Research
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Non-interacting compact objects
Most known stellar black holes are members of close binaries, where accretion-fueled X-ray emission was able to trigger their detection. However, if the separation between the two components is sufficiently large, the accretion rate drops, leaving the black hole in quiescence. Presumably, most black holes in binaries reside in this dormant state, waiting to be discovered. I use the astrometric orbits provided by the Gaia mission to identify and study these systems.
Extreme precision radial velocity
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Ultra-short period planets
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Transit duration variation
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