SIGNALMEN and anomaly light curves
Up-to-the-minute microlensing model light curves along with data collected
by OGLE, MOA, MiNDSTEp, RoboNet-II, MicroFUN, and uFUN-PLANET
Show magnitude shifts for multiple sites
The observed flux at time t reads F(t)
= FSA(t) + FB, where
the source flux FS and the background flux
FB are specific to each observing site and filter,
while A(t) denotes the theoretical magnification.
In order to put
different data sets
(ti, Fi, σFi) on the same plot, we show the theoretical magnitude shift
Δm = 2.5 lg A(t) along with
mi = 2.5 lg Ai and the error bar
σmi = [2.5/ln(10)] [σFi/|FSAi|]. Epochs for
which Ai ≤ 0 are marked by small stars below the
PLEASE NOTE THE FOLLOWING:
All data displayed on the plots fall under the copyright of the respective observing team. Please consult their webpages for the policies that apply
to their use.
All data are the result of preliminary reductions. Despite the fact that
all teams aim at providing as accurate data as possible,
no warranty whatsoever is
given, and they may be withdrawn at any time.