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Data Validation (DV) Report for Kepler ID 9836149 Quarters 1 - 16 16-Aug-2013 06:09:34 Z

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Page 1: for Kepler ID 9836149 Quarters 1 - 16

Data Validation (DV) Reportfor Kepler ID 9836149

Quarters 1 - 16

16-Aug-2013 06:09:34 Z

Page 2: for Kepler ID 9836149 Quarters 1 - 16

Contents

1 Summary 1

2 UKIRT Image 3

3 Flux Time Series 4

4 Dashboards 16

5 Centroid Cloud Plot 17

6 Pixel Level Diagnostics 186.1 Planet Candidate 1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18

7 Phased Light Curves 69

8 Planet Candidate 1 718.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 718.2 Model Fitter: Reduced Parameter Fit Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 788.3 Validation Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 80

8.3.1 Weak Secondary Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 808.3.2 Flux-Weighted Centroid Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 808.3.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 808.3.4 Bootstrap Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 80

Appendices 100

A Planet Candidate 1 100A.1 Model Fitter: All Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100A.2 Model Fitter: Odd & Even Transits . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102A.3 Eclipsing Binary Discrimination Test . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112

B Single Event Statistics from Residual Flux 113

C Alerts 114

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Page 3: for Kepler ID 9836149 Quarters 1 - 16

1 SUMMARY Target 9836149

1 Summary

Target Properties Value Uncertainty Units Provenance

Sky Group 39RA 19.59877070 0 hours KICDec 46.68775000 0 degrees KICMagnitude 15.2 0 KICRadius 0.93 0.223 Solar radii DSEPEffective Temperature 5964 131 Kelvin SPE47log(g) 4.48 0.196 cm/sec2 SPE47[Fe/H] -0.22 0.16 Solar metallicity SPE47Number of Planet Candidates 1Categories GO LC,

MERGED,CLUSTER,PLANETARY,INCLUDE

Prior Pipeline Instance ID -External TCE Model -Software Revision svn+ssh://murzim/repo/soc/tags/release/9.1.2@52755Date Report Generated 16-Aug-2013 06:09:34 Z

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

1 20 18/3 0.9297 0.8146 0.3768 0.5436 -0.1976 -0.00972 21 14/3 0.9448 0.7637 0.3768 0.5436 -0.1976 -0.00973 26 8/3 0.9151 0.8655 0.3768 0.5436 -0.1976 -0.00974 29 12/3 0.8861 0.8089 0.3768 0.5436 -0.1976 -0.00975 32 18/3 0.9277 0.8141 0.3768 0.5436 -0.1976 -0.00976 35 14/3 0.9455 0.7515 0.3768 0.5436 -0.1976 -0.00977 38 8/3 0.9156 0.8665 0.3768 0.5436 -0.1976 -0.00978 41 12/3 0.8862 0.8085 0.3768 0.5436 -0.1976 -0.00979 44 18/3 0.9261 0.8143 0.3768 0.5436 -0.1976 -0.0097

10 47 14/3 0.9455 0.7549 0.3768 0.5436 -0.1976 -0.009711 50 8/3 0.9158 0.8666 0.3768 0.5436 -0.1976 -0.009712 53 12/3 0.8866 0.8088 0.3768 0.5436 -0.1976 -0.009713 56 18/3 0.9256 0.8144 0.3768 0.5436 -0.1976 -0.009714 59 14/3 0.9455 0.7547 0.3768 0.5436 -0.1976 -0.009715 62 8/3 0.9155 0.8664 0.3768 0.5436 -0.1976 -0.009716 65 12/3 0.9021 0.7585 0.3768 0.5436 -0.1976 -0.0097

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Page 4: for Kepler ID 9836149 Quarters 1 - 16

1 SUMMARY Target 9836149

Planet TPS Period DV Period Period Ratio TPS Epoch DV Epoch Semi-major Radius False SuspectedCandidate (days) (days) (DV) (JD-2454833) (BKJD) Axis (AU) (Earth radii) Alarm EB

1 17.8 17.8 1.0 134.5 134.5 0.1 3.2 N/A false

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Page 5: for Kepler ID 9836149 Quarters 1 - 16

2 UKIRT IMAGE Target 9836149

2 UKIRT Image

UKIRT Wide Field Camera (WFCAM) infra-red J-band image. The 1’ x 1’ image is centered on the target (9836149).

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Page 6: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

3 Flux Time Series

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with TPS epoch/period. Transits of identified planets are labeledwith epoch KJD and orbital period determined by TPS. For the data of quarter 1, target table 20, start JD is 2454964 and the vertical offset is 0 ppm. For the data ofquarter 2, target table 21, start JD is 2455002 and the vertical offset is 50000 ppm. For the data of quarter 3, target table 26, start JD is 2455093 and the vertical offsetis 100000 ppm. For the data of quarter 4, target table 29, start JD is 2455184 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-tps-01-020.fig

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Page 7: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with TPS epoch/period. Transits of identified planets are labeledwith epoch KJD and orbital period determined by TPS. For the data of quarter 5, target table 32, start JD is 2455276 and the vertical offset is 0 ppm. For the data ofquarter 6, target table 35, start JD is 2455372 and the vertical offset is 50000 ppm. For the data of quarter 7, target table 38, start JD is 2455463 and the vertical offsetis 100000 ppm. For the data of quarter 8, target table 41, start JD is 2455568 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-tps-05-032.fig

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Page 8: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with TPS epoch/period. Transits of identified planets are labeledwith epoch KJD and orbital period determined by TPS. For the data of quarter 9, target table 44, start JD is 2455641 and the vertical offset is 0 ppm. For the data ofquarter 10, target table 47, start JD is 2455739 and the vertical offset is 50000 ppm. For the data of quarter 11, target table 50, start JD is 2455834 and the verticaloffset is 100000 ppm. For the data of quarter 12, target table 53, start JD is 2455932 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-tps-09-044.fig

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Page 9: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with TPS epoch/period. Transits of identified planets are labeledwith epoch KJD and orbital period determined by TPS. For the data of quarter 13, target table 56, start JD is 2456015 and the vertical offset is 0 ppm. For the dataof quarter 14, target table 59, start JD is 2456107 and the vertical offset is 50000 ppm. For the data of quarter 15, target table 62, start JD is 2456206 and the verticaloffset is 100000 ppm. For the data of quarter 16, target table 65, start JD is 2456305 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-tps-13-056.fig

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Page 10: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with DV fitted epoch/period. Transits of identified planets arelabeled with epoch BKJD and orbital period determined by DV transit fitter. For the data of quarter 1, target table 20, start BJD is 2454964 and the vertical offset is0 ppm. For the data of quarter 2, target table 21, start BJD is 2455002 and the vertical offset is 50000 ppm. For the data of quarter 3, target table 26, start BJD is2455093 and the vertical offset is 100000 ppm. For the data of quarter 4, target table 29, start BJD is 2455184 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-dv-fit-01-020.fig

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Page 11: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with DV fitted epoch/period. Transits of identified planets arelabeled with epoch BKJD and orbital period determined by DV transit fitter. For the data of quarter 5, target table 32, start BJD is 2455276 and the vertical offset is0 ppm. For the data of quarter 6, target table 35, start BJD is 2455372 and the vertical offset is 50000 ppm. For the data of quarter 7, target table 38, start BJD is2455463 and the vertical offset is 100000 ppm. For the data of quarter 8, target table 41, start BJD is 2455568 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-dv-fit-05-032.fig

