  We report an attempt to detect molecular and atomic species in the atmosphere
of the ultra-hot Jupiter WASP-33b using the high-resolution echelle
spectrograph NEID with a wavelength coverage of 380$-$930 nm. By analyzing the
transmission spectrum of WASP-33b using the line-by-line technique and the
cross-correlation technique, we confirm previous detection of H$\alpha$,
H$\beta$, H$\gamma$, and Ca II infrared triplets. We find no evidence for a
significant day-to-night wind in WASP-33b, taking into account the effects of
stellar pulsations using a relatively novel GP method and poorly constrained
systemic velocity measurements. We also detect the previously reported
pre-transit absorption signal, which may be a pulsation mode induced by the
planet. Combined with previous CARMENES and HARPS-N observations, we report the
non-detection of TiO, Ti I, and V I in the transmission spectrum, while they
were already detected in the dayside atmosphere of WASP-33b. This implies a
difference in the chemical compositions and abundances between the dayside and
terminator atmospheres of WASP-33b, and certainly requires further improvements
in the sensitivity of the detection methods.
