  Using integrated spectra for two gravitationally lensed galaxies from the
JWST TEMPLATES Early Release Science program, we analyze faint auroral lines,
which provide direct measurements of the gas-phase chemical abundance. For the
brighter galaxy, SGAS1723$+$34 ($z = 1.3293$), we detect the
[OIII]$\lambda4363$, [SIII]$\lambda6312$, and [OII]$\lambda\lambda$7320,7330
auroral emission lines, and set an upper limit for the [NII]$\lambda5755$ line.
For the second galaxy, SGAS1226$+$21 ($z = 2.925$), we do not detect any
auroral lines, and report upper limits. With these measurements and upper
limits, we constrain the electron temperatures in different ionization zones
within both of these galaxies. For SGAS1723$+$34, where auroral lines are
detected, we calculate direct oxygen and nitrogen abundances, finding an N/O
ratio consistent with observations of nearby ($z\sim 0$) galaxies. These
observations highlight the potent combination of JWST and gravitational lensing
to measure faint emission lines in individual distant galaxies and to directly
study the chemical abundance patterns in those galaxies.
