A Transition Discovered in the Subcritical Regime of 1A 0535+262

We present NICER observations of accreting X-ray pulsar 1A 0535+262 during its faint state ($\lesssim 6\times {10}^{36}$ erg/s) observed in several type I and II outbursts. We discovered a transition of temporal and spectral properties around the luminosity $L_{\mathrm{t}}=3.3\times {10}^{35}$ erg/s, below which spectra are relatively soft and the pulse profiles have only a narrow peak. The spectra are harder and a secondary hump gradually appears in pulse profiles when $L\gtrsim L_{\mathrm{t}}$. We discuss possible physical mechanisms for this transition, including different Comptonization seed photons, the disappearance of gas shocks on the neutron star surface, and the combination of plasma and vacuum polarization effects.