PINES. II. Observations used for 131 light curves

We use this algorithm to search for transits in 131 PINES light curves and identify two transit candidates: 2MASSJ18212815+1414010 (2MASSJ1821+1414) and 2MASSJ08350622+1953050 (2MASSJ0835+1953). We disfavor 2MASSJ1821+1414 as a genuine transit candidate due to the known variability properties of the source.

We cannot rule out the planetary nature of 2MASSJ0835+1953's candidate event and perform follow-up observations in an attempt to recover a second transit. A repeat event has yet to be observed, but these observations suggest that target variability is an unlikely cause of the candidate transit. We perform a Markov Chain Monte Carlo simulation of the light curve and estimate a planet radius ranging from 4.2_-1.6_^+3.5^R{Earth} to 5.8_-2.1_^+4.8^R{Earth}, depending on the host's age.