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. Theis_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 ofmultinest
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"]
, whereA
andB
specify a local linear trend of the formA*(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"]
, whereA
andB
specify a local linear trend of the formA*(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
["$t_1$", "$t_2$", "$R_p$", "$a$", "$b$", "$q_1$", "$q_2$"]
-
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 |