The James Webb Space Telescope (JWST) is the scientific successor to the Hubble and Spitzer Space Telescopes. Goddard Space Flight Center (GSFC) is providing a fully tested and characterized detector subsystem for the JWST near-infrared spectorgraph (NIRSpec). Considering the small photon rate per pixel for faint object spectroscopy, this detector has challenging noise requirements. Given the low background in space, the detector itself will typically be the dominant source of noise. Non-ideal pixel behavior will contribute to detector noise. Already, several anomalous behaviors have been observed in the NIRSpec HAWAII-2RG (H2RG) detectors and more are left for discovery. A more detailed study of these detectors and their non-ideal behavior is necessary to reduce noise and optimize sensitivity.