data validation (dv) reportexoplanetarchive.ipac.caltech.edu/data/keplerdata/010/... ·...

Data Validation (DV) Reportfor Kepler ID 10905746

Quarters 1 - 17

This Data Validation Report was produced in theKepler Science Operations Center Pipeline

at NASA Ames Research Center

01-Feb-2016 06:49:08 Z

This page intentionally left blank.

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Contents

1 Summary 1

2 UKIRT Image 2

3 Flux Time Series 3

4 Dashboards 13

5 Centroid Cloud Plot 15

6 Image Artifacts 166.1 Planet Candidate 1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166.2 Planet Candidate 2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16

7 Pixel Level Diagnostics 177.1 Planet Candidate 1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177.2 Planet Candidate 2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45

8 Phased Light Curves 73

9 Planet Candidate 1 779.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 779.2 Model Fitter: Reduced Parameter Fit Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 859.3 Model Fitter: Trapezoidal Fit Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 879.4 Validation Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 89

9.4.1 Weak Secondary Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 899.4.2 Flux-Weighted Centroid Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 899.4.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 909.4.4 Bootstrap Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 909.4.5 Ghost Diagnostic Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 909.4.6 Validation Test Figures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91

10 Planet Candidate 2 10310.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10310.2 Model Fitter: Reduced Parameter Fit Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11110.3 Model Fitter: Trapezoidal Fit Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11310.4 Validation Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115

10.4.1 Weak Secondary Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11510.4.2 Flux-Weighted Centroid Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11510.4.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11610.4.4 Bootstrap Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11610.4.5 Ghost Diagnostic Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11610.4.6 Validation Test Figures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117

Appendices 129

iii

A Planet Candidate 1 129A.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129A.2 Model Fitter: Odd & Even Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131A.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142

B Planet Candidate 2 143B.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 143B.2 Model Fitter: Odd & Even Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145B.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156

C Single Event Statistics from Residual Flux 157

D Alerts 158

iv

1 SUMMARY Target 10905746

1 Summary

Target Properties Value Uncertainty Units Provenance

Kepler ID 10905746KOI ID K01725Kepler Name -Sky Group 12RA 18.90858870 0 hours KICDec 48.39100300 0 degrees KICMagnitude 13.496 0 KICRadius 0.42 0.056 Solar radii DSEPEffective Temperature 3609 81 Kelvin SPE70log(g) 4.84 0.055 cm/sec2 SPE60[Fe/H] -0.06 0.15 Solar metallicity SPE70Number of Planet Candidates 2Categories ST SC1, MERGED, ST SC3, PLANETARY, ST SC2, UNCLASSIFIED, INCLUDEKOI Model cumulative 20150925110000.csvKepler Names Model keplernames 20150925110000.csvExternal TCE Model -Software Revision svn+ssh://murzim/repo/soc/tags/release/9.3.42@60958Date Report Generated 01-Feb-2016 06:49:08 Z

Quarter Target Module/ Crowding Flux Limb Darkening CoefficientsTable Output Metric Fraction 1 2 3 4

1 20 6/4 0.9986 0.9511 0.4772 0.6629 -0.4038 0.080511 50 20/4 1.0000 0.9302 0.4772 0.6629 -0.4038 0.080512 53 4/4 1.0000 0.8853 0.4772 0.6629 -0.4038 0.080513 56 6/4 0.9983 0.9439 0.4772 0.6629 -0.4038 0.080514 59 22/4 0.9998 0.8714 0.4772 0.6629 -0.4038 0.080515 62 20/4 1.0000 0.9301 0.4772 0.6629 -0.4038 0.080516 65 4/4 1.0000 0.7766 0.4772 0.6629 -0.4038 0.080517 68 6/4 1.0000 0.8609 0.4772 0.6629 -0.4038 0.0805

Planet KOI ID Kepler KOI Period Period Epoch Semi-major Radius Teq False SuspectedCandidate Name Correlation (days) Ratio (BKJD) Axis (AU) (Re) (K) Alarm EB

1 - - - 9.9 1.0 138.4 0.1 1.9 393 0.00e+00 false2 - - - 107.4 10.9 218.5 0.3 1.0 177 8.86e-15 false

DV did not produce matching results for the following KOI IDs: K01725.01

1

2 UKIRT IMAGE Target 10905746

2 UKIRT Image

UKIRT Wide Field Camera (WFCAM) infra-red J-band image. The 1’ x 1’ image is centered on the target (10905746).

2

3 FLUX TIME SERIES Target 10905746

3 Flux Time Series

Summary plot of quarter-stitched PDC flux time series and transits for target 10905746, marked with DV fitted epoch/period (or TPS epoch/period if fit was notsuccessful). Transits of identified planets are labeled with epoch BKJD and orbital period. For the data of quarter 1, target table 20, start BJD is 2454964 and thevertical offset is 0 ppm. For the data of quarter 2, target table 21, start BJD is 2455002 and the vertical offset is 20000 ppm. For the data of quarter 3, target table 26,start BJD is 2455093 and the vertical offset is 40000 ppm. For the data of quarter 4, target table 29, start BJD is 2455184 and the vertical offset is 60000 ppm.Open ./summary-plots/010905746-00-flux-dv-fit-01-020.fig

3

./summary-plots/010905746-00-flux-dv-fit-01-020.fig


Summary plot of quarter-stitched PDC flux time series and transits for target 10905746, marked with DV fitted epoch/period (or TPS epoch/period if fit was notsuccessful). Transits of identified planets are labeled with epoch BKJD and orbital period. For the data of quarter 5, target table 32, start BJD is 2455276 and thevertical offset is 0 ppm. For the data of quarter 6, target table 35, start BJD is 2455372 and the vertical offset is 20000 ppm. For the data of quarter 7, target table 38,start BJD is 2455463 and the vertical offset is 40000 ppm. For the data of quarter 8, target table 41, start BJD is 2455568 and the vertical offset is 60000 ppm.Open ./summary-plots/010905746-00-flux-dv-fit-05-032.fig

4



Summary plot of quarter-stitched PDC flux time series and transits for target 10905746, marked with DV fitted epoch/period (or TPS epoch/period if fit was notsuccessful). Transits of identified planets are labeled with epoch BKJD and orbital period. For the data of quarter 9, target table 44, start BJD is 2455641 and thevertical offset is 0 ppm. For the data of quarter 10, target table 47, start BJD is 2455739 and the vertical offset is 20000 ppm. For the data of quarter 11, target table50, start BJD is 2455834 and the vertical offset is 40000 ppm. For the data of quarter 12, target table 53, start BJD is 2455932 and the vertical offset is 60000 ppm.Open ./summary-plots/010905746-00-flux-dv-fit-09-044.fig

5



Summary plot of quarter-stitched PDC flux time series and transits for target 10905746, marked with DV fitted epoch/period (or TPS epoch/period if fit was notsuccessful). Transits of identified planets are labeled with epoch BKJD and orbital period. For the data of quarter 13, target table 56, start BJD is 2456015 and thevertical offset is 0 ppm. For the data of quarter 14, target table 59, start BJD is 2456107 and the vertical offset is 20000 ppm. For the data of quarter 15, target table62, start BJD is 2456206 and the vertical offset is 40000 ppm. For the data of quarter 16, target table 65, start BJD is 2456305 and the vertical offset is 60000 ppm.Open ./summary-plots/010905746-00-flux-dv-fit-13-056.fig

6



Summary plot of quarter-stitched PDC flux time series and transits for target 10905746, marked with DV fitted epoch/period (or TPS epoch/period if fit was notsuccessful). Transits of identified planets are labeled with epoch BKJD and orbital period. For the data of quarter 17, target table 68, start BJD is 2456392.Open ./summary-plots/010905746-00-flux-dv-fit-17-068.fig

7



Summary plot of raw flux time series. For the data of quarter 1, target table 20, start JD is 2454964 and the vertical offset is 0 electrons/cadence. For the data of quarter2, target table 21, start JD is 2455002 and the vertical offset is 0 electrons/cadence. For the data of quarter 3, target table 26, start JD is 2455093 and the vertical offsetis 0 electrons/cadence. For the data of quarter 4, target table 29, start JD is 2455184 and the vertical offset is 0 electrons/cadence.Open ./summary-plots/010905746-00-raw-flux-01-020.fig

8

./summary-plots/010905746-00-raw-flux-01-020.fig


Summary plot of raw flux time series. For the data of quarter 5, target table 32, start JD is 2455276 and the vertical offset is 0 electrons/cadence. For the data of quarter6, target table 35, start JD is 2455372 and the vertical offset is 0 electrons/cadence. For the data of quarter 7, target table 38, start JD is 2455463 and the vertical offsetis 0 electrons/cadence. For the data of quarter 8, target table 41, start JD is 2455568 and the vertical offset is 0 electrons/cadence.Open ./summary-plots/010905746-00-raw-flux-05-032.fig

9



Summary plot of raw flux time series. For the data of quarter 9, target table 44, start JD is 2455641 and the vertical offset is 0 electrons/cadence. For the data of quarter10, target table 47, start JD is 2455739 and the vertical offset is 0 electrons/cadence. For the data of quarter 11, target table 50, start JD is 2455834 and the verticaloffset is 0 electrons/cadence. For the data of quarter 12, target table 53, start JD is 2455932 and the vertical offset is 0 electrons/cadence.Open ./summary-plots/010905746-00-raw-flux-09-044.fig