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Page 12: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with DV fitted epoch/period. Transits of identified planets arelabeled with epoch BKJD and orbital period determined by DV transit fitter. For the data of quarter 9, target table 44, start BJD is 2455641 and the vertical offset is0 ppm. For the data of quarter 10, target table 47, start BJD is 2455739 and the vertical offset is 50000 ppm. For the data of quarter 11, target table 50, start BJD is2455834 and the vertical offset is 100000 ppm. For the data of quarter 12, target table 53, start BJD is 2455932 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-dv-fit-09-044.fig

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Page 13: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

Summary plot of PDC flux time series (with harmonic content) and transits for target 9836149, marked with DV fitted epoch/period. Transits of identified planets arelabeled with epoch BKJD and orbital period determined by DV transit fitter. For the data of quarter 13, target table 56, start BJD is 2456015 and the vertical offset is0 ppm. For the data of quarter 14, target table 59, start BJD is 2456107 and the vertical offset is 50000 ppm. For the data of quarter 15, target table 62, start BJD is2456206 and the vertical offset is 100000 ppm. For the data of quarter 16, target table 65, start BJD is 2456305 and the vertical offset is 150000 ppm.Open ./summary-plots/009836149-00-flux-with-harmonics-dv-fit-13-056.fig

No figures named 009836149-00-flux-harmonics-free-tps-*.fig are available.

No figures named 009836149-00-flux-harmonics-free-dv-fit-*.fig are available.

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Page 14: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

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/009836149-00-raw-flux-01-020.fig

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Page 15: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

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/009836149-00-raw-flux-05-032.fig

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Page 16: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

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/009836149-00-raw-flux-09-044.fig

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Page 17: for Kepler ID 9836149 Quarters 1 - 16

3 FLUX TIME SERIES Target 9836149

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/009836149-00-raw-flux-13-056.fig

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4 DASHBOARDS Target 9836149 / Planet Candidate 1

4 Dashboards

Planet Candidate 1

Mod

elF

itte

r

Stellar Radius0.9 ± 0.0 Solar units C

entroid

Test

Period = 17.8 ± 0.0 daysDepth = 907 ± 27 ppmPlanet Radius = 3.2 ± 0.2 Earth radiiSemi-major Axis = 0.1 ± 0.0 AUEquilibrium Temperature = 699 ± 85 KelvinChi-squared/DoF = 0.8SNR = 33.6

Flux Weighted Motion Detection Statistic

Value = 3.34e+00Significance = 18.80%Peak RA Offset 2.07e-04 ± 2.80e-04 arcsec (0.74 σ)Peak Dec Offset = 2.22e-04 ± 3.19e-04 arcsec (0.7 σ)Peak Offset Distance = 3.04e-04 ± 3.02e-04 arcsec (1 σ)Source RA Offset = -1.87e-01 ± 3.01e-01 arcsec (-0.62 σ)Source Dec Offset = -1.06e-01 ± 3.37e-01 arcsec (-0.32 σ)Source Offset Distance = 2.15e-01 ± 3.11e-01 arcsec (0.69 σ)

Ecl

ipsi

ng

Bin

ary

Dis

crim

inat

ion

Tes

t

Odd-Even DepthComparison Statistic

Value = 5.91e-02Significance = 80.79%

Odd-Even EpochComparison Statistic

Value = 6.84e-04Significance = 97.91%

Offsets Relative to Out of Transit Centroid

Source RA Offset = 3.05e-02 ± 1.23e-01 arcsec (0.25 σ)Source Dec Offset = -2.00e-01 ± 1.42e-01 arcsec (-1.42 σ)Source Offset Distance = 2.03e-01 ± 1.41e-01 arcsec (1.44 σ)

Offsets Relative to KIC Position

Source RA Offset = 6.21e-03 ± 1.14e-01 arcsec (0.05 σ)Source Dec Offset = -1.59e-01 ± 1.39e-01 arcsec (-1.14 σ)Source Offset Distance = 1.59e-01 ± 1.40e-01 arcsec (1.14 σ)

Diff

erence

Image

Cen

troidO

ffsets

Shorter PeriodComparison Statistic

Value = N/ASignificance = N/A

Longer PeriodComparison Statistic

Value = N/ASignificance = N/A

False Alarm = N/AFinal Skip Count = N/AObserved Number of Transits = 73Max Multiple Event Statistic = 3.05e+01

Bootstrap

Test

Summary of model fitter results and validation test results for target 9836149, 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.

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5 CENTROID CLOUD PLOT Target 9836149

5 Centroid Cloud Plot

KeplerId 9836149, KeplerMag 15.2 - This figure shows median detrended flux as a function of median detrended centroids for both ra and dec on the sky. Transit featuresabove 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 centroid timeseries 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. The outof transit mean and standard deviation (SD) indicated in the lower left-hand corner are robust values.Open ./summary-plots/009836149-00-fluxWeighted-centroids-cloud.fig

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1

6 Pixel Level Diagnostics

6.1 Planet Candidate 1

Difference Image Summary Metrics

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

16 16 16 1.0000 0.70

Difference image centroid offsets for target 9836149, 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/009836149-01-difference-image-centroid-offsets.fig

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Page 21: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1

Multi-Quarter Average PRF Fit of the Difference Images

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

Offset 0.0305± 1.23e− 01 −0.2004± 1.42e− 01 arcsecondsOffset/σ 0.25 −1.42

Offset Distance 0.2027± 1.41e− 01 arcsecondsOffset Distance/σ 1.443σ Radius 0.4235 arcseconds

Mean offset from the KIC RA and DecRA Dec Units

Offset 0.0062± 1.14e− 01 −0.1591± 1.39e− 01 arcsecondsOffset/σ 0.05 −1.14

Offset Distance 0.1593± 1.40e− 01 arcsecondsOffset Distance/σ 1.143σ Radius 0.4196 arcseconds

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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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1

Pixel correlation centroid offsets figure cannot be generated because there are no valid centroid offsets.

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 1 / Target Table 20

Difference image for target 9836149, 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 = 2; number of valid in-transitcadences = 10; number of in-transit cadence gaps = 1; number of valid out-of-transit cadences = 29; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.95 (good).Open ./planet-01/difference-image/009836149-01-difference-image-01-020.fig

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 1 / Target Table 20

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 20.

