  We present new HI observations of the REionization-Limited HI Cloud (RELHIC)
candidate, M94-CL9, detected around M94 by Zhou et al. using the
Five-hundred-meter Aperture Spherical Telescope (FAST). M94-CL9's HI properties
as detected by FAST are consistent with a RELHIC as noted by Benitez-Llambay &
Navarro. Our observations with the Robert C. Byrd Green Bank Telescope (GBT)
detect greater HI emission in M94-CL9 and result in HI properties that are
larger (corrected velocity width, $W_{50,c,t}=35.7\pm0.6\,\mathrm{km\,s^{-1}}$;
and integrated flux,
$\int\mathrm{Sdv}=0.28\pm0.04\,\mathrm{Jy}\cdot\mathrm{km\,s^{-1}}$) than those
found by Zhou et al. but that match those from the FAST All-Sky HI (FASHI)
survey. These larger properties do not preclude M94-CL9 from being a RELHIC,
but the wider spectral extent and spectral asymmetry reported here may be in
tension with predictions of RELHIC properties.