10



Summary plot of raw flux time series. For the data of quarter 13, target table 56, start JD is 2456015 and the vertical offset is 0 electrons/cadence. For the data ofquarter 14, target table 59, start JD is 2456107 and the vertical offset is 0 electrons/cadence. For the data of quarter 15, target table 62, start JD is 2456206 and thevertical offset is 0 electrons/cadence. For the data of quarter 16, target table 65, start JD is 2456305 and the vertical offset is 0 electrons/cadence.Open ./summary-plots/010905746-00-raw-flux-13-056.fig

11



Summary plot of raw flux time series. For the data of quarter 17, target table 68, start JD is 2456392.Open ./summary-plots/010905746-00-raw-flux-17-068.fig

12


4 DASHBOARDS Target 10905746 / Planet Candidate 1

4 Dashboards

Planet Candidate 1

Mod

elF

itte

r

Stellar Radius0.4 ± 0.1 Solar units C

entroid

Test

Period = 9.9 ± 0.0 daysDepth = 1514 ± 23 ppmPlanet Radius = 1.9 ± 0.3 Earth radiiSemi-major Axis = 0.1 ± 0.0 AUEffective Stellar Flux = 5.7 ± 0.9Equilibrium Temperature = 393 ± 15 KelvinChi-squared/DoF = 0.9SNR = 77.8

Flux Weighted Motion Detection Statistic

Value = 2.36e+01Significance = 0.00%Peak RA Offset 6.90e-04 ± 2.15e-04 arcsec (3.2 σ)Peak Dec Offset = -1.87e-04 ± 1.84e-04 arcsec (-1 σ)Peak Offset Distance = 7.15e-04 ± 2.13e-04 arcsec (3.3 σ)Source RA Offset = -1.21e+00 ± 1.31e-01 arcsec (-9.2 σ)Source Dec Offset = -1.93e-01 ± 8.86e-02 arcsec (-2.2 σ)Source Offset Distance = 1.23e+00 ± 1.30e-01 arcsec (9.4 σ)

Ecl

ipsi

ng

Bin

ary

Dis

crim

inat

ion

Tes

t

Odd-Even DepthComparison Statistic

Value = 9.18e-01Significance = 33.81%

Odd-Even EpochComparison Statistic


Offsets Relative to Out of Transit Centroid

Source RA Offset = -3.49e-01 ± 7.80e-02 arcsec (-4.47 σ)Source Dec Offset = 1.81e-02 ± 9.51e-02 arcsec (0.19 σ)Source Offset Distance = 3.49e-01 ± 7.80e-02 arcsec (4.48 σ)

Offsets Relative to KIC Position

Source RA Offset = -1.32e+00 ± 7.67e-02 arcsec (-17.22 σ)Source Dec Offset = -4.64e-01 ± 8.54e-02 arcsec (-5.43 σ)Source Offset Distance = 1.40e+00 ± 7.77e-02 arcsec (18.01 σ)

Diff

erence

Image

Cen

troidO

ffsets

Shorter PeriodComparison Statistic

Value = N/ASignificance = N/A

Longer PeriodComparison Statistic

Value = 7.80e+04Significance = 100.00%

False Alarm = 0.00e+00Final Skip Count = -1Observed Number of Transits = 57Max Multiple Event Statistic = 73.4

Bootstrap

Test

Summary of model fitter results and validation test results for target 10905746, planet candidate 1. In general, green denotes that the candidate is likely a planet, whilered denotes that the candidate is unlikely to be a planet. Cyan denotes that no data is available. The color of the Model Fitter block is: green, when the SNR of thefit is greater than or equal to 10; yellow, if the SNR is greater than or equal to 7.1 but less than 10; red, if the SNR is less than 7.1 or if the fitter failed. The color ofthe Centroid Test and Eclipsing Binary Discrimination Test blocks are: green, when the significance is within 2-sigma; yellow, when the significance is between 2- and3-sigma; red when the significance is greater than 3-sigma. The color of the Difference Image Centroid Offsets block is: green, when the max offset distance sigma is lessthan or equal to 2; yellow, when the max sigma is between 2 and 3; red when the max sigma is greater than 3. The color of the Bootstrap Test block is green wheneverthe false alarm probability is less than 10−12, low enough to limit the total number of false alarms from a four year mission to less than one. If the false alarm probabilityis greater than 10−12, the color of the Bootstrap Test block is: green, when the false alarm probability is less than or equal to the CCDF of a Gaussian distribution at theobserved maximum multiple event statistic; yellow when the false alarm probability is between 1 and 2 times that of a Gaussian distribution at the max multiple eventstatistic; and red when the false alarm probability is more than 2 times that of a Gaussian distribution at the max multiple event statistic.

13

4 DASHBOARDS Target 10905746 / Planet Candidate 2

Planet Candidate 2M

od

elF

itte

r

Stellar Radius0.4 ± 0.1 Solar units C

entroid

Test

Period = 107.4 ± 0.0 daysDepth = 548 ± 100 ppmPlanet Radius = 1.0 ± 2.2 Earth radiiSemi-major Axis = 0.3 ± 0.0 AUEffective Stellar Flux = 0.2 ± 0.0Equilibrium Temperature = 177 ± 7 KelvinChi-squared/DoF = 1.4SNR = 7.7

Flux Weighted Motion Detection Statistic

Value = 2.07e+00Significance = 35.44%Peak RA Offset -7.38e-04 ± 6.36e-04 arcsec (-1.2 σ)Peak Dec Offset = 1.05e-04 ± 3.57e-04 arcsec (0.29 σ)Peak Offset Distance = 7.45e-04 ± 6.32e-04 arcsec (1.2 σ)Source RA Offset = 5.89e-01 ± 1.14e+00 arcsec (0.52 σ)Source Dec Offset = -5.08e-01 ± 5.43e-01 arcsec (-0.93 σ)Source Offset Distance = 7.77e-01 ± 9.30e-01 arcsec (0.84 σ)

Ecl

ipsi

ng

Bin

ary

Dis

crim

inat

ion

Tes

t

Odd-Even DepthComparison Statistic


Odd-Even EpochComparison Statistic


Offsets Relative to Out of Transit Centroid

Source RA Offset = 3.27e+00 ± 2.81e-01 arcsec (11.61 σ)Source Dec Offset = -5.67e-01 ± 1.36e-01 arcsec (-4.17 σ)Source Offset Distance = 3.32e+00 ± 2.78e-01 arcsec (11.92 σ)

Offsets Relative to KIC Position

Source RA Offset = 2.23e+00 ± 2.78e-01 arcsec (8.03 σ)Source Dec Offset = -1.07e+00 ± 1.89e-01 arcsec (-5.66 σ)Source Offset Distance = 2.47e+00 ± 2.64e-01 arcsec (9.39 σ)

Diff

erence

Image

Cen

troidO

ffsets

Shorter PeriodComparison Statistic


Longer PeriodComparison Statistic

Value = N/ASignificance = N/A

False Alarm = 8.86e-15Final Skip Count = -1Observed Number of Transits = 4Max Multiple Event Statistic = 11.4

Bootstrap

Test

Summary of model fitter results and validation test results for target 10905746, planet candidate 2. In general, green denotes that the candidate is likely a planet, whilered denotes that the candidate is unlikely to be a planet. Cyan denotes that no data is available. The color of the Model Fitter block is: green, when the SNR of thefit is greater than or equal to 10; yellow, if the SNR is greater than or equal to 7.1 but less than 10; red, if the SNR is less than 7.1 or if the fitter failed. The color ofthe Centroid Test and Eclipsing Binary Discrimination Test blocks are: green, when the significance is within 2-sigma; yellow, when the significance is between 2- and3-sigma; red when the significance is greater than 3-sigma. The color of the Difference Image Centroid Offsets block is: green, when the max offset distance sigma is lessthan or equal to 2; yellow, when the max sigma is between 2 and 3; red when the max sigma is greater than 3. The color of the Bootstrap Test block is green wheneverthe false alarm probability is less than 10−12, low enough to limit the total number of false alarms from a four year mission to less than one. If the false alarm probabilityis greater than 10−12, the color of the Bootstrap Test block is: green, when the false alarm probability is less than or equal to the CCDF of a Gaussian distribution at theobserved maximum multiple event statistic; yellow when the false alarm probability is between 1 and 2 times that of a Gaussian distribution at the max multiple eventstatistic; and red when the false alarm probability is more than 2 times that of a Gaussian distribution at the max multiple event statistic.