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 1 / Target Table 20

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 845.14± 5.02e− 05 538.04± 3.73e− 05 pixels 19.59877181± 5.08e− 09 46.68778232± 4.69e− 08 hours/degreesDifference Image Centroid 845.31± 6.09e− 02 538.19± 5.23e− 02 pixels 19.59876551± 6.51e− 06 46.68754134± 5.84e− 05 hours/degreesOffset 0.1616± 6.09e− 02 0.1578± 5.23e− 02 pixels −0.2336± 2.41e− 01 −0.8675± 2.10e− 01 arcsecondsOffset/σ 2.65 3.02 −0.97 −4.13

Offset Distance 0.2259± 5.49e− 02 pixels 0.8984± 2.18e− 01 arcsecondsOffset Distance/σ 4.11 4.12

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

KIC Reference Centroid 845.17± 7.97e− 06 538.06± 8.08e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 845.31± 6.09e− 02 538.19± 5.23e− 02 pixels 19.59876551± 6.51e− 06 46.68754134± 5.84e− 05 hours/degreesOffset 0.1378± 6.09e− 02 0.1379± 5.23e− 02 pixels −0.1923± 2.41e− 01 −0.7512± 2.10e− 01 arcsecondsOffset/σ 2.26 2.64 −0.80 −3.57

Offset Distance 0.1949± 5.48e− 02 pixels 0.7754± 2.18e− 01 arcsecondsOffset Distance/σ 3.56 3.56

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 20.

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 2 / Target Table 21

Difference image for target 9836149, planet candidate 1, quarter 2, target table 21. 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 = 4; number of valid in-transitcadences = 21; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 56; number of out-of-transit cadence gaps = 1. Difference image qualitymetric = 0.97 (good).Open ./planet-01/difference-image/009836149-01-difference-image-02-021.fig

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 2 / Target Table 21

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 21.

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 2 / Target Table 21

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 840.14± 3.85e− 05 538.24± 2.54e− 05 pixels 19.59877137± 3.99e− 09 46.68777771± 3.30e− 08 hours/degreesDifference Image Centroid 840.12± 7.54e− 02 537.95± 7.72e− 02 pixels 19.59875735± 7.94e− 06 46.68806445± 8.70e− 05 hours/degreesOffset −0.0198± 7.54e− 02 −0.2899± 7.72e− 02 pixels −0.5195± 2.94e− 01 1.0322± 3.13e− 01 arcsecondsOffset/σ −0.26 −3.76 −1.77 3.29

Offset Distance 0.2905± 7.75e− 02 pixels 1.1556± 3.08e− 01 arcsecondsOffset Distance/σ 3.75 3.75

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

KIC Reference Centroid 840.16± 7.34e− 06 538.26± 9.29e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.12± 7.54e− 02 537.95± 7.72e− 02 pixels 19.59875735± 7.94e− 06 46.68806445± 8.70e− 05 hours/degreesOffset −0.0380± 7.54e− 02 −0.3083± 7.72e− 02 pixels −0.4946± 2.94e− 01 1.1320± 3.13e− 01 arcsecondsOffset/σ −0.50 −4.00 −1.68 3.61

Offset Distance 0.3106± 7.77e− 02 pixels 1.2354± 3.09e− 01 arcsecondsOffset Distance/σ 4.00 4.00

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 21.

26

Page 29: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 3 / Target Table 26

Difference image for target 9836149, planet candidate 1, quarter 3, target table 26. 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 = 5; number of valid in-transitcadences = 26; number of in-transit cadence gaps = 2; number of valid out-of-transit cadences = 73; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.95 (good).Open ./planet-01/difference-image/009836149-01-difference-image-03-026.fig

27

Page 30: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 3 / Target Table 26

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 26.

28

Page 31: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 3 / Target Table 26

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 840.42± 1.99e− 05 534.11± 2.84e− 05 pixels 19.59876837± 2.60e− 09 46.68775061± 3.09e− 08 hours/degreesDifference Image Centroid 840.36± 5.83e− 02 534.11± 8.37e− 02 pixels 19.59877337± 6.99e− 06 46.68778769± 8.68e− 05 hours/degreesOffset −0.0572± 5.83e− 02 −0.0052± 8.37e− 02 pixels 0.1854± 2.59e− 01 0.1335± 3.13e− 01 arcsecondsOffset/σ −0.98 −0.06 0.72 0.43

Offset Distance 0.0574± 5.87e− 02 pixels 0.2285± 2.34e− 01 arcsecondsOffset Distance/σ 0.98 0.98

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

KIC Reference Centroid 840.40± 8.77e− 06 534.12± 9.33e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.36± 5.83e− 02 534.11± 8.37e− 02 pixels 19.59877337± 6.99e− 06 46.68778769± 8.68e− 05 hours/degreesOffset −0.0388± 5.83e− 02 −0.0167± 8.37e− 02 pixels 0.0990± 2.59e− 01 0.1357± 3.13e− 01 arcsecondsOffset/σ −0.67 −0.20 0.38 0.43

Offset Distance 0.0422± 6.36e− 02 pixels 0.1680± 2.53e− 01 arcsecondsOffset Distance/σ 0.66 0.66

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 26.

29

Page 32: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 4 / Target Table 29

Difference image for target 9836149, planet candidate 1, quarter 4, target table 29. 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 = 15; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 44; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.89 (good).Open ./planet-01/difference-image/009836149-01-difference-image-04-029.fig

30

Page 33: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 4 / Target Table 29

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 29.

31

Page 34: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 4 / Target Table 29

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 844.03± 2.94e− 05 534.60± 2.52e− 05 pixels 19.59876931± 3.21e− 09 46.68775488± 2.99e− 08 hours/degreesDifference Image Centroid 844.09± 6.42e− 02 534.64± 6.53e− 02 pixels 19.59876634± 6.97e− 06 46.68768364± 7.15e− 05 hours/degreesOffset 0.0566± 6.42e− 02 0.0414± 6.53e− 02 pixels −0.1099± 2.58e− 01 −0.2565± 2.58e− 01 arcsecondsOffset/σ 0.88 0.63 −0.43 −1.00

Offset Distance 0.0701± 6.43e− 02 pixels 0.2790± 2.56e− 01 arcsecondsOffset Distance/σ 1.09 1.09

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

KIC Reference Centroid 844.03± 8.84e− 06 534.61± 6.72e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 844.09± 6.42e− 02 534.64± 6.53e− 02 pixels 19.59876634± 6.97e− 06 46.68768364± 7.15e− 05 hours/degreesOffset 0.0655± 6.42e− 02 0.0310± 6.53e− 02 pixels −0.1614± 2.58e− 01 −0.2389± 2.58e− 01 arcsecondsOffset/σ 1.02 0.48 −0.63 −0.93

Offset Distance 0.0725± 6.42e− 02 pixels 0.2883± 2.55e− 01 arcsecondsOffset Distance/σ 1.13 1.13

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 29.

32

Page 35: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 5 / Target Table 32

Difference image for target 9836149, planet candidate 1, quarter 5, target table 32. 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 = 5; number of valid in-transitcadences = 27; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 72; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.94 (good).Open ./planet-01/difference-image/009836149-01-difference-image-05-032.fig

33

Page 36: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 5 / Target Table 32

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 32.

