I entered the
astrophysics field of microlensing as an intern at Goddard Space Flight Center
over the summer; for all intents and purposes, I brought my work back with me
for the fall semester. It hit me on the 10th of July – given our
equipment at the GMU observatory, we should be able to detect microlensing
events! At the beginning I was optimistic but hesitant about the prospects of
the research, but the more I read into other observatory locations and
equipment, the more confident I grew about the chances o f successfully
detecting these magnification events. The exoplanet research group here at
Mason discovered only the other year that the observatory was capable of conducting
research on transit-timing but no one had yet looked into microlensing, so my
mentor and I changed our project from moon composition mapping to microlensing.
Just the question of whether or not we really could see these events was
exciting enough for us to go forward with the research.
The project has
been a huge success so far, and I would like to see microlensing research
continue at Mason. It’s my hope that our data will prove our location is
conducive for these observations in the northern hemisphere, and thus be added
as an observatory location for one of several international follow-up
microlensing detection surveys. Not only that but I would like to get other
universities in Virginia involved to create a student research network between
the physics departments across the state.
Observations
are conducted as often as possible, weather permitting; such is the nature of
ground-based astrophysics research. In order to maximize the number of targets
we point to each night, we prioritize targets by elevation in the sky –
observing the targets lowest in the sky first and working up to the targets at
higher elevations – and we have to move quickly when observing because of the
time it takes to point the telescope and observatory dome in the direction of
the designated target event. Outside of the observatory I spend most of my time
(currently) triangulating the position of these events within our images, which
sounds much easier than the actual process. Soon, however, the observations
from our location will be out of our view and we’ll move on to data processing
in order to finalize our results.
This past week
in particular was rather exciting; we did not expect to see a lot of these
events at our latitude – they are rare in general – but after reviewing two
different observatory lists of hundreds of these events, our list of targets
rose from eight to nineteen, and we were just alerted of several more!