14

5 CENTROID CLOUD PLOT Target 10905746

5 Centroid Cloud Plot

KeplerId 10905746, KeplerMag 13.496 - This figure shows median detrended flux as a function of median detrended centroids for both ra and dec on the sky. Transitfeatures above the noise jitter are seen as scatter outside the central cloud. Features in the flux time series are seen in the vertical direction while features in the centroidtime series are seen in the horizontal direction. Any tilt to the out-of-cloud scatter indicates correlation between transit features in the flux and centroid time series. Theout of transit mean and standard deviation (SD) indicated in the lower left-hand corner are robust values.Open ./summary-plots/010905746-00-fluxWeighted-centroids-cloud.fig

15

./summary-plots/010905746-00-fluxWeighted-centroids-cloud.fig

6 IMAGE ARTIFACTS Target 10905746 / Planet Candidate 2

6 Image Artifacts

6.1 Planet Candidate 1

Rolling Band Contamination

Severity Level Transit Count Transit Fraction

0 50 1.001 0 0.002 0 0.003 0 0.004 0 0.00

50 1.00


Rolling Band Contamination

Severity Level Transit Count Transit Fraction

0 4 1.001 0 0.002 0 0.003 0 0.004 0 0.00

4 1.00

16

7 PIXEL LEVEL DIAGNOSTICS Target 10905746 / Planet Candidate 1

7 Pixel Level Diagnostics


Difference Image Summary Metrics

Number of Number of Number of Fraction of QualityDifference Images Metrics Good Metrics Good Metrics Threshold

8 8 8 1.0000 0.70

Difference image centroid offsets for target 10905746, planet candidate 1. Left: difference image PRF centroid offsets in RA and Dec with respect to the quarterlyout-of-transit centroids for the given target. Right: difference image PRF centroid offsets in RA and Dec with respect to the KIC coordinates of the given target. Symbolkey: green cross: quarterly centroid offsets with 1-sigma error bars in RA and Dec; magenta cross: robust weighted mean offset over all quarters with 1-sigma error barsin RA and Dec; blue circle: 3-sigma radius of confusion for weighted mean offset; red cross (where applicable): multi-quarter PRF centroid offset with 1-sigma error barsin RA and Dec; cyan circle (where applicable): 3-sigma radius of confusion for multi-quarter PRF offset; red asterisk: location of target star; blue asterisk: location ofother KIC objects in the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRT extension to the KIChave IDs between 15,000,000 and 30,000,000). A constant error term of 0.0667 arcseconds has been added in quadrature to the computed uncertainty in the RA and Deccomponents of the robust mean offset and the multi-quarter PRF offset.Open ./planet-01/difference-image/010905746-01-difference-image-centroid-offsets.fig

17

./planet-01/difference-image/010905746-01-difference-image-centroid-offsets.fig


Difference image centroid offsets for target 10905746, planet candidate 1, diplayed on UKIRT image for given target. Left: difference image PRF centroid offsets in RAand Dec with respect to the quarterly out-of-transit centroids for the given target. Right: difference image PRF centroid offsets in RA and Dec with respect to the KICcoordinates of the given target. Symbol key: green cross: quarterly centroid offsets with 1-sigma error bars in RA and Dec; magenta cross: robust weighted mean offsetover all quarters with 1-sigma error bars in RA and Dec; blue circle: 3-sigma radius of confusion for weighted mean offset; red asterisk: location of target star; blueasterisk: location of other KIC objects in the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRTextension to the KIC have IDs between 15,000,000 and 30,000,000). A constant error term of 0.0667 arcseconds has been added in quadrature to the computed uncertaintyin the RA and Dec components of the robust mean offset and the multi-quarter PRF offset.Open ./planet-01/difference-image/010905746-01-difference-image-centroid-offsets-ukirt.fig

18

./planet-01/difference-image/010905746-01-difference-image-centroid-offsets-ukirt.fig


Multi-Quarter Average PRF Fit of the Difference Images

Mean offset from the PRF fit to the out of transit imageRA Dec Units

Offset −0.3488± 7.80e− 02 0.0181± 9.51e− 02 arcsecondsOffset/σ −4.47 0.19

Offset Distance 0.3492± 7.80e− 02 arcsecondsOffset Distance/σ 4.483σ Radius 0.2340 arcseconds

Mean offset from the KIC RA and DecRA Dec Units

Offset −1.3215± 7.67e− 02 −0.4640± 8.54e− 02 arcsecondsOffset/σ −17.22 −5.43


Bootstrap Multi-Quarter PRF Fit of the Difference Images

Bootstrap multi-quarter PRF fit results for the difference images associated with this planet candidate are not available.

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Pixel correlation centroid offsets figure for this planet candidate is not available.

20

7 PIXEL LEVEL DIAGNOSTICS Target 10905746 / Planet Candidate 1 / Quarter 1 / Target Table 20

Difference image for target 10905746, planet candidate 1, quarter 1, target table 20. Upper left: difference between mean flux out-of-transit and in-transit; upper right:mean out-of-transit flux; lower left: mean in-transit flux; lower right: difference between mean flux out-of-transit and in-transit after normalizing by the uncertainty inthe difference for each pixel. The optimal aperture is outlined with a white dash-dotted line in each panel and the target mask is outlined with a solid white line. Symbolkey: x: target position from KIC RA and Dec converted to CCD coordinates via motion polynomials; *: position of nearby KIC objects converted to CCD coordinates viamotion polynomials (objects in the UKIRT extension to the KIC have IDs between 15,000,000 and 30,000,000); +: PRF-fit location of target from out-of-transit image;triangle: PRF-fit location of transit source from the difference image. CCD row and column coordinates are 0-based. Number of transits = 3; number of valid in-transitcadences = 8; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 24; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 1.00 (good).Open ./planet-01/difference-image/010905746-01-difference-image-01-020.fig

21

./planet-01/difference-image/010905746-01-difference-image-01-020.fig


The pixel correlation statistic plot is not available for target 10905746, planet candidate 1, in target table 20.

22


PRF Fit of the Difference Image

Offset from the PRF fit to the out of transit imageRow Column Units RA Dec Units

Out of Transit Image Centroid 844.28± 1.12e− 05 63.72± 1.16e− 05 pixels 18.90856564± 2.33e− 09 48.39094501± 2.40e− 08 hours/degreesDifference Image Centroid 844.31± 1.19e− 02 63.85± 1.51e− 02 pixels 18.90855606± 1.44e− 06 48.39083533± 1.56e− 05 hours/degreesOffset 0.0250± 1.19e− 02 0.1293± 1.51e− 02 pixels −0.3434± 5.17e− 02 −0.3948± 5.61e− 02 arcsecondsOffset/σ 2.10 8.58 −6.65 −7.03

Offset Distance 0.1317± 1.53e− 02 pixels 0.5233± 6.07e− 02 arcsecondsOffset Distance/σ 8.62 8.63

Offset from the KIC RA and Dec converted to pixels via motion polynomialsRow Column Units RA Dec Units

KIC Reference Centroid 844.37± 1.85e− 05 63.52± 1.78e− 05 pixels 18.90858870± 0.00e+ 00 48.39100300± 0.00e+ 00 hours/degreesDifference Image Centroid 844.31± 1.19e− 02 63.85± 1.51e− 02 pixels 18.90855606± 1.44e− 06 48.39083533± 1.56e− 05 hours/degreesOffset −0.0616± 1.19e− 02 0.3255± 1.51e− 02 pixels −1.1703± 5.17e− 02 −0.6036± 5.61e− 02 arcsecondsOffset/σ −5.18 21.60 −22.65 −10.75


PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 10905746, planet candidate 1, in target table 20.

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Out of Transit Image Centroid 839.08± 7.11e− 06 58.70± 5.99e− 06 pixels 18.90855909± 2.95e− 09 48.39084596± 3.19e− 08 hours/degreesDifference Image Centroid 839.01± 8.32e− 03 58.74± 8.75e− 03 pixels 18.90855015± 1.00e− 06 48.39088238± 8.83e− 06 hours/degreesOffset −0.0756± 8.32e− 03 0.0432± 8.75e− 03 pixels −0.3205± 3.59e− 02 0.1311± 3.18e− 02 arcsecondsOffset/σ −9.08 4.93 −8.92 4.12







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Out of Transit Image Centroid 838.93± 9.42e− 06 63.48± 7.99e− 06 pixels 18.90856144± 2.29e− 09 48.39093352± 2.41e− 08 hours/degreesDifference Image Centroid 838.95± 1.30e− 02 63.57± 1.28e− 02 pixels 18.90855510± 1.37e− 06 48.39085536± 1.49e− 05 hours/degreesOffset 0.0205± 1.30e− 02 0.0887± 1.28e− 02 pixels −0.2277± 4.90e− 02 −0.2814± 5.37e− 02 arcsecondsOffset/σ 1.57 6.92 −4.65 −5.24







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Out of Transit Image Centroid 839.10± 7.75e− 06 58.70± 6.53e− 06 pixels 18.90855945± 2.39e− 09 48.39084192± 2.48e− 08 hours/degreesDifference Image Centroid 839.06± 9.71e− 03 58.76± 9.05e− 03 pixels 18.90855205± 1.11e− 06 48.39084133± 9.59e− 06 hours/degreesOffset −0.0407± 9.71e− 03 0.0530± 9.05e− 03 pixels −0.2655± 3.99e− 02 −0.0021± 3.45e− 02 arcsecondsOffset/σ −4.19 5.85 −6.66 −0.06







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Out of Transit Image Centroid 844.35± 1.12e− 05 63.74± 1.16e− 05 pixels 18.90856238± 2.46e− 09 48.39089555± 2.56e− 08 hours/degreesDifference Image Centroid 844.27± 1.41e− 02 63.86± 1.65e− 02 pixels 18.90854626± 1.67e− 06 48.39087902± 1.72e− 05 hours/degreesOffset −0.0777± 1.41e− 02 0.1238± 1.65e− 02 pixels −0.5780± 6.00e− 02 −0.0595± 6.19e− 02 arcsecondsOffset/σ −5.50 7.51 −9.63 −0.96







44



Difference Image Summary Metrics

Number of Number of Number of Fraction of QualityDifference Images Metrics Good Metrics Good Metrics Threshold