34

Page 37: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 5 / Target Table 32

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 845.10± 3.21e− 05 538.03± 2.43e− 05 pixels 19.59877136± 3.32e− 09 46.68778309± 3.11e− 08 hours/degreesDifference Image Centroid 845.25± 6.17e− 02 538.12± 5.72e− 02 pixels 19.59876184± 6.59e− 06 46.68761318± 6.38e− 05 hours/degreesOffset 0.1546± 6.17e− 02 0.0872± 5.72e− 02 pixels −0.3528± 2.44e− 01 −0.6117± 2.30e− 01 arcsecondsOffset/σ 2.51 1.52 −1.45 −2.66

Offset Distance 0.1775± 6.01e− 02 pixels 0.7061± 2.39e− 01 arcsecondsOffset Distance/σ 2.95 2.95

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

KIC Reference Centroid 845.12± 8.67e− 06 538.05± 6.99e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 845.25± 6.17e− 02 538.12± 5.72e− 02 pixels 19.59876184± 6.59e− 06 46.68761318± 6.38e− 05 hours/degreesOffset 0.1341± 6.17e− 02 0.0645± 5.72e− 02 pixels −0.3283± 2.44e− 01 −0.4925± 2.30e− 01 arcsecondsOffset/σ 2.17 1.13 −1.35 −2.14

Offset Distance 0.1488± 6.04e− 02 pixels 0.5919± 2.40e− 01 arcsecondsOffset Distance/σ 2.46 2.46

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 32.

35

Page 38: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 6 / Target Table 35

Difference image for target 9836149, planet candidate 1, quarter 6, target table 35. 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 = 5; number of valid in-transitcadences = 28; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 71; number of out-of-transit cadence gaps = 1. Difference image qualitymetric = 0.96 (good).Open ./planet-01/difference-image/009836149-01-difference-image-06-035.fig

36

Page 39: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 6 / Target Table 35

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 35.

37

Page 40: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 6 / Target Table 35

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 840.09± 3.41e− 05 538.21± 2.40e− 05 pixels 19.59876979± 3.58e− 09 46.68776029± 3.11e− 08 hours/degreesDifference Image Centroid 839.99± 7.33e− 02 538.27± 5.53e− 02 pixels 19.59878272± 7.41e− 06 46.68776085± 6.71e− 05 hours/degreesOffset −0.1038± 7.33e− 02 0.0609± 5.53e− 02 pixels 0.4787± 2.75e− 01 0.0020± 2.42e− 01 arcsecondsOffset/σ −1.42 1.10 1.74 0.01

Offset Distance 0.1203± 6.88e− 02 pixels 0.4787± 2.75e− 01 arcsecondsOffset Distance/σ 1.75 1.74

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

KIC Reference Centroid 840.09± 8.99e− 06 538.22± 8.80e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 839.99± 7.33e− 02 538.27± 5.53e− 02 pixels 19.59878272± 7.41e− 06 46.68776085± 6.71e− 05 hours/degreesOffset −0.1013± 7.33e− 02 0.0485± 5.53e− 02 pixels 0.4451± 2.75e− 01 0.0391± 2.42e− 01 arcsecondsOffset/σ −1.38 0.88 1.62 0.16

Offset Distance 0.1123± 7.00e− 02 pixels 0.4468± 2.79e− 01 arcsecondsOffset Distance/σ 1.60 1.60

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 35.

38

Page 41: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 7 / Target Table 38

Difference image for target 9836149, planet candidate 1, quarter 7, target table 38. 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 = 5; number of valid in-transitcadences = 26; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 72; number of out-of-transit cadence gaps = 1. Difference image qualitymetric = 0.95 (good).Open ./planet-01/difference-image/009836149-01-difference-image-07-038.fig

39

Page 42: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 7 / Target Table 38

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 38.

40

Page 43: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 7 / Target Table 38

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 840.40± 2.01e− 05 534.12± 2.83e− 05 pixels 19.59876855± 2.62e− 09 46.68775245± 3.10e− 08 hours/degreesDifference Image Centroid 840.33± 4.96e− 02 534.28± 6.84e− 02 pixels 19.59878412± 5.90e− 06 46.68763600± 7.11e− 05 hours/degreesOffset −0.0711± 4.96e− 02 0.1646± 6.84e− 02 pixels 0.5769± 2.18e− 01 −0.4192± 2.56e− 01 arcsecondsOffset/σ −1.43 2.41 2.64 −1.64

Offset Distance 0.1793± 6.56e− 02 pixels 0.7131± 2.61e− 01 arcsecondsOffset Distance/σ 2.73 2.73

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

KIC Reference Centroid 840.38± 9.07e− 06 534.13± 9.55e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.33± 4.96e− 02 534.28± 6.84e− 02 pixels 19.59878412± 5.90e− 06 46.68763600± 7.11e− 05 hours/degreesOffset −0.0550± 4.96e− 02 0.1525± 6.84e− 02 pixels 0.4972± 2.18e− 01 −0.4104± 2.56e− 01 arcsecondsOffset/σ −1.11 2.23 2.28 −1.60

Offset Distance 0.1621± 6.63e− 02 pixels 0.6447± 2.64e− 01 arcsecondsOffset Distance/σ 2.44 2.44

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 38.

41

Page 44: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 8 / Target Table 41

Difference image for target 9836149, planet candidate 1, quarter 8, target table 41. 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 = 4; number of valid in-transitcadences = 21; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 56; number of out-of-transit cadence gaps = 2. Difference image qualitymetric = 0.97 (good).Open ./planet-01/difference-image/009836149-01-difference-image-08-041.fig

42

Page 45: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 8 / Target Table 41

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 41.

43

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 8 / Target Table 41

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 844.00± 2.90e− 05 534.59± 2.24e− 05 pixels 19.59876986± 3.14e− 09 46.68775801± 2.73e− 08 hours/degreesDifference Image Centroid 844.04± 5.83e− 02 534.54± 5.11e− 02 pixels 19.59876353± 6.14e− 06 46.68778217± 5.80e− 05 hours/degreesOffset 0.0395± 5.83e− 02 −0.0488± 5.11e− 02 pixels −0.2343± 2.28e− 01 0.0870± 2.09e− 01 arcsecondsOffset/σ 0.68 −0.96 −1.03 0.42

Offset Distance 0.0628± 5.46e− 02 pixels 0.2499± 2.18e− 01 arcsecondsOffset Distance/σ 1.15 1.15

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

KIC Reference Centroid 844.00± 8.83e− 06 534.60± 6.65e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 844.04± 5.83e− 02 534.54± 5.11e− 02 pixels 19.59876353± 6.14e− 06 46.68778217± 5.80e− 05 hours/degreesOffset 0.0426± 5.83e− 02 −0.0591± 5.11e− 02 pixels −0.2655± 2.28e− 01 0.1158± 2.09e− 01 arcsecondsOffset/σ 0.73 −1.16 −1.17 0.55

Offset Distance 0.0728± 5.42e− 02 pixels 0.2897± 2.17e− 01 arcsecondsOffset Distance/σ 1.34 1.34

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 41.

44

Page 47: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 9 / Target Table 44

Difference image for target 9836149, planet candidate 1, quarter 9, target table 44. 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 = 6; number of valid in-transitcadences = 32; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 84; number of out-of-transit cadence gaps = 2. Difference image qualitymetric = 0.98 (good).Open ./planet-01/difference-image/009836149-01-difference-image-09-044.fig

45

Page 48: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 9 / Target Table 44

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 44.

