When a nearby star or brown dwarf passes close to the line of sight of a distant star (within a few arcsecondes) it produces a shift in the position of the background star of a few dozen to hundred of microarcsecondes, in reach of upcoming interferometers such as VLTI's PRIMA or LINC-NIRVANA on the LBT, that will gives a direct (model-independent) mass measurement. Using existing high-quality position and proper motion catalogues, you'll search for targets for these new machines: objects that we expect will produce a microlensing signal, that we will later monitor to measure their mass.
You will search in large databases using (partly existing) scripts, and select the most interesting targets. At least 3 months in total. |