3 3 3 1.0000 0.70

Difference image centroid offsets for target 10905746, planet candidate 2. Left: difference image PRF centroid offsets in RA and Dec with respect to the quarterlyout-of-transit centroids for the given target. Right: difference image PRF centroid offsets in RA and Dec with respect to the KIC coordinates of the given target. Symbolkey: green cross: quarterly centroid offsets with 1-sigma error bars in RA and Dec; magenta cross: robust weighted mean offset over all quarters with 1-sigma error barsin RA and Dec; blue circle: 3-sigma radius of confusion for weighted mean offset; red cross (where applicable): multi-quarter PRF centroid offset with 1-sigma error barsin RA and Dec; cyan circle (where applicable): 3-sigma radius of confusion for multi-quarter PRF offset; red asterisk: location of target star; blue asterisk: location ofother KIC objects in the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRT extension to the KIChave IDs between 15,000,000 and 30,000,000). A constant error term of 0.0667 arcseconds has been added in quadrature to the computed uncertainty in the RA and Deccomponents of the robust mean offset and the multi-quarter PRF offset.Open ./planet-02/difference-image/010905746-02-difference-image-centroid-offsets.fig

45

./planet-02/difference-image/010905746-02-difference-image-centroid-offsets.fig


Difference image centroid offsets for target 10905746, planet candidate 2, diplayed on UKIRT image for given target. Left: difference image PRF centroid offsets in RAand Dec with respect to the quarterly out-of-transit centroids for the given target. Right: difference image PRF centroid offsets in RA and Dec with respect to the KICcoordinates of the given target. Symbol key: green cross: quarterly centroid offsets with 1-sigma error bars in RA and Dec; magenta cross: robust weighted mean offsetover all quarters with 1-sigma error bars in RA and Dec; blue circle: 3-sigma radius of confusion for weighted mean offset; red asterisk: location of target star; blueasterisk: location of other KIC objects in the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRTextension to the KIC have IDs between 15,000,000 and 30,000,000). A constant error term of 0.0667 arcseconds has been added in quadrature to the computed uncertaintyin the RA and Dec components of the robust mean offset and the multi-quarter PRF offset.Open ./planet-02/difference-image/010905746-02-difference-image-centroid-offsets-ukirt.fig

46

./planet-02/difference-image/010905746-02-difference-image-centroid-offsets-ukirt.fig


Multi-Quarter Average PRF Fit of the Difference Images

Mean offset from the PRF fit to the out of transit imageRA Dec Units

Offset 3.2679± 2.81e− 01 −0.5669± 1.36e− 01 arcsecondsOffset/σ 11.61 −4.17


Mean offset from the KIC RA and DecRA Dec Units

Offset 2.2302± 2.78e− 01 −1.0718± 1.89e− 01 arcsecondsOffset/σ 8.03 −5.66


Bootstrap Multi-Quarter PRF Fit of the Difference Images

Bootstrap multi-quarter PRF fit results for the difference images associated with this planet candidate are not available.

47


Pixel correlation centroid offsets figure for this planet candidate is not available.

48


Direct image for target 10905746, planet candidate 2, quarter 1, target table 20. A difference image cannot be generated because there were no transits for this planetcandidate and target table. The mean flux over all cadences is shown in the figure. The optimal aperture is outlined with a white dash-dotted line and the target mask isoutlined with a solid white line. Symbol key: x: target position from KIC RA and Dec converted to CCD coordinates via motion polynomials; *: position of nearby KICobjects converted to CCD coordinates via motion polynomials (objects in the UKIRT extension to the KIC have IDs between 15,000,000 and 30,000,000). CCD row andcolumn coordinates are 0-based.Open ./planet-02/difference-image/010905746-02-difference-image-01-020.fig

49




50



The out of transit image centroid and difference image centroid could not be calculated for target 10905746,planet candidate 2, in target table 20.



51



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Out of Transit Image Centroid 839.13± 1.14e− 05 58.70± 9.63e− 06 pixels 18.90855876± 3.08e− 09 48.39084061± 3.25e− 08 hours/degreesDifference Image Centroid 839.75± 1.17e− 02 58.19± 2.07e− 02 pixels 18.90864550± 2.06e− 06 48.39064583± 1.63e− 05 hours/degreesOffset 0.6203± 1.17e− 02 −0.5078± 2.07e− 02 pixels 3.1106± 7.39e− 02 −0.7012± 5.86e− 02 arcsecondsOffset/σ 53.04 −24.56 42.07 −11.96



KIC Reference Centroid 839.18± 3.08e− 05 58.39± 2.17e− 05 pixels 18.90858870± 0.00e+ 00 48.39100300± 0.00e+ 00 hours/degreesDifference Image Centroid 839.75± 1.17e− 02 58.19± 2.07e− 02 pixels 18.90864550± 2.06e− 06 48.39064583± 1.63e− 05 hours/degreesOffset 0.5700± 1.17e− 02 −0.2045± 2.07e− 02 pixels 2.0369± 7.39e− 02 −1.2858± 5.86e− 02 arcsecondsOffset/σ 48.74 −9.89 27.55 −21.93




54



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57


Direct image for target 10905746, planet candidate 2, quarter 13, target table 56. A difference image cannot be generated because there were no clean transits for thisplanet candidate and target table. The mean flux over all cadences is shown in the figure. The optimal aperture is outlined with a white dash-dotted line and the targetmask is outlined with a solid white line. Symbol key: x: target position from KIC RA and Dec converted to CCD coordinates via motion polynomials; *: position ofnearby KIC objects converted to CCD coordinates via motion polynomials (objects in the UKIRT extension to the KIC have IDs between 15,000,000 and 30,000,000).CCD row and column coordinates are 0-based.Open ./planet-02/difference-image/010905746-02-difference-image-13-056.fig

58




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60


Direct image for target 10905746, planet candidate 2, quarter 14, target table 59. A difference image cannot be generated because there were no clean transits for thisplanet candidate and target table. The mean flux over all cadences is shown in the figure. The optimal aperture is outlined with a white dash-dotted line and the targetmask is outlined with a solid white line. Symbol key: x: target position from KIC RA and Dec converted to CCD coordinates via motion polynomials; *: position ofnearby KIC objects converted to CCD coordinates via motion polynomials (objects in the UKIRT extension to the KIC have IDs between 15,000,000 and 30,000,000).CCD row and column coordinates are 0-based.Open ./planet-02/difference-image/010905746-02-difference-image-14-059.fig

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8 PHASED LIGHT CURVES Target 10905746

8 Phased Light Curves

Phased unwhitened flux time series is plotted in black dots. When all transits fit completed with full or secondary convergence, the phase is determined with the fittedepoch and period; otherwise, the phase is determined with the TPS epoch and period. The values of the phased unwhitened flux time series averaged in one cadencewide bins are plotted in bigger blue dots. When all transits fit completes with full or secondary convergence, the averaged values of the phased unwhitened fitted modellight curve are plotted in red dots. Transit event markers in different colors indicate the locations of the transits of all planet candidates. The transits of the same planetcandidate are labeled with the markers of the same color, for example, blue markers for transits of plane candidate #1, red markers for transits of planet candidate #2,etc.Open ./summary-plots/010905746-01-phased-unwhitened-flux-time-series.fig

73

./summary-plots/010905746-01-phased-unwhitened-flux-time-series.fig


Phased whitened flux time series is plotted in black dots. When all transits fit completed with full or secondary convergence, the phase is determined with the fitted epochand period; otherwise, the phase is determined with the TPS epoch and period. The values of the phased whitened flux time series averaged in one cadence wide bins areplotted in bigger blue dots. When all transits fit completes with full or secondary convergence, the averaged values of the phased whitened fitted model light curve areplotted in red dots. Transit event markers in different colors indicate the locations of the transits of all planet candidates. The transits of the same planet candidate arelabeled with the markers of the same color, for example, blue markers for transits of plane candidate #1, red markers for transits of planet candidate #2, etc.Open ./summary-plots/010905746-01-phased-whitened-flux-time-series.fig

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./summary-plots/010905746-01-phased-whitened-flux-time-series.fig


Phased unwhitened flux time series by quarter for target 10905746, planet candidate 1. Period = 9.8787 days; transit epoch = 138.4094 BKJD.Open ./summary-plots/010905746-01-phased-unwhitened-flux-time-series-by-quarter.fig

75

./summary-plots/010905746-01-phased-unwhitened-flux-time-series-by-quarter.fig


Phased unwhitened flux time series by quarter for target 10905746, planet candidate 2. Period = 107.423 days; transit epoch = 218.5006 BKJD.Open ./summary-plots/010905746-02-phased-unwhitened-flux-time-series-by-quarter.fig

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./summary-plots/010905746-02-phased-unwhitened-flux-time-series-by-quarter.fig

9 PLANET CANDIDATE 1 Target 10905746 / Planet Candidate 1

9 Planet Candidate 1

9.1 Model Fitter: All Transits

Model Characteristic Name

Transit Model mandel-agol geometric transit modelLimb Darkening Model claret nonlinear limb darkening model 2011

TCE Parameter Value Units

Trial Transit Pulse Duration 2.0 hoursTransit Epoch 54970.9174454 MJDOrbital Period 9.8785598 daysMaximum SES 22.2Maximum MES 73.4Robust Statistic 67.0Chi Square Goodness of Fit Statistic (DoF) 773.7 (223)Chi Square2 Statistic (DoF) 336.0 (434.9)Threshold for Desired PFA