46

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 9 / Target Table 44

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 845.11± 3.07e− 05 538.04± 2.21e− 05 pixels 19.59877151± 3.19e− 09 46.68778221± 2.85e− 08 hours/degreesDifference Image Centroid 845.11± 6.58e− 02 538.04± 4.85e− 02 pixels 19.59877193± 6.58e− 06 46.68779063± 6.00e− 05 hours/degreesOffset −0.0072± 6.58e− 02 −0.0046± 4.85e− 02 pixels 0.0155± 2.44e− 01 0.0303± 2.16e− 01 arcsecondsOffset/σ −0.11 −0.09 0.06 0.14

Offset Distance 0.0086± 6.22e− 02 pixels 0.0340± 2.47e− 01 arcsecondsOffset Distance/σ 0.14 0.14

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

KIC Reference Centroid 845.14± 8.40e− 06 538.06± 6.52e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 845.11± 6.58e− 02 538.04± 4.85e− 02 pixels 19.59877193± 6.58e− 06 46.68779063± 6.00e− 05 hours/degreesOffset −0.0286± 6.58e− 02 −0.0258± 4.85e− 02 pixels 0.0457± 2.44e− 01 0.1463± 2.16e− 01 arcsecondsOffset/σ −0.43 −0.53 0.19 0.68

Offset Distance 0.0385± 5.97e− 02 pixels 0.1532± 2.37e− 01 arcsecondsOffset Distance/σ 0.65 0.65

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 44.

47

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 10 / Target Table 47

Difference image for target 9836149, planet candidate 1, quarter 10, target table 47. 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 = 5; number of valid in-transitcadences = 28; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 70; number of out-of-transit cadence gaps = 2. Difference image qualitymetric = 0.97 (good).Open ./planet-01/difference-image/009836149-01-difference-image-10-047.fig

48

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 10 / Target Table 47

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 47.

49

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 10 / Target Table 47

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 840.08± 3.44e− 05 538.21± 2.44e− 05 pixels 19.59877160± 3.57e− 09 46.68777152± 3.14e− 08 hours/degreesDifference Image Centroid 840.19± 8.26e− 02 538.24± 5.15e− 02 pixels 19.59876296± 8.55e− 06 46.68768870± 6.23e− 05 hours/degreesOffset 0.1074± 8.26e− 02 0.0235± 5.15e− 02 pixels −0.3202± 3.17e− 01 −0.2981± 2.24e− 01 arcsecondsOffset/σ 1.30 0.46 −1.01 −1.33

Offset Distance 0.1100± 7.99e− 02 pixels 0.4375± 3.18e− 01 arcsecondsOffset Distance/σ 1.38 1.38

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

KIC Reference Centroid 840.10± 7.01e− 06 538.23± 8.97e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.19± 8.26e− 02 538.24± 5.15e− 02 pixels 19.59876296± 8.55e− 06 46.68768870± 6.23e− 05 hours/degreesOffset 0.0903± 8.26e− 02 0.0110± 5.15e− 02 pixels −0.2869± 3.17e− 01 −0.2207± 2.24e− 01 arcsecondsOffset/σ 1.09 0.21 −0.91 −0.98

Offset Distance 0.0910± 8.13e− 02 pixels 0.3619± 3.24e− 01 arcsecondsOffset Distance/σ 1.12 1.12

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 47.

50

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 11 / Target Table 50

Difference image for target 9836149, planet candidate 1, quarter 11, target table 50. 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 = 5; number of valid in-transitcadences = 24; number of in-transit cadence gaps = 1; number of valid out-of-transit cadences = 72; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.99 (good).Open ./planet-01/difference-image/009836149-01-difference-image-11-050.fig

51

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 11 / Target Table 50

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 50.

52

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 11 / Target Table 50

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 840.40± 2.03e− 05 534.12± 2.87e− 05 pixels 19.59876811± 2.65e− 09 46.68774373± 3.14e− 08 hours/degreesDifference Image Centroid 840.40± 4.93e− 02 534.09± 6.81e− 02 pixels 19.59876664± 5.96e− 06 46.68777468± 6.99e− 05 hours/degreesOffset −0.0025± 4.93e− 02 −0.0311± 6.81e− 02 pixels −0.0544± 2.21e− 01 0.1114± 2.52e− 01 arcsecondsOffset/σ −0.05 −0.46 −0.25 0.44

Offset Distance 0.0312± 6.79e− 02 pixels 0.1240± 2.70e− 01 arcsecondsOffset Distance/σ 0.46 0.46

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

KIC Reference Centroid 840.37± 9.08e− 06 534.13± 9.61e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.40± 4.93e− 02 534.09± 6.81e− 02 pixels 19.59876664± 5.96e− 06 46.68777468± 6.99e− 05 hours/degreesOffset 0.0211± 4.93e− 02 −0.0385± 6.81e− 02 pixels −0.1503± 2.21e− 01 0.0888± 2.52e− 01 arcsecondsOffset/σ 0.43 −0.56 −0.68 0.35

Offset Distance 0.0439± 6.48e− 02 pixels 0.1746± 2.58e− 01 arcsecondsOffset Distance/σ 0.68 0.68

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 50.

53

Page 56: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 12 / Target Table 53

Difference image for target 9836149, planet candidate 1, quarter 12, target table 53. 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 = 4; number of valid in-transitcadences = 23; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 55; number of out-of-transit cadence gaps = 2. Difference image qualitymetric = 0.91 (good).Open ./planet-01/difference-image/009836149-01-difference-image-12-053.fig

54

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 12 / Target Table 53

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 53.

55

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 12 / Target Table 53

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 844.02± 2.79e− 05 534.55± 2.24e− 05 pixels 19.59876951± 3.08e− 09 46.68775420± 2.72e− 08 hours/degreesDifference Image Centroid 843.85± 1.20e− 01 534.64± 6.15e− 02 pixels 19.59878967± 1.14e− 05 46.68776904± 9.25e− 05 hours/degreesOffset −0.1684± 1.20e− 01 0.0841± 6.15e− 02 pixels 0.7470± 4.23e− 01 0.0534± 3.33e− 01 arcsecondsOffset/σ −1.40 1.37 1.77 0.16

Offset Distance 0.1882± 1.09e− 01 pixels 0.7489± 4.35e− 01 arcsecondsOffset Distance/σ 1.73 1.72

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

KIC Reference Centroid 844.01± 9.52e− 06 534.56± 7.27e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 843.85± 1.20e− 01 534.64± 6.15e− 02 pixels 19.59878967± 1.14e− 05 46.68776904± 9.25e− 05 hours/degreesOffset −0.1608± 1.20e− 01 0.0752± 6.15e− 02 pixels 0.7028± 4.23e− 01 0.0685± 3.33e− 01 arcsecondsOffset/σ −1.34 1.22 1.66 0.21

Offset Distance 0.1775± 1.10e− 01 pixels 0.7061± 4.39e− 01 arcsecondsOffset Distance/σ 1.61 1.61

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 53.

56

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 13 / Target Table 56

Difference image for target 9836149, planet candidate 1, quarter 13, target table 56. 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 = 4; number of valid in-transitcadences = 20; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 59; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.91 (good).Open ./planet-01/difference-image/009836149-01-difference-image-13-056.fig

57

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 13 / Target Table 56

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 56.

