Information on Service 'Time series for the microlensing event OGLE-2015-BLG-0060'
Further access options are discussed below
We present the analysis of stellar binary microlensing event
OGLE-2015-BLG-0060 based on observations obtained from 13 different
telescopes. Intensive coverage of the anomalous parts of the light
curve was achieved by automated follow-up observations from the
robotic telescopes of the Las Cumbres Observatory. We show that, for
the first time, all main features of an anomalous microlensing event
are well covered by follow-up data, allowing us to estimate the
physical parameters of the lens. The strong detection of second-order
effects in the event light curve necessitates the inclusion of
longer-baseline survey data in order to constrain the parallax vector.
We find that the event was most likely caused by a stellar binary-lens
with masses M_star1 = 0.87 ± 0.12 Msun and M_star2 = 0.77 ± 0.11Msun.
The distance to the lensing system is 6.41 ± 0.14 kpc and the
projected separation between the two components is 13.85 ± 0.16 AU.
This collection contains lightcurves resulting from different data
processing pipelines in a common reduction. See the accompanying paper
for details.
For a list of all services and tables belonging to this service's
resource, see Information on resource 'Time series for the microlensing event OGLE-2015-BLG-0060'
Overview
You can access this service using:
-
static --
static (i.e. prepared) data or custom client-side code; probably used to access ancillary files here
-
fixed --
a custom page, possibly with dynamic content
This service is published as follows:
- Within the
set(s) local with the renderer
fixed
local means it is listed on our front page,
ivo_managed means
it has a record in the VO registry.
Citation Info
VOResource XML (that's something exclusively for VO nerds)