Frymire & Ardila (2023) reported an anomalous flux variation in the
Transiting Exoplanet Survey Satellite (TESS) Sector 43 light curve of the white
dwarf HZ 4. We show that this flux variation was caused by the main-belt
asteroid 4382 Stravinsky traversing the nearby TESS pixels, and it is therefore
not a cause for concern regarding the continued use of HZ 4 as a photometric
standard star.Comment: Accepted for publication in Research Notes of the American
Astronomical Societ