This tutorial demonstrates the basic steps required to recover a transiting planet candidate in the Kepler data.

We will show how you can recover the signal of Kepler-10b, the first rocky planet that was discovered by Kepler!

```
[1]:
```

```
from lightkurve import search_targetpixelfile
tpf = search_targetpixelfile("Kepler-10", quarter=3).download()
tpf.shape
```

```
[1]:
```

```
(4140, 10, 11)
```

Let’s use the `plot`

method and pass along an aperture mask and a few plotting arguments.

```
[2]:
```

```
tpf.plot(scale='log');
```

The target pixel file contains one bright star with approximately 50,000 counts.

Now, we will use the `to_lightcurve`

method to create a simple aperture photometry lightcurve using the mask defined by the pipeline which is stored in `tpf.pipeline_mask`

.

```
[3]:
```

```
lc = tpf.to_lightcurve(aperture_mask=tpf.pipeline_mask)
```

Let’s take a look at the output lightcurve.

```
[4]:
```

```
lc.plot();
```

Now let’s use the `flatten`

method, removes long-term variability that we are not interested in.

```
[5]:
```

```
flat, trend = lc.flatten(window_length=301, return_trend=True)
```

Let’s plot the trend estimated by the Savitzky-Golay filter:

```
[6]:
```

```
ax = lc.errorbar() # plot() returns a matplotlib axes ...
trend.plot(ax=ax, color='red', label='Trend'); # which we can pass to the next plot() to use the same axes
```

and the flat lightcurve:

```
[7]:
```

```
flat.errorbar();
```

Now, let’s run a period search function using the Box-Least Squares algorithm, which was added to the AstroPy package in version 3.1.

```
[8]:
```

```
from astropy.stats import BoxLeastSquares
bls = BoxLeastSquares(flat.time, flat.flux, flat.flux_err)
```

We will use the BLS algorithm to search a pre-defined grid of transit periods and durations:

```
[9]:
```

```
import numpy as np
periods = np.arange(0.3, 1.5, 0.001)
durations = np.arange(0.005, 0.15, 0.001)
periodogram = bls.power(periods, durations)
```

```
[10]:
```

```
import matplotlib.pyplot as plt
plt.plot(periodogram.period, periodogram.power)
plt.ylabel("Power")
plt.xlabel("Period [day]");
```

```
[11]:
```

```
best_fit = periods[np.argmax(periodogram.power)]
print('Best Fit Period: {:0.4f} days'.format(best_fit))
```

```
Best Fit Period: 0.8380 days
```

```
[12]:
```

```
flat.fold(best_fit).errorbar();
```

We successfully recovered the planet!

Created with ♥ by the Lightkurve collaboration. Please cite us or join us on GitHub.