58

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 13 / Target Table 56

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 845.12± 3.71e− 05 538.04± 2.64e− 05 pixels 19.59877127± 3.82e− 09 46.68777852± 3.38e− 08 hours/degreesDifference Image Centroid 845.34± 5.35e− 02 538.21± 5.27e− 02 pixels 19.59876021± 5.98e− 06 46.68749601± 5.59e− 05 hours/degreesOffset 0.2189± 5.35e− 02 0.1676± 5.27e− 02 pixels −0.4099± 2.21e− 01 −1.0170± 2.01e− 01 arcsecondsOffset/σ 4.09 3.18 −1.85 −5.05

Offset Distance 0.2757± 5.07e− 02 pixels 1.0965± 2.02e− 01 arcsecondsOffset Distance/σ 5.43 5.43

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

KIC Reference Centroid 845.14± 8.73e− 06 538.06± 6.84e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 845.34± 5.35e− 02 538.21± 5.27e− 02 pixels 19.59876021± 5.98e− 06 46.68749601± 5.59e− 05 hours/degreesOffset 0.2012± 5.35e− 02 0.1481± 5.27e− 02 pixels −0.3886± 2.21e− 01 −0.9144± 2.01e− 01 arcsecondsOffset/σ 3.76 2.81 −1.76 −4.54

Offset Distance 0.2498± 5.08e− 02 pixels 0.9935± 2.02e− 01 arcsecondsOffset Distance/σ 4.92 4.92

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 56.

59

Page 62: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 14 / Target Table 59

Difference image for target 9836149, planet candidate 1, quarter 14, target table 59. 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 = 4; number of valid in-transitcadences = 21; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 58; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.97 (good).Open ./planet-01/difference-image/009836149-01-difference-image-14-059.fig

60

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 14 / Target Table 59

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 59.

61

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 14 / Target Table 59

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 840.06± 3.72e− 05 538.21± 2.72e− 05 pixels 19.59877159± 3.88e− 09 46.68776266± 3.43e− 08 hours/degreesDifference Image Centroid 839.96± 6.68e− 02 538.24± 5.98e− 02 pixels 19.59878201± 6.87e− 06 46.68779385± 6.95e− 05 hours/degreesOffset −0.0979± 6.68e− 02 0.0251± 5.98e− 02 pixels 0.3859± 2.54e− 01 0.1123± 2.50e− 01 arcsecondsOffset/σ −1.47 0.42 1.52 0.45

Offset Distance 0.1010± 6.57e− 02 pixels 0.4019± 2.62e− 01 arcsecondsOffset Distance/σ 1.54 1.53

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

KIC Reference Centroid 840.07± 7.21e− 06 538.22± 9.07e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 839.96± 6.68e− 02 538.24± 5.98e− 02 pixels 19.59878201± 6.87e− 06 46.68779385± 6.95e− 05 hours/degreesOffset −0.1108± 6.68e− 02 0.0195± 5.98e− 02 pixels 0.4188± 2.54e− 01 0.1579± 2.50e− 01 arcsecondsOffset/σ −1.66 0.33 1.65 0.63

Offset Distance 0.1125± 6.61e− 02 pixels 0.4476± 2.64e− 01 arcsecondsOffset Distance/σ 1.70 1.70

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 59.

62

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 15 / Target Table 62

Difference image for target 9836149, planet candidate 1, quarter 15, target table 62. 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 = 5; number of valid in-transitcadences = 26; number of in-transit cadence gaps = 1; number of valid out-of-transit cadences = 72; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.98 (good).Open ./planet-01/difference-image/009836149-01-difference-image-15-062.fig

63

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 15 / Target Table 62

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 62.

64

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 15 / Target Table 62

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 840.41± 2.05e− 05 534.12± 2.93e− 05 pixels 19.59876809± 2.68e− 09 46.68774492± 3.19e− 08 hours/degreesDifference Image Centroid 840.37± 4.59e− 02 534.31± 6.52e− 02 pixels 19.59878260± 5.45e− 06 46.68758797± 6.80e− 05 hours/degreesOffset −0.0439± 4.59e− 02 0.1911± 6.52e− 02 pixels 0.5373± 2.02e− 01 −0.5650± 2.45e− 01 arcsecondsOffset/σ −0.96 2.93 2.66 −2.31

Offset Distance 0.1960± 6.40e− 02 pixels 0.7797± 2.55e− 01 arcsecondsOffset Distance/σ 3.06 3.06

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

KIC Reference Centroid 840.39± 9.00e− 06 534.13± 9.50e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 840.37± 4.59e− 02 534.31± 6.52e− 02 pixels 19.59878260± 5.45e− 06 46.68758797± 6.80e− 05 hours/degreesOffset −0.0206± 4.59e− 02 0.1826± 6.52e− 02 pixels 0.4407± 2.02e− 01 −0.5833± 2.45e− 01 arcsecondsOffset/σ −0.45 2.80 2.18 −2.38

Offset Distance 0.1838± 6.48e− 02 pixels 0.7311± 2.58e− 01 arcsecondsOffset Distance/σ 2.84 2.84

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 62.

65

Page 68: for Kepler ID 9836149 Quarters 1 - 16

6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 16 / Target Table 65

Difference image for target 9836149, planet candidate 1, quarter 16, target table 65. 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 = 16; number of in-transit cadence gaps = 0; number of valid out-of-transit cadences = 44; number of out-of-transit cadence gaps = 0. Difference image qualitymetric = 0.93 (good).Open ./planet-01/difference-image/009836149-01-difference-image-16-065.fig

66

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 16 / Target Table 65

The pixel correlation statistic plot is not available because either the fit for target 9836149, planet candidate 1 failed,or there were no observed transits for this candidate in target table 65.

67

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6 PIXEL LEVEL DIAGNOSTICS Target 9836149 / Planet Candidate 1 / Quarter 16 / Target Table 65

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 844.04± 2.96e− 05 534.56± 2.53e− 05 pixels 19.59876927± 3.23e− 09 46.68774687± 3.00e− 08 hours/degreesDifference Image Centroid 844.01± 8.79e− 02 534.53± 6.63e− 02 pixels 19.59876953± 9.12e− 06 46.68779614± 7.77e− 05 hours/degreesOffset −0.0248± 8.79e− 02 −0.0371± 6.63e− 02 pixels 0.0097± 3.38e− 01 0.1774± 2.80e− 01 arcsecondsOffset/σ −0.28 −0.56 0.03 0.63

Offset Distance 0.0447± 7.15e− 02 pixels 0.1776± 2.84e− 01 arcsecondsOffset Distance/σ 0.62 0.63

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

KIC Reference Centroid 844.03± 8.84e− 06 534.57± 6.71e− 06 pixels 19.59877070± 0.00e+ 00 46.68775000± 0.00e+ 00 hours/degreesDifference Image Centroid 844.01± 8.79e− 02 534.53± 6.63e− 02 pixels 19.59876953± 9.12e− 06 46.68779614± 7.77e− 05 hours/degreesOffset −0.0119± 8.79e− 02 −0.0415± 6.63e− 02 pixels −0.0432± 3.38e− 01 0.1661± 2.80e− 01 arcsecondsOffset/σ −0.14 −0.63 −0.13 0.59

Offset Distance 0.0432± 6.69e− 02 pixels 0.1716± 2.66e− 01 arcsecondsOffset Distance/σ 0.65 0.65

PRF Fit of the Pixel Correlation Image

The pixel correlation image centroid could not be calculated for target 9836149,planet candidate 1, in target table 65.

