Gould, Andrew, Dong, Subo, Bennett, David P., Bond, Ian A., Udalski, Andrzej, Kozlowski, Szymon
At present, microlensing light curves from different telescopes and filters are photometrically aligned by fitting them to a common model. We present a second method based on photometry of common...
Gaudi, B. Scott, Bennett, David P., Bond, Ian A., Dong, Subo, Gould, Andrew, ...
In the currently-favored paradigm of planet formation, the location of the snow line in the protoplanetary disk plays a crucial role. Determining the demographics of planets beyond the snow line of...
A High-Resolution Spectrum of the Highly Magnified Bulge G-Dwarf MOA-2006-BLG-099S (2008)
Johnson, Jennifer A., Gaudi, B. Scott, Sumi, Takahiro, Bond, Ian A., Gould, Andrew
We analyze a high-resolution spectrum of a microlensed G-dwarf in the Galactic bulge, acquired when the star was magnified by a factor of 110. We measure a spectroscopic temperature, derived from the...
Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 Planetary Host Star (2006)
Bennett, David P., Anderson, Jay, Bond, Ian A., Udalski, Andrzej, Gould, Andrew
We present the results of HST observations of the host star for the first definitive extrasolar planet detected by microlensing. The light curve model for this event predicts that the lens star...
Detecting Extra-Solar Planets via Microlensing at High Magnification (2002)
Rattenbury, Nicholas J., Bond, Ian A., Skuljan, Jovan, Yock, Phil
Extra-solar planets can be efficiently detected in gravitational microlensing events of high magnification. High accuracy photometry is required over a short, well-defined time interval only, of...