Binary detection probabilities as a function of the orbital period for four different observing strategies used to constitute our dataset: (1) two observations were obtained within 1 week and one observation 6 weeks later, (2) two observations were obtained spread over about 2 months, (3) four observations were obtained: two during 1 week, and two collected during another week 2 months later, and (4) two observations were obtained on consecutive nights and one observation 2 months later.