DoF: Degrees of Freedom

Parameter Value Uncertainty Units

SNR 77.8Orbital Period 9.8786660 6.8584e-06 daysTransit Epoch 138.4094056 6.9988e-04 BKJDImpact Parameter 0.8342 7.3914e-02Planet Radius to Star Radius Ratio 0.0404171 1.9509e-03Semi-major Axis to Star Radius Ratio 22.6567 4.5397e+00Planet Radius 1.8612 2.6282e-01 Earth radiiSemi-major Axis 0.0692 6.7821e-03 AUEffective Stellar Flux 5.6544 8.5780e-01 GoldilocksEquilibrium Temperature 393 1.4913e+01 KelvinTransit Depth 1514 2.2944e+01 ppmTransit Duration 2.0725 9.7262e-02 hoursTransit Ingress Time 0.2459 1.1268e-01 hoursEccentricity 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 degreesModel Chi Square Statistic (DoF) 1040.5 (1145.2)Model Chi Square Goodness of Fit Statistic (DoF) 167.8 (291)Model Chi Square2 Statistic (DoF) 58.5 (56)


77


PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. For the data of Quarter-01/TargetTableId-020, start BJD is 2454964 andthe vertical offset is 0. For the data of Quarter-02/TargetTableId-021, start BJD is 2455002 and the vertical offset is 0.02. For the data of Quarter-03/TargetTableId-026,start BJD is 2455093 and the vertical offset is 0.04. For the data of Quarter-04/TargetTableId-029, start BJD is 2455184 and the vertical offset is 0.06. Transit eventmarkers indicate the location of transits of the given planet candidate. All transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-01-020.fig

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./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-01-020.fig



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PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. For the data of Quarter-17/TargetTableId-068, start BJD is 2456392. Transitevent markers indicate the location of transits of the given planet candidate. All transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-17-068.fig

82



PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain, zoomed on last 5 transits in the unit of work. If # of transits is smaller than5, all transits are shown.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-zoomed.fig

PDC Flux time series of all transits for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. Data has been high-pass filtered via a median filter operatingat a specified multiple of the transit duration, folded per the fitted period and epoch, and zoomed to the location of the model transit.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-filtered-zoomed.fig

83

./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-zoomed.fig

./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-unwhitened-filtered-zoomed.fig


Folded flux time series for KeplerId 10905746, Planet candidate 1 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. Theblue dots represent the averaged values of the folded flux time series; the red dots represent the averaged values of the folded model light curve of the all transits fit; thegreen dots are the averaged folded fit residuals, vertically offset for clarity. All transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-whitened.fig

Folded flux time series for KeplerId 10905746, Planet candidate 1 in the whitened domain, zoomed on the transit. The flux data whose robust weights are larger/smallerthan 0.1 are plotted in dark green/cyan dots, respectively. Values are averaged into 1 cadence wide bins. The blue dots represent the averaged values of the folded fluxtime series; the red dots represent the averaged values of the fitted model light curve of the all transits fit; the green dots are the averaged folded fit residuals, verticallyoffset for clarity. Magenta dots are the averaged values of the folded flux time series, with a phase shift of 0.5 relative to the blue dots, vertically offset for clarity. Alltransits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-whitened-zoomed.fig

84

./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-whitened.fig

./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-whitened-zoomed.fig


9.2 Model Fitter: Reduced Parameter Fit Results

Impact SNR Model Planet Radius Uncert Semi-major Axis Uncert Transit Uncert Transit UncertParameter Chi Square to Star Radius to Star Radius Depth Duration

(ppm) (hours)

0.10 83.0 4335.1 0.0350973 3.1973e-04 40.3029 3.9017e-01 1497 2.7108e+01 1.9294 1.8581e-020.30 81.3 4256.1 0.0351998 3.3026e-04 38.5614 3.7692e-01 1477 2.7547e+01 1.9393 1.8851e-020.50 82.9 3972.9 0.0362307 3.3748e-04 35.0493 3.3895e-01 1497 2.7714e+01 1.9547 1.8787e-020.70 83.3 3419.0 0.0379031 3.5601e-04 28.9785 2.8617e-01 1500 2.7981e+01 1.9965 1.9544e-020.90 83.7 2531.5 0.0428191 4.2959e-04 17.9026 1.9330e-01 1526 3.0271e+01 2.2236 2.3631e-02

Highlighted row is the best reduced-parameter model fit.

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Model chi squares of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 1. The fit result with the minimum chi square is marked witha dashed line in the plot.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-chi-square.fig

Ratios of planet radius to star radius of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 1. The fit result with the minimum chisquare is marked with a dashed line in the plot.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-rp-over-rstar.fig

Ratios of semimajor axis to star radius of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 1. The fit result with the minimum chisquare is marked with a dashed line in the plot.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-a-over-rstar.fig

86

./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-chi-square.fig

./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-rp-over-rstar.fig

./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-01-reduced-fits-a-over-rstar.fig


9.3 Model Fitter: Trapezoidal Fit Results


Transit Model trapezoidal modelLimb Darkening Model





SNR 153.3Orbital Period 9.8785598 daysTransit Epoch 138.4218824 BKJDTransit Depth 1375 ppmTransit Duration 1.9884 hoursTransit Ingress Time 0.3268 hoursModel Chi Square Statistic (DoF) 38789.9 (1739)


87


Folded detrended flux time series for KeplerId 10905746, Planet candidate 1 and folded trapezoidal model light curve.Open ./planet-01/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-01-all-trapezoidal.fig

Zoomed folded detrended flux time series for KeplerId 10905746, Planet candidate 1 and folded trapezoidal model light curve.Open ./planet-01/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-01-all-trapezoidal-zoomed.fig

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./planet-01/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-01-all-trapezoidal.fig

./planet-01/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-01-all-trapezoidal-zoomed.fig


9.4 Validation Tests

The Centroid Test and Eclipsing Binary Discrimination Test are chi-squared hypothesis tests. For these tests, a significance of 100% favors a planet, while 0% indicatesan unlikely planet.

9.4.1 Weak Secondary Test

Result Value Uncertainty Units Statistic in Sigmas Significance (%)

Orbital Period 9.8786 daysTransit Duration 2 hoursMaximum MES 73.4Secondary Phase 4.0452 daysSecondary MES 4.4Minimum Phase -1.925 daysMinimum MES -3.6Median MES 0.0MAD MES 0.92632Robust Statistic 3.5Secondary Depth 73.5 1.9328e+01 ppmGeometric Albedo 55.9 1.7079e+01 3.2128 0.07Planet Effective Temperature 1662 1.2224e+02 Kelvin 10.3039 0.00

9.4.2 Flux-Weighted Centroid Test

Result Value Uncertainty Units Value in Sigmas Significance (%)

Stellar Magnitude 13.4960 0.0000e+00Motion Detection Statistic 2.3624e+01 0.00Peak RA Offset 6.8967e-04 2.1543e-04 arcseconds 3.2014Peak Dec Offset -1.8704e-04 1.8385e-04 arcseconds -1.0174Peak Offset Distance 7.1458e-04 2.1341e-04 arcseconds 3.3484Source RA Offset -1.2114e+00 1.3099e-01 arcseconds -9.2480Source Dec Offset -1.9315e-01 8.8612e-02 arcseconds -2.1797Source Offset Distance 1.2267e+00 1.3011e-01 arcseconds 9.4284Source RA 18.90855492 3.6531e-06 hoursSource Dec 48.39094935 2.4615e-05 degrees

Peak offsets are relative to the out-of-transit centroid. Source offsets are relative to the KIC target location.

89


9.4.3 Eclipsing Binary Discrimination Test

Result Value Value in Sigmas Significance (%)

Odd Even Transit Depth Comparison Statistic 9.1771e-01 0.9580 33.81Odd Even Transit Epoch Comparison Statistic 2.0255e-04 0.0142 98.86Longer Period Comparison Statistic 7.8000e+04 279.2850 100.00

9.4.4 Bootstrap Test

Result Value

False Alarm Probability 0.0000e+00Bootstrap Threshold for Desired PFA 8.7MES Mean 0.16MES Standard Deviation 1.20Observed Number of Transits 57

9.4.5 Ghost Diagnostic Test

Result Value Significance (%)

Maximum MES 73.4SNR 77.8Core Aperture Statistic 2.7012e+01 100.00Halo Aperture Statistic 1.2939e+01 100.00Ratio of Core/Halo Aperture Statistics 2.0877e+00

90


9.4.6 Validation Test Figures

The primary event has been set to zero and both the max and min of the resulting MES vs. Phase are marked with a red star. The best matched pulse duration inhours is 2. The maximum secondary MES and corresponding phase are 4.4213 and 4.0452 days respectively. The minimum secondary MES and corresponding phase are-3.6427 and -1.925 days respectively.Open ./planet-01/report-summary/010905746-01-weak-secondary-diagnostic.fig

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./planet-01/report-summary/010905746-01-weak-secondary-diagnostic.fig


Flux weighted centroid test source offsets for target 10905746, planet candidate 1. Symbol key: magenta cross: flux weighted centroid test source offsets with 1-sigmaerror bars in RA and Dec; blue circle: 3-sigma radius of confusion for source offset; red asterisk: location of target star; blue asterisk: location of other KIC objectsin the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRT extension to the KIC have IDs between15,000,000 and 30,000,000). Figure on right is displayed on UKIRT image for given target.Open ./planet-01/centroid-test-results/010905746-01-centroid-test-source-offsets.fig

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./planet-01/centroid-test-results/010905746-01-centroid-test-source-offsets.fig


