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Data from Wheeler & Kipping 2019. Find our code at github.com/coolworlds/weirddetector

  • detections.csv contains the period with the highest zeta value (merit function) for each KIC we analyzed. The is_known column is true for KICs we threw out in our analysis , i.e. those in the Villanova eclipsing binary catalog (Kirk et al. 2016; Abdul-Masih et al. 2016), Kepler KOIs and TCEs (Thompson et al. 2018), the candidates from (Huang et al. 2013), the long-period candidates from the wavelet-based search of Foreman-Mackey et al. (2016) and planet hunters (Wang et al. 2015), and the ultra-short period planets in Sanchis Ojeda et al. (2015)

  • multinest_files contains the output of multinest for each fit to a transit candidate (each row in table 2).

    • the parameters for the candidates fit with e==0 (KIC 4754691, KIC 9955874, and KIC 10190048) are ["$t_0$", "$R_p/R_*$","$\\log(P)$", "$b$", "$\\log(\\rho_*)$", "$q_1$", "$q_2$", "A", "B"], where A and B specify a local linear trend of the form A*(t-t0) + B

    • the parameters for the candidates fit with eccentricity unfixed (KIC 5475628 and KIC 10474113) are ["$cos(w)$", "$sqrt(e)sin(w)$", "$t_0$", "$R_p/R_*$","$\\log(P)$", "$b$", "$\\log(\\rho_*)$", "$q_1$", "$q_2$", "A", "B"], where A and B specify a local linear trend of the form A*(t-t0) + B

    • the parameters for KIC 7947784 are ["$t_1$", "$R_1/R_*$", "$\log(P_1)$", "$b_1$", "$A_1$", "$B_1$", "$t_2$", "$R_2/R_*$","$\log(P_2)$", "$b_2$", "$A_2$", "$B_2$", "$\\log(\\rho_*)$", "$q_1$", "$q_2$"]

    • the parameters for KIC 8508736 are ["$t_1$", "$t_2$", "$R_p$", "$a$", "$b$", "$q_1$", "$q_2$"]

Priors

t0 (as well at t1 and t2, the epochs of KIC 8508736) was given a uniform prior of width 0.04 days centered on the approximate transit epoch. This is much wider than the posterior width for this parameter.

We sample uniformly in log(rho), but apply a skewed-normal prior from Mathur+2018 as a penalty to the log-likelihood (see equation 10 in the paper for details).

The applied prior was uniform in the remaining sampling parameters, with bounds listed below.

parameter lower bound upper bound
Rplanet / Rstar 0 1
log(P / 1 day) 2.7 6
b 0 1
log(rho / (g/cc)) -7 2
q1 0 1
q2 0 1
A -0.02 0.02
B -0.02 0.02
cos(w) -1 1
sqrt(e)sin(w) 0 1

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