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7 PHASED LIGHT CURVES Target 9836149

7 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/009836149-01-phased-unwhitened-flux-time-series.fig

69

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7 PHASED LIGHT CURVES Target 9836149

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/009836149-01-phased-whitened-flux-time-series.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

8 Planet Candidate 1

8.1 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 3.5000 hoursTransit Epoch 54966.9738658 MJDOrbital Period 17.8161831 daysMaximum SES 15.9Maximum MES 30.5Robust Statistic 27.1Chi Square1 Statistic 950.4Chi Square1 Degrees of Freedom 1008Chi Square2 Statistic 96.9Chi Square2 Degrees of Freedom 71

DV Fit Parameter Value Uncertainty Units

SNR 33.6Model Chi Square 2112Degrees of Freedom 2551Transit Epoch 134.4823813 2.0688e-03 BKJDEccentricity 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 degreesPlanet Radius 3.2159 2.4078e-01 Earth radiiPlanet Radius to Star Radius Ratio 0.0315867 2.3649e-03Semi-major Axis 0.1321 2.2598e-07 AUSemi-major Axis to Star Radius Ratio 21.9269 7.6121e+00Impact Parameter 0.8595 1.0738e-01Star Radius 0.9330 0.0000e+00 solar radiiTransit Duration 3.5414 2.5694e-01 hoursTransit Ingress Time 0.3835 2.9668e-01 hoursTransit Depth 907 2.7117e+01 ppmOrbital Period 17.8159471 4.5724e-05 daysEquilibrium Temperature 699 8.4971e+01 Kelvin

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PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-01/TargetTableId-020, start BJD is 2454964 and thevertical offset is 0. For the data of Quarter-02/TargetTableId-021, start BJD is 2455002 and the vertical offset is 0.05. For the data of Quarter-03/TargetTableId-026,start BJD is 2455093 and the vertical offset is 0.1. For the data of Quarter-04/TargetTableId-029, start BJD is 2455184 and the vertical offset is 0.15. 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/009836149-01-all-unwhitened-01-020.fig

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PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-05/TargetTableId-032, start BJD is 2455276 and thevertical offset is 0. For the data of Quarter-06/TargetTableId-035, start BJD is 2455372 and the vertical offset is 0.05. For the data of Quarter-07/TargetTableId-038,start BJD is 2455463 and the vertical offset is 0.1. For the data of Quarter-08/TargetTableId-041, start BJD is 2455568 and the vertical offset is 0.15. 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/009836149-01-all-unwhitened-05-032.fig

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PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-09/TargetTableId-044, start BJD is 2455641 and thevertical offset is 0. For the data of Quarter-10/TargetTableId-047, start BJD is 2455739 and the vertical offset is 0.05. For the data of Quarter-11/TargetTableId-050,start BJD is 2455834 and the vertical offset is 0.1. For the data of Quarter-12/TargetTableId-053, start BJD is 2455932 and the vertical offset is 0.15. 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/009836149-01-all-unwhitened-09-044.fig

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PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-13/TargetTableId-056, start BJD is 2456015 and thevertical offset is 0. For the data of Quarter-14/TargetTableId-059, start BJD is 2456107 and the vertical offset is 0.05. For the data of Quarter-15/TargetTableId-062,start BJD is 2456206 and the vertical offset is 0.1. For the data of Quarter-16/TargetTableId-065, start BJD is 2456305 and the vertical offset is 0.15. 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/009836149-01-all-unwhitened-13-056.fig

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PDC Flux time series for KeplerId 9836149, 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/009836149-01-all-unwhitened-zoomed.fig

PDC Flux time series of all transits for KeplerId 9836149, 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/009836149-01-all-unwhitened-filtered-zoomed.fig

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Folded flux time series for KeplerId 9836149, Planet candidate 1 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. The bluedots 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; the greendots 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/009836149-01-all-whitened.fig

Folded flux time series for KeplerId 9836149, 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/009836149-01-all-whitened-zoomed.fig

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8.2 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 34.8 2865.9 0.0272970 4.0603e-04 41.8409 6.7809e-01 891 2.6503e+01 3.3258 5.3709e-020.30 34.8 2866.6 0.0275344 4.0978e-04 40.0963 6.5572e-01 891 2.6510e+01 3.3359 5.4346e-020.50 34.8 2866.7 0.0281001 4.1817e-04 36.3790 5.9548e-01 891 2.6515e+01 3.3609 5.4763e-020.70 34.8 2866.3 0.0292416 4.3571e-04 30.1068 4.9782e-01 891 2.6528e+01 3.4111 5.6042e-020.90 34.9 2861.0 0.0324286 4.8978e-04 18.6362 3.4149e-01 898 2.7057e+01 3.6945 6.6810e-02

Highlighted row is used to seed all transits fit with all parameters.

Model chi squares of reduced parameter fits vs. impact parameter for KeplerId 9836149, Planet candidate 1. The fit result with the minimum chi square is marked witha dashed line in the plot and set as the seed for the all transits fit with all model parameters.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/009836149-01-reduced-fits-chi-square.fig

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Ratios of planet radius to star radius of reduced parameter fits vs. impact parameter for KeplerId 9836149, Planet candidate 1. The fit result with the minimum chisquare is marked with a dashed line in the plot and set as the seed for the all transits fit with all model parameters.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/009836149-01-reduced-fits-rp-over-rstar.fig

Ratios of semimajor axis to star radius of reduced parameter fits vs. impact parameter for KeplerId 9836149, Planet candidate 1. The fit result with the minimum chisquare is marked with a dashed line in the plot and set as the seed for the all transits fit with all model parameters.Open ./planet-01/planet-search-and-model-fitting-results/reduced-parameter-fits/009836149-01-reduced-fits-a-over-rstar.fig

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8.3 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.

8.3.1 Weak Secondary Test

Period (days) Duration (hours) Max MES Sec Phase (days) Sec MES Min Phase (days) Min MES MAD

17.8162 3.5 30.5168 3.2966 2.9083 -0.21115 -4.9933 0.72814

8.3.2 Flux-Weighted Centroid Test

Result Value Uncertainty Units Value in Sigmas Significance (%)

Stellar Magnitude 15.2000Motion Detection Statistic 3.3424e+00 18.80Peak RA Offset 2.0702e-04 2.8036e-04 arcseconds 0.7384Peak Dec Offset 2.2193e-04 3.1884e-04 arcseconds 0.6961Peak Offset Distance 3.0350e-04 3.0155e-04 arcseconds 1.0065Source RA Offset -1.8702e-01 3.0141e-01 arcseconds -0.6205Source Dec Offset -1.0647e-01 3.3728e-01 arcseconds -0.3157Source Offset Distance 2.1520e-01 3.1058e-01 arcseconds 0.6929Source RA 19.59876565 8.1369e-06 hoursSource Dec 46.68772042 9.3689e-05 degrees

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

8.3.3 Eclipsing Binary Discrimination Test

Result Value Value in Sigmas Significance (%)

Odd Even Transit Depth Comparison Statistic 5.9125e-02 0.2432 80.79Odd Even Transit Epoch Comparison Statistic 6.8439e-04 0.0262 97.91

8.3.4 Bootstrap Test

No bootstrap results available.