KeplerId 10905746, KeplerMag 13.50 - FOLDED FLUX AND CENTROIDS - This figure shows detrended flux and centroid data folded at the fitted orbital period andcentered on the fitted transit over a few fitted transit durations. The top panel shows the change in corrected flux for this target, normalized to the median out of transitvalue, median detrended with the median out of transit value removed. The bottom two panels show the corresponding change in the centroid in right ascension (RA)and declination (DEC) angles on the sky. The centroids are detrended against ancillary data and have the mean out-of-transit value removed. The scaled transit modelfit to the target flux is shown on the centroid plots in red. The peak fitted offset from the out-of-transit centroid is indicated by the solid black horizontal line. One sigmaerror bars are indicated with dashed black horizontal lines. In-transit data points for any other planets identified for this target have been gapped. The out-of-transitmean and standard deviation (SD) indicated in the lower left-hand corner are robust estimates.Open ./planet-01/centroid-test-results/010905746-01-folded-transit-fit-fluxWeighted-centroids.fig

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./planet-01/centroid-test-results/010905746-01-folded-transit-fit-fluxWeighted-centroids.fig


KeplerId 10905746, KeplerMag 13.50 - UNFOLDED FLUX AND CENTROIDS - This figure shows detrended flux and centroid data over the full time range of the dataset. The top panel shows the change in corrected flux for this target, normalized to the median out of transit value, median detrended with the median out of transitvalue removed. The bottom two panels show the corresponding change in the centroid in right ascension (RA) and declination (DEC) angles on the sky. The centroidsare detrended against ancillary data and have the mean out-of-transit value removed. The scaled transit model fit to the target flux is shown on the centroid plots in red.The peak fitted offset from the out of transit centroid is indicated by the solid black horizontal line. One sigma error bars are indicated with dashed black horizontal lines.Red circles and vertical lines mark the fitted transit centers. In-transit data points for any other planets identified for this target have been gapped. The out-of-transitmean and standard deviation (SD) indicated in the lower left-hand corner are robust estimates.Open ./planet-01/centroid-test-results/010905746-01-transit-fit-fluxWeighted-centroids-01.fig

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./planet-01/centroid-test-results/010905746-01-transit-fit-fluxWeighted-centroids-01.fig



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Bootstrap results for target 10905746, planet 1. Cumulative sum of the probabilities (derived from the histogram of counts) from upper tail to the search transit threshold;false alarm probability is indicated by the star. The Gaussian equivalent threshold for this false alarm probability is Inf. The threshold on this distribution that achievesthe same false alarm rate as a 7.1 sigma threshold on a Gaussian distribution is 8.6898.Open ./planet-01/bootstrap-results/010905746-01-bootstrap-false-alarm.fig

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./planet-01/bootstrap-results/010905746-01-bootstrap-false-alarm.fig


10 Planet Candidate 2

10.1 Model Fitter: All Transits


Transit Model mandel-agol geometric transit modelLimb Darkening Model claret nonlinear limb darkening model 2011





SNR 7.7Orbital Period 107.4230427 4.6819e-03 daysTransit Epoch 218.5005923 4.8035e-02 BKJDImpact Parameter 0.4518 1.6904e+01Planet Radius to Star Radius Ratio 0.0217174 4.7885e-02Semi-major Axis to Star Radius Ratio 92.5951 8.8434e+02Planet Radius 1.0001 2.2091e+00 Earth radiiSemi-major Axis 0.3396 3.3289e-02 AUEffective Stellar Flux 0.2347 3.5606e-02 GoldilocksEquilibrium Temperature 177 6.7312e+00 KelvinTransit Depth 548 9.9726e+01 ppmTransit Duration 8.1221 4.2051e+00 hoursTransit Ingress Time 0.2158 4.6090e+00 hoursEccentricity 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 degreesModel Chi Square Statistic (DoF) 445.8 (311.6)Model Chi Square Goodness of Fit Statistic (DoF) 60.5 (69)Model Chi Square2 Statistic (DoF) 24.9 (3)


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PDC Flux time series for KeplerId 10905746, Planet candidate 2 in the unwhitened domain. For the data of Quarter-17/TargetTableId-068, start BJD is 2456392. Transitevent markers indicate the location of transits of the given planet candidate. All transits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-unwhitened-17-068.fig

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PDC Flux time series for KeplerId 10905746, Planet candidate 2 in the unwhitened domain, zoomed on last 5 transits in the unit of work. If # of transits is smaller than5, all transits are shown.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-unwhitened-zoomed.fig

PDC Flux time series of all transits for KeplerId 10905746, Planet candidate 2 in the unwhitened domain. Data has been high-pass filtered via a median filter operatingat a specified multiple of the transit duration, folded per the fitted period and epoch, and zoomed to the location of the model transit.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-unwhitened-filtered-zoomed.fig

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./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-unwhitened-zoomed.fig

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Folded flux time series for KeplerId 10905746, Planet candidate 2 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. Theblue dots represent the averaged values of the folded flux time series; the red dots represent the averaged values of the folded model light curve of the all transits fit; thegreen dots are the averaged folded fit residuals, vertically offset for clarity. All transits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-whitened.fig

Folded flux time series for KeplerId 10905746, Planet candidate 2 in the whitened domain, zoomed on the transit. The flux data whose robust weights are larger/smallerthan 0.1 are plotted in dark green/cyan dots, respectively. Values are averaged into 1 cadence wide bins. The blue dots represent the averaged values of the folded fluxtime series; the red dots represent the averaged values of the fitted model light curve of the all transits fit; the green dots are the averaged folded fit residuals, verticallyoffset for clarity. Magenta dots are the averaged values of the folded flux time series, with a phase shift of 0.5 relative to the blue dots, vertically offset for clarity. Alltransits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-whitened-zoomed.fig

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./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-whitened.fig

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10.2 Model Fitter: Reduced Parameter Fit Results

Impact SNR Model Planet Radius Uncert Semi-major Axis Uncert Transit Uncert Transit UncertParameter Chi Square to Star Radius to Star Radius Depth Duration

(ppm) (hours)

0.10 16.7 3533.0 0.0315083 2.7834e-03 66.9632 1.9760e+00 1213 2.1324e+02 12.5806 3.7543e-010.30 12.7 3482.6 0.0268122 3.1286e-03 85.5897 4.2132e+00 862 2.0010e+02 9.4155 4.6780e-010.50 16.3 3751.3 0.0317757 3.1064e-03 63.5865 2.1625e+00 1158 2.2533e+02 11.6485 3.9616e-010.70 10.4 3678.3 0.0255406 4.4235e-03 96.3692 1.0807e+01 684 2.3645e+02 6.3825 7.1168e-010.90 9.5 3717.7 0.0279678 6.5508e-03 59.6374 9.6072e+00 656 3.0801e+02 6.8352 1.1566e+00

Highlighted row is the best reduced-parameter model fit.

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Model chi squares of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 2. The fit result with the minimum chi square is marked witha dashed line in the plot.Open ./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-chi-square.fig

Ratios of planet radius to star radius of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 2. The fit result with the minimum chisquare is marked with a dashed line in the plot.Open ./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-rp-over-rstar.fig

Ratios of semimajor axis to star radius of reduced parameter fits vs. impact parameter for KeplerId 10905746, Planet candidate 2. The fit result with the minimum chisquare is marked with a dashed line in the plot.Open ./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-a-over-rstar.fig

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./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-chi-square.fig

./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-rp-over-rstar.fig

./planet-02/planet-search-and-model-fitting-results/reduced-parameter-fits/010905746-02-reduced-fits-a-over-rstar.fig


10.3 Model Fitter: Trapezoidal Fit Results


Transit Model trapezoidal modelLimb Darkening Model





SNR 42.1Orbital Period 107.4120013 daysTransit Epoch 218.7595768 BKJDTransit Depth 852 ppmTransit Duration 6.4051 hoursTransit Ingress Time 0.5739 hoursModel Chi Square Statistic (DoF) 35268.1 (350)


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Folded detrended flux time series for KeplerId 10905746, Planet candidate 2 and folded trapezoidal model light curve.Open ./planet-02/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-02-all-trapezoidal.fig

Zoomed folded detrended flux time series for KeplerId 10905746, Planet candidate 2 and folded trapezoidal model light curve.Open ./planet-02/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-02-all-trapezoidal-zoomed.fig

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./planet-02/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-02-all-trapezoidal.fig

./planet-02/planet-search-and-model-fitting-results/trapezoidal-model-fit/010905746-02-all-trapezoidal-zoomed.fig


10.4 Validation Tests

The Centroid Test and Eclipsing Binary Discrimination Test are chi-squared hypothesis tests. For these tests, a significance of 100% favors a planet, while 0% indicatesan unlikely planet.

10.4.1 Weak Secondary Test

Result Value Uncertainty Units Statistic in Sigmas Significance (%)

Orbital Period 107.412 daysTransit Duration 6 hoursMaximum MES 11.4Secondary Phase -24.9221 daysSecondary MES 5.7Minimum Phase 15.332 daysMinimum MES -5.7Median MES 0.0MAD MES 0.7813Robust Statistic 3.4Secondary Depth 254.0 8.4816e+01 ppmGeometric Albedo 16111.2 7.1278e+04 0.2260 41.06Planet Effective Temperature 3092 3.4188e+03 Kelvin 0.8524 19.70

10.4.2 Flux-Weighted Centroid Test

Result Value Uncertainty Units Value in Sigmas Significance (%)

Stellar Magnitude 13.4960 0.0000e+00Motion Detection Statistic 2.0745e+00 35.44Peak RA Offset -7.3785e-04 6.3613e-04 arcseconds -1.1599Peak Dec Offset 1.0483e-04 3.5711e-04 arcseconds 0.2936Peak Offset Distance 7.4526e-04 6.3180e-04 arcseconds 1.1796Source RA Offset 5.8873e-01 1.1352e+00 arcseconds 0.5186Source Dec Offset -5.0764e-01 5.4314e-01 arcseconds -0.9346Source Offset Distance 7.7737e-01 9.2999e-01 arcseconds 0.8359Source RA 18.90860512 3.1657e-05 hoursSource Dec 48.39086199 1.5087e-04 degrees

Peak offsets are relative to the out-of-transit centroid. Source offsets are relative to the KIC target location.

