Flickers, Bursts, and Dips: Detecting Rapid Variability with the <i>g</i> ⁽²⁾ Autocorrelation Function

Abstract Rapid optical transient events can be hard to detect because of the limited number of photons they produce. I discuss a method of inferring the presence of fast, chaotic variability in photometry using the normalized autocorrelation function, what is called g (2) in quantum optics. The variability’s signature is a bump in the function at short lags. No periodicity is needed for the method to work. Versions of this method are attested in stellar variability studies, but its uses in some other subfields apparently have not been realized. I calculate expected signal-to-noise ratios with shot noise and scintillation. This method could be used to find unknown phenomena, particularly submillisecond optical variability. I present simple models of three example use cases: a flickering artificial “lantern” near a host Sun, optical microbursts from the Crab pulsar, and frequent irregular transits of a star by cometary bodies.