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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 3.5. The maximum secondary MES and corresponding phase are 2.9083 and 3.2966 days respectively.The minimum secondary MES and corresponding phase are-4.9933 and -0.21115 days respectively.Open ./planet-01/report-summary/009836149-01-weak-secondary-diagnostic.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-folded-transit-fit-fluxWeighted-centroids.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-01.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-02.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-03.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-04.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-05.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-06.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-07.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-08.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-09.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-10.fig

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KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-11.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-12.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-13.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-14.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-15.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

KeplerId 9836149, KeplerMag 15.20 - 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/009836149-01-transit-fit-fluxWeighted-centroids-16.fig

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8 PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

No figures named 009836149-01-bootstrap-false-alarm.fig are available.

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Appendix A Planet Candidate 1

A.1 Model Fitter: All Transits

Robust weights distribution for KeplerId 9836149, 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/009836149-01-all-robust-weights.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Fit residuals distribution for KeplerId 9836149, 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/009836149-01-all-histo-used.fig

Fit residuals distribution for KeplerId 9836149, 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/009836149-01-all-histo-all-and-unused.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

A.2 Model Fitter: Odd & Even Transits

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

SNR 24.4 23.2Model Chi Square 2007 2007Degrees of Freedom 2444 2444Transit Epoch 134.4803884 2.7829e-03 152.3002010 2.9155e-03 BKJD 9.5908e-01Eccentricity 0.0000 0.0000e+00 0.0000 0.0000e+00Peri Longitude 0.0000 0.0000e+00 0.0000 0.0000e+00 degreesPlanet Radius 3.0843 6.2880e-01 3.1715 4.6130e-01 Earth radii 1.1182e-01Planet Radius to Star Radius Ratio 0.0302943 6.1761e-03 0.0311509 4.5309e-03 1.1182e-01Semi-major Axis 0.1321 3.1393e-07 0.1321 3.1387e-07 AU 1.2771e+00Semi-major Axis to Star Radius Ratio 25.6561 2.4857e+01 24.9405 1.7071e+01 2.3733e-02Impact Parameter 0.7835 4.8443e-01 0.8276 2.6478e-01 7.9846e-02Star Radius 0.9330 0.0000e+00 0.9330 0.0000e+00 solar radiiTransit Duration 3.5492 4.8504e-01 3.3567 4.0088e-01 hours 3.0589e-01Transit Ingress Time 0.2586 5.5728e-01 0.3028 4.6144e-01 hours 6.1102e-02Transit Depth 903 3.6193e+01 916 3.9224e+01 ppm 2.4316e-01Orbital Period 17.8160083 6.3521e-05 17.8158936 6.3507e-05 days 1.2771e+00Equilibrium Temperature 699 8.4971e+01 699 8.4971e+01 Kelvin 1.2490e-05

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-01/TargetTableId-020, start BJD is 2454964 and thevertical offset is 0. For the data of Quarter-02/TargetTableId-021, start BJD is 2455002 and the vertical offset is 0.05. For the data of Quarter-03/TargetTableId-026,start BJD is 2455093 and the vertical offset is 0.1. For the data of Quarter-04/TargetTableId-029, start BJD is 2455184 and the vertical offset is 0.15. 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/009836149-01-odd-even-unwhitened-01-020.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-05/TargetTableId-032, start BJD is 2455276 and thevertical offset is 0. For the data of Quarter-06/TargetTableId-035, start BJD is 2455372 and the vertical offset is 0.05. For the data of Quarter-07/TargetTableId-038,start BJD is 2455463 and the vertical offset is 0.1. For the data of Quarter-08/TargetTableId-041, start BJD is 2455568 and the vertical offset is 0.15. 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/009836149-01-odd-even-unwhitened-05-032.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-09/TargetTableId-044, start BJD is 2455641 and thevertical offset is 0. For the data of Quarter-10/TargetTableId-047, start BJD is 2455739 and the vertical offset is 0.05. For the data of Quarter-11/TargetTableId-050,start BJD is 2455834 and the vertical offset is 0.1. For the data of Quarter-12/TargetTableId-053, start BJD is 2455932 and the vertical offset is 0.15. 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/009836149-01-odd-even-unwhitened-09-044.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

PDC Flux time series for KeplerId 9836149, Planet candidate 1 in the unwhitened domain. For the data of Quarter-13/TargetTableId-056, start BJD is 2456015 and thevertical offset is 0. For the data of Quarter-14/TargetTableId-059, start BJD is 2456107 and the vertical offset is 0.05. For the data of Quarter-15/TargetTableId-062,start BJD is 2456206 and the vertical offset is 0.1. For the data of Quarter-16/TargetTableId-065, start BJD is 2456305 and the vertical offset is 0.15. 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/009836149-01-odd-even-unwhitened-13-056.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

PDC Flux time series for KeplerId 9836149, 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/009836149-01-odd-even-unwhitened-zoomed.fig

PDC Flux time series of odd/even transits for KeplerId 9836149, 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/009836149-01-odd-even-unwhitened-filtered-zoomed.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Folded flux time series for KeplerId 9836149, Planet candidate 1 in the whitened domain is plotted in black dots. Values are averaged into 1 cadence wide bins. The bluedots 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 transits fit;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/009836149-01-odd-even-whitened.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Folded flux time series for KeplerId 9836149, 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/009836149-01-odd-even-whitened-zoomed.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Robust weights distribution for KeplerId 9836149, 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/009836149-01-odd-even-robust-weights.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

Fit residuals distribution for KeplerId 9836149, 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/009836149-01-odd-even-histo-used.fig

Fit residuals distribution for KeplerId 9836149, 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/009836149-01-odd-even-histo-all-and-unused.fig

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APPENDIX A: PLANET CANDIDATE 1 Target 9836149 / Planet Candidate 1

A.3 Eclipsing Binary Discrimination Test

Top-left: Diagnostic plot of Odd/Even Transit Depth Test for keplerId 9836149, 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 9836149, planet 1. A significance level close to 1/0 favors a transiting planet/an eclipsing binary.Open ./planet-01/binary-discrimination-test-results/009836149-01-eclipsing-binary-discrimination-tests.fig

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APPENDIX B: SINGLE EVENT STATISTICS FROM RESIDUAL FLUX Target 9836149

Appendix B Single Event Statistics from Residual Flux

No figures named 009836149-00-residual-ses-*.fig are available.

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APPENDIX C: ALERTS Target 9836149

Appendix C Alerts

Time Severity Message

56520.2506 warning Multi-quarter PRF fitting and offset analysis will not be performed because model fit SNR is above specified threshold (target=1,keplerId=9836149, planet=1, component=generateDvDifferenceImages)

56520.2536 warning No centroid data available. Centroid test results set to default values for all planets. (target=1, keplerId=9836149, component=Centroidtest prf)

56520.2566 warning Pixel correlation test is disabled (target=1, keplerId=9836149, component=Pixel correlation test)56520.2566 warning Statistical bootstrap is disabled (target=1, keplerId=9836149, component=bootstrap)

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