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10.4.3 Eclipsing Binary Discrimination Test

Result Value Value in Sigmas Significance (%)

Odd Even Transit Depth Comparison Statistic 2.6003e+00 1.6126 10.68Odd Even Transit Epoch Comparison Statistic 1.8773e-03 0.0433 96.54Shorter Period Comparison Statistic 7.8000e+04 279.2850 100.00

10.4.4 Bootstrap Test

Result Value

False Alarm Probability 8.8599e-15Bootstrap Threshold for Desired PFA 10.5MES Mean -1.79MES Standard Deviation 1.72Observed Number of Transits 4

10.4.5 Ghost Diagnostic Test

Result Value Significance (%)

Maximum MES 11.4SNR 7.7Core Aperture Statistic 3.1603e+00 99.92Halo Aperture Statistic 1.6346e+00 94.89Ratio of Core/Halo Aperture Statistics 1.9333e+00

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10.4.6 Validation Test Figures

The primary event has been set to zero and both the max and min of the resulting MES vs. Phase are marked with a red star. The best matched pulse duration inhours is 6. The maximum secondary MES and corresponding phase are 5.7446 and -24.9221 days respectively. The minimum secondary MES and corresponding phaseare -5.7158 and 15.332 days respectively.Open ./planet-02/report-summary/010905746-02-weak-secondary-diagnostic.fig

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./planet-02/report-summary/010905746-02-weak-secondary-diagnostic.fig


Flux weighted centroid test source offsets for target 10905746, planet candidate 2. Symbol key: magenta cross: flux weighted centroid test source offsets with 1-sigmaerror bars in RA and Dec; blue circle: 3-sigma radius of confusion for source offset; red asterisk: location of target star; blue asterisk: location of other KIC objectsin the neighborhood. KIC ID and magnitude are noted in the text associated with each marked object (objects in the UKIRT extension to the KIC have IDs between15,000,000 and 30,000,000). Figure on right is displayed on UKIRT image for given target.Open ./planet-02/centroid-test-results/010905746-02-centroid-test-source-offsets.fig

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./planet-02/centroid-test-results/010905746-02-centroid-test-source-offsets.fig


KeplerId 10905746, KeplerMag 13.50 - FOLDED FLUX AND CENTROIDS - This figure shows detrended flux and centroid data folded at the fitted orbital period andcentered on the fitted transit over a few fitted transit durations. The top panel shows the change in corrected flux for this target, normalized to the median out of transitvalue, median detrended with the median out of transit value removed. The bottom two panels show the corresponding change in the centroid in right ascension (RA)and declination (DEC) angles on the sky. The centroids are detrended against ancillary data and have the mean out-of-transit value removed. The scaled transit modelfit to the target flux is shown on the centroid plots in red. The peak fitted offset from the out-of-transit centroid is indicated by the solid black horizontal line. One sigmaerror bars are indicated with dashed black horizontal lines. In-transit data points for any other planets identified for this target have been gapped. The out-of-transitmean and standard deviation (SD) indicated in the lower left-hand corner are robust estimates.Open ./planet-02/centroid-test-results/010905746-02-folded-transit-fit-fluxWeighted-centroids.fig

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Bootstrap results for target 10905746, planet 2. Cumulative sum of the probabilities (derived from the histogram of counts) from upper tail to the search transit threshold;false alarm probability is indicated by the star. The Gaussian equivalent threshold for this false alarm probability is 7.6662. The threshold on this distribution thatachieves the same false alarm rate as a 7.1 sigma threshold on a Gaussian distribution is 10.5066.Open ./planet-02/bootstrap-results/010905746-02-bootstrap-false-alarm.fig

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./planet-02/bootstrap-results/010905746-02-bootstrap-false-alarm.fig

APPENDIX A: PLANET CANDIDATE 1 Target 10905746 / Planet Candidate 1

Appendix A Planet Candidate 1

A.1 Model Fitter: All Transits

Robust weights distribution for KeplerId 10905746, Planet candidate 1. Top plot: all data points. Middle plot: all data points, folded per the fitted period and epoch.Bottom plot: all data points, folded and zoomed.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-robust-weights.fig

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./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-robust-weights.fig


Fit residuals distribution for KeplerId 10905746, Planet candidate 1. Only the valid data points used to constrain the fit are shown here. A Gaussian fit to the histogramis shown in red.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-histo-used.fig

Fit residuals distribution for KeplerId 10905746, Planet candidate 1. Top plot: all valid data. Bottom plot: valid data not used to constrain fit (due to distance from atransit). Gaussian fits to the histograms are shown in red.Open ./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-histo-all-and-unused.fig

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./planet-01/planet-search-and-model-fitting-results/all-transits-fit/010905746-01-all-histo-used.fig

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A.2 Model Fitter: Odd & Even Transits

Parameter Odd Transits Odd Transits Even Transits Even Transits Units Difference‖Uncertainty‖Value Uncertainty Value Uncertainty

SNR 58.1 51.3Orbital Period 9.8786759 1.0032e-05 9.8786642 9.3107e-06 days 8.5551e-01Transit Epoch 138.4083984 1.0172e-03 148.2882976 9.6746e-04 BKJD 8.7848e-01Impact Parameter 0.8623 6.0743e-02 0.7623 2.9356e-01 3.3350e-01Planet Radius to Star Radius Ratio 0.0415092 2.0634e-03 0.0386611 4.8196e-03 5.4325e-01Semi-major Axis to Star Radius Ratio 20.9088 4.2167e+00 26.5396 1.4037e+01 3.8417e-01Planet Radius 1.9115 2.7087e-01 1.7803 3.2415e-01 Earth radii 3.1048e-01Semi-major Axis 0.0692 6.7821e-03 0.0692 6.7821e-03 AU 5.7003e-06Effective Stellar Flux 5.6544 8.5780e-01 5.6544 8.5780e-01 Goldilocks 7.3664e-06Equilibrium Temperature 393 1.4913e+01 393 1.4913e+01 Kelvin 7.3664e-06Transit Depth 1536 3.1619e+01 1491 3.4695e+01 ppm 9.5797e-01Transit Duration 2.1105 1.1733e-01 2.0072 1.8204e-01 hours 4.7685e-01Transit Ingress Time 0.2992 1.3941e-01 0.1704 2.0379e-01 hours 5.2153e-01Eccentricity 0.0000 0.0000e+00 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 0.0000 0.0000e+00 degreesModel Chi Square Statistic (DoF) 1011.0 (1140.2) 1011.0 (1140.2)


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PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. For the data of Quarter-01/TargetTableId-020, start BJD is 2454964 andthe vertical offset is 0. For the data of Quarter-02/TargetTableId-021, start BJD is 2455002 and the vertical offset is 0.02. For the data of Quarter-03/TargetTableId-026,start BJD is 2455093 and the vertical offset is 0.04. For the data of Quarter-04/TargetTableId-029, start BJD is 2455184 and the vertical offset is 0.06. Transit eventmarkers indicate the location of transits of the given planet candidate. Odd-even transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-unwhitened-01-020.fig

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PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. For the data of Quarter-17/TargetTableId-068, start BJD is 2456392. Transitevent markers indicate the location of transits of the given planet candidate. Odd-even transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-unwhitened-17-068.fig

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PDC Flux time series for KeplerId 10905746, Planet candidate 1 in the unwhitened domain, zoomed on last 5 transits in the unit of work. If # of transits is smaller than5, all transits are shown.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-unwhitened-zoomed.fig

PDC Flux time series of odd/even transits for KeplerId 10905746, Planet candidate 1 in the unwhitened domain. Data has been high-pass filtered via a median filteroperating at a specified multiple of the transit duration, folded per the fitted period and epoch, and zoomed to the location of the model transit.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-unwhitened-filtered-zoomed.fig

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Folded flux time series for KeplerId 10905746, Planet candidate 1 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. Theblue dots represent the averaged values of the folded flux time series; the red dots represent the averaged values of the folded model light curve of the odd/even transitsfit; the green dots are the averaged folded fit residuals, vertically offset for clarity. Odd-even transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-whitened.fig

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./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-whitened.fig


Folded flux time series for KeplerId 10905746, Planet candidate 1 in the whitened domain, zoomed on the transit. The flux data whose robust weights are larger/smallerthan 0.1 are plotted in dark green/cyan dots, respectively. Values are averaged into 1 cadence wide bins. The blue dots represent the averaged values of the folded fluxtime series; the red dots represent the averaged values of the fitted model light curve of the odd/even transits fit; the green dots are the averaged folded fit residuals,vertically offset for clarity. Magenta dots are the averaged values of the folded flux time series, with a phase shift of 0.5 relative to the blue dots, vertically offset forclarity. Odd-even transits fit completed with full convergence.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-whitened-zoomed.fig

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./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-whitened-zoomed.fig


Robust weights distribution for KeplerId 10905746, Planet candidate 1. Top plot: all data points. Middle plot: all data points, folded per the fitted period and epoch.Bottom plot: all data points, folded and zoomed.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-robust-weights.fig

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./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-robust-weights.fig


