We present a catalog of 450 high signal-to-noise microlensing events observed by the MA-CHO colla... more We present a catalog of 450 high signal-to-noise microlensing events observed by the MA-CHO collaboration between 1993 and 1999. The events are distributed throughout our fields and, as expected, they show clear concentration toward the Galactic center. No optical depth is given for this sample since no blending efficiency calculation has been performed, and we find evidence for substantial blending. In a companion paper we give optical depths for the sub-sample of events on clump giant source stars, where blending is not a significant effect.
We present a catalog of 450 high signal-to-noise microlensing events observed by the MA-CHO colla... more We present a catalog of 450 high signal-to-noise microlensing events observed by the MA-CHO collaboration between 1993 and 1999. The events are distributed throughout our fields and, as expected, they show clear concentration toward the Galactic center. No optical depth is given for this sample since no blending efficiency calculation has been performed, and we find evidence for substantial blending. In a companion paper we give optical depths for the sub-sample of events on clump giant source stars, where blending is not a significant effect.
Uploads
Papers by W. Sutherland