Resumen
We report the mass and distance measurements of two single-lens events from the 2017 Spitzer microlensing campaign. The ground-based observations yield the detection of finite-source effects, and the microlens parallaxes are derived from the joint analysis of ground-based observations and Spitzer observations. We find that the lens of OGLE-2017-BLG-1254 is a 0.60 0.03 M o star with D LS = 0.53 0.11 kpc, where D LS is the distance between the lens and the source. The second event, OGLE-2017-BLG-1161, is subject to the known satellite parallax degeneracy, and thus is either a star with D LS = 0.40 0.12 kpc or a star with D LS = 0.53 0.19 kpc. Both of the lenses are therefore isolated stars in the Galactic bulge. By comparing the mass and distance distributions of the eight published Spitzer finite-source events with the expectations from a Galactic model, we find that the Spitzer sample is in agreement with the probability of finite-source effects occurring in single-lens events.
Idioma original | Inglés |
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Número de artículo | 3 |
Publicación | Astrophysical Journal |
Volumen | 891 |
N.º | 1 |
DOI | |
Estado | Publicada - 2020 |
Nota bibliográfica
Publisher Copyright:© 2020. The American Astronomical Society. All rights reserved.
Áreas temáticas de ASJC Scopus
- Astronomía y astrofísica
- Ciencias planetarias y espacial