Unidos
The University of Arizona - Estados Unidos
28 Vanmunster, T. - Ctr Backyard Astrophys Belgium - Bélgica
Center for Backyard Astrophysics Belgium - Bélgica
29 Zhu, Wei - UNIV TORONTO - Canadá
Canadian Institute for Theoretical Astrophysics - Canadá
L’Institut Canadien d’Astrophysique Théorique - Canadá

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Financiamiento



Fuente
National Natural Science Foundation of China
National science foundation of China
National Key R&D Program of China
Natural Science Foundation of Shandong Province
NASA
Seventh Framework Programme
Young Scholars Program of Shandong University
National Science Foundation of China (NSFC)
JPL grant
Beatrice and Vincent Tremaine Fellowship at CITA
NASA through JPL/Caltech
European Research Council under the European Unions Seventh Framework Programme (FP 7) ERC

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
We thank Tianshu Wang, Jennifer Yee, Akihiko Fukui, and Naoki Koshimoto for fruitful discussions. We are grateful to Robin Leadbeater and Paolo Berardi for making their spectroscopic observations available to us during the observing campaign. S.D. and P.C. are supported by the National Key R&D Program of China No. 2019YFA0405100 and Projects 11573003 supported by the National Science Foundation of China (NSFC). W.Z., H.Y., S.-S.L., and S.M. acknowledge support by the National Science Foundation of China (grant No. 11821303 and 11761131004). Work by AG was supported by AST-1516842 and by JPL grant 1500811. A.G. received support from the European Research Council under the European Unions Seventh Framework Programme (FP 7) ERC grant Agreement No. [321035]. This work is based (in part) on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. Work by S.M.Hu. was supported by the Natural Science Foundation of Shandong province (No. JQ201702), and the Young Scholars Program of Shandong University (No. 20820162003). W.Z. was supported by the Beatrice and Vincent Tremaine Fellowship at CITA.
2020-07-01 2020-07-16 13:43:10 cgi/release: Article released bin/incoming: New from .zip National Science Foundation of China (NSFC) 11573003 National Science Foundation of China (NSFC) 11821303 National Science Foundation of China (NSFC) 11761131004 the European Research Council 321035 Natural Science Foundation of Shandong Province JQ201702 Young Scholars Program of Shandong University 20820162003 National Key R&D program of China 2019YFA0405100 yes

Muestra la fuente de financiamiento declarada en la publicación.