Fit residuals distribution for KeplerId 10905746, Planet candidate 1. Only the valid data points used to constrain the fit are shown here. A Gaussian fit to the histogramis shown in red.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-histo-used.fig

Fit residuals distribution for KeplerId 10905746, Planet candidate 1. Top plot: all valid data. Bottom plot: valid data not used to constrain fit (due to distance from atransit). Gaussian fits to the histograms are shown in red.Open ./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-histo-all-and-unused.fig

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./planet-01/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-01-odd-even-histo-used.fig

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A.3 Eclipsing Binary Discrimination Test

Top-left: Diagnostic plot of Odd/Even Transit Depth Test for keplerId 10905746, planet 1. A significance level close to 1/0 favors a transiting planet/an eclipsing binary.Top-right: Diagnostic plot of Odd/Even Transit Epoch Test for keplerId 10905746, planet 1. A significance level close to 1/0 favors a transiting planet/an eclipsing binary.Bottom-right: Diagnostic plot of Orbital Period Test for keplerId 10905746. Orbital periods of planet 1 and the planet with longer period are compared. A significancelevel close to 1/0 favors a transiting planet/an eclipsing binary.Open ./planet-01/binary-discrimination-test-results/010905746-01-eclipsing-binary-discrimination-tests.fig

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./planet-01/binary-discrimination-test-results/010905746-01-eclipsing-binary-discrimination-tests.fig

APPENDIX B: PLANET CANDIDATE 2 Target 10905746 / Planet Candidate 2

Appendix B Planet Candidate 2

B.1 Model Fitter: All Transits

Robust weights distribution for KeplerId 10905746, Planet candidate 2. Top plot: all data points. Middle plot: all data points, folded per the fitted period and epoch.Bottom plot: all data points, folded and zoomed.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-robust-weights.fig

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./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-robust-weights.fig


Fit residuals distribution for KeplerId 10905746, Planet candidate 2. Only the valid data points used to constrain the fit are shown here. A Gaussian fit to the histogramis shown in red.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-histo-used.fig

Fit residuals distribution for KeplerId 10905746, Planet candidate 2. Top plot: all valid data. Bottom plot: valid data not used to constrain fit (due to distance from atransit). Gaussian fits to the histograms are shown in red.Open ./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-histo-all-and-unused.fig

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./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-histo-used.fig

./planet-02/planet-search-and-model-fitting-results/all-transits-fit/010905746-02-all-histo-all-and-unused.fig


B.2 Model Fitter: Odd & Even Transits

Parameter Odd Transits Odd Transits Even Transits Even Transits Units Difference‖Uncertainty‖Value Uncertainty Value Uncertainty

SNR 8.3 4.9Orbital Period 107.4188122 4.7106e-03 107.4242205 1.9525e-02 days 2.6927e-01Transit Epoch 218.5363195 4.5363e-02 325.9747430 1.8889e-01 BKJD 7.9176e-02Impact Parameter 0.7658 6.2867e-01 0.6116 1.0501e+01 1.4657e-02Planet Radius to Star Radius Ratio 0.0299720 9.0853e-03 0.0208431 4.8970e-02 1.8329e-01Semi-major Axis to Star Radius Ratio 60.8743 7.1341e+01 76.4671 7.7610e+02 2.0007e-02Planet Radius 1.3802 4.5671e-01 0.9598 2.2587e+00 Earth radii 1.8243e-01Semi-major Axis 0.3396 3.3288e-02 0.3396 3.3289e-02 AU 2.4212e-04Effective Stellar Flux 0.2347 3.5608e-02 0.2347 3.5605e-02 Goldilocks 3.1289e-04Equilibrium Temperature 177 6.7313e+00 177 6.7312e+00 Kelvin 3.1289e-04Transit Depth 899 1.9423e+02 478 1.7414e+02 ppm 1.6126e+00Transit Duration 9.2855 1.6961e+00 8.7722 5.4196e+00 hours 9.0403e-02Transit Ingress Time 0.6294 1.6568e+00 0.2828 6.4407e+00 hours 5.2109e-02Eccentricity 0.0000 0.0000e+00 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 0.0000 0.0000e+00 degreesModel Chi Square Statistic (DoF) 414.2 (306.5) 414.2 (306.5)


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PDC Flux time series for KeplerId 10905746, Planet candidate 2 in the unwhitened domain. For the data of Quarter-17/TargetTableId-068, start BJD is 2456392. Transitevent markers indicate the location of transits of the given planet candidate. Odd-even transits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-unwhitened-17-068.fig

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PDC Flux time series for KeplerId 10905746, Planet candidate 2 in the unwhitened domain, zoomed on last 5 transits in the unit of work. If # of transits is smaller than5, all transits are shown.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-unwhitened-zoomed.fig

PDC Flux time series of odd/even transits for KeplerId 10905746, Planet candidate 2 in the unwhitened domain. Data has been high-pass filtered via a median filteroperating at a specified multiple of the transit duration, folded per the fitted period and epoch, and zoomed to the location of the model transit.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-unwhitened-filtered-zoomed.fig

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./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-unwhitened-zoomed.fig

./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-unwhitened-filtered-zoomed.fig


Folded flux time series for KeplerId 10905746, Planet candidate 2 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. Theblue dots represent the averaged values of the folded flux time series; the red dots represent the averaged values of the folded model light curve of the odd/even transitsfit; the green dots are the averaged folded fit residuals, vertically offset for clarity. Odd-even transits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-whitened.fig

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./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-whitened.fig


Folded flux time series for KeplerId 10905746, Planet candidate 2 in the whitened domain, zoomed on the transit. The flux data whose robust weights are larger/smallerthan 0.1 are plotted in dark green/cyan dots, respectively. Values are averaged into 1 cadence wide bins. The blue dots represent the averaged values of the folded fluxtime series; the red dots represent the averaged values of the fitted model light curve of the odd/even transits fit; the green dots are the averaged folded fit residuals,vertically offset for clarity. Magenta dots are the averaged values of the folded flux time series, with a phase shift of 0.5 relative to the blue dots, vertically offset forclarity. Odd-even transits fit completed with full convergence.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-whitened-zoomed.fig

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./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-whitened-zoomed.fig


Robust weights distribution for KeplerId 10905746, Planet candidate 2. Top plot: all data points. Middle plot: all data points, folded per the fitted period and epoch.Bottom plot: all data points, folded and zoomed.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-robust-weights.fig

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./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-robust-weights.fig


Fit residuals distribution for KeplerId 10905746, Planet candidate 2. Only the valid data points used to constrain the fit are shown here. A Gaussian fit to the histogramis shown in red.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-histo-used.fig

Fit residuals distribution for KeplerId 10905746, Planet candidate 2. Top plot: all valid data. Bottom plot: valid data not used to constrain fit (due to distance from atransit). Gaussian fits to the histograms are shown in red.Open ./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-histo-all-and-unused.fig

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./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-histo-used.fig

./planet-02/planet-search-and-model-fitting-results/odd-even-transits-fit/010905746-02-odd-even-histo-all-and-unused.fig


B.3 Eclipsing Binary Discrimination Test

Top-left: Diagnostic plot of Odd/Even Transit Depth Test for keplerId 10905746, planet 2. A significance level close to 1/0 favors a transiting planet/an eclipsing binary.Top-right: Diagnostic plot of Odd/Even Transit Epoch Test for keplerId 10905746, planet 2. A significance level close to 1/0 favors a transiting planet/an eclipsing binary.Bottom-left: Diagnostic plot of Orbital Period Test for keplerId 10905746. Orbital periods of planet 2 and the planet with shorter period are compared. A significancelevel close to 1/0 favors a transiting planet/an eclipsing binary.Open ./planet-02/binary-discrimination-test-results/010905746-02-eclipsing-binary-discrimination-tests.fig

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./planet-02/binary-discrimination-test-results/010905746-02-eclipsing-binary-discrimination-tests.fig

APPENDIX C: SINGLE EVENT STATISTICS FROM RESIDUAL FLUX Target 10905746

Appendix C Single Event Statistics from Residual Flux

No figures named 010905746-00-residual-ses-*.fig are available.

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APPENDIX D: ALERTS Target 10905746

Appendix D Alerts

Time Severity Message

57419.2658 warning Difference image cannot be generated because there were no transits for this planet candidate and target table (target=1, kep-lerId=10905746, planet=2, targetTable=20, component=generateDvDifferenceImages)


57419.2664 warning Difference image cannot be generated because there were no clean transits for this planet candidate and target table (target=1, kep-lerId=10905746, planet=2, targetTable=56, component=generateDvDifferenceImages)

57419.2666 warning Difference image cannot be generated because there were no clean transits for this planet candidate and target table (target=1, kep-lerId=10905746, planet=2, targetTable=59, component=generateDvDifferenceImages)


57419.2670 warning Multi-quarter PRF fitting and offset analysis will not be performed because model fit SNR is above specified threshold (target=1,keplerId=10905746, planet=1, component=generateDvDifferenceImages)

57419.2670 warning Multi-quarter PRF fitting and offset analysis will not be performed because model fit SNR is above specified threshold (target=1,keplerId=10905746, planet=2, component=generateDvDifferenceImages)

57419.2688 warning No centroid data available. Centroid test results set to default values for all planets. (target=1, keplerId=10905746, component=Centroidtest prf)

57419.2841 warning Pixel correlation test is disabled (target=1, keplerId=10905746, component=Pixel correlation test)

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data validation (dv) reportexoplanetarchive.ipac.caltech.edu/data/keplerdata/010/... ·...

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