Projects per year
Abstract
We report on the mass and distance measurements of two single-lens events from the 2015 Spitzer microlensing campaign. With both finite-source effect and microlens parallax measurements, we find that the lens of OGLE-2015-BLG-1268 is very likely a brown dwarf (BD). Assuming that the source star lies behind the same amount of dust as the Bulge red clump, we find the lens is a 45 ± 7 M_jup }BD at 5.9 ± 1.0 kpc. The lens of of the second event, OGLE-2015-BLG-0763, is a 0.50 ± 0.04 M_sun star at 6.9 ± 1.0 kpc. We show that the probability to definitively measure the mass of isolated microlenses is dramatically increased once simultaneous ground- and space-based observations are conducted.
| Original language | English |
|---|---|
| Article number | 60 |
| Number of pages | 10 |
| Journal | Astrophysical Journal |
| Volume | 825 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 27 Jun 2016 |
Keywords
- Brown dwarfs
- Gravitational lensing: micro
- Stars: fundamental parameters
Fingerprint
Dive into the research topics of 'Mass measurements of isolated objects from space-based microlensing'. Together they form a unique fingerprint.Projects
- 1 Finished
-
Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018
Jardine, M. (PI), Cameron, A. (CoI), Cyganowski, C. (CoI), Horne, K. (CoI) & Wood, K. (CoI)
Science & Technology Facilities Council
1/04/15 → 31/03/18
Project: Standard
Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver