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Dynamical Constraints on the HR 8799 Planets with GPI
The orbit and transit prospects for {beta} Pictoris b constrained with one milliarcsecond astrometry
GPI spectra of \objS{HR 8799 c}{HR 8799 c}, \objS{HR 8799 d}{d}, and \objS{HR 8799 e}{e} from 1.5 to 2.4 {mu}m with KLIP forward modeling
Improving and Assessing Planet Sensitivity of the GPI Exoplanet Survey with a Forward Model Matched Filter
