# Image stretching and normalization¶

The `astropy.visualization`

module provides a framework for
transforming values in images (and more generally any arrays),
typically for the purpose of visualization. Two main types of
transformations are provided:

- Normalization to the [0:1] range using lower and upper limits where \(x\) represents the values in the original image:

*Stretching*of values in the [0:1] range to the [0:1] range using a linear or non-linear function:

In addition, classes are provided in order to identify lower and upper limits for a dataset based on specific algorithms (such as using percentiles).

Identifying lower and upper limits, as well as re-normalizing, is described in the Intervals and Normalization section, while stretching is described in the Stretching section.

## Intervals and Normalization¶

Several classes are provided for determining intervals and for
normalizing values in this interval to the [0:1] range. One of the
simplest examples is the
`MinMaxInterval`

which determines the
limits of the values based on the minimum and maximum values in the
array. The class is instantiated with no arguments:

```
>>> from astropy.visualization import MinMaxInterval
>>> interval = MinMaxInterval()
```

and the limits can be determined by calling the
`get_limits()`

method, which
takes the array of values:

```
>>> interval.get_limits([1, 3, 4, 5, 6])
(1, 6)
```

The `interval`

instance can also be called like a function to
actually normalize values to the range:

```
>>> interval([1, 3, 4, 5, 6])
array([0. , 0.4, 0.6, 0.8, 1. ])
```

Other interval classes include
`ManualInterval`

,
`PercentileInterval`

,
`AsymmetricPercentileInterval`

, and
`ZScaleInterval`

. For these, values in
the array can fall outside of the limits given by the interval. A
`clip`

argument is provided to control the behavior of the
normalization when values fall outside the limits:

```
>>> from astropy.visualization import PercentileInterval
>>> interval = PercentileInterval(50.)
>>> interval.get_limits([1, 3, 4, 5, 6])
(3.0, 5.0)
>>> interval([1, 3, 4, 5, 6]) # default is clip=True
array([0. , 0. , 0.5, 1. , 1. ])
>>> interval([1, 3, 4, 5, 6], clip=False)
array([-1. , 0. , 0.5, 1. , 1.5])
```

## Stretching¶

In addition to classes that can scale values to the [0:1] range, a
number of classes are provided to ‘stretch’ the values using different
functions. These map a [0:1] range onto a transformed [0:1] range. A
simple example is the `SqrtStretch`

class:

```
>>> from astropy.visualization import SqrtStretch
>>> stretch = SqrtStretch()
>>> stretch([0., 0.25, 0.5, 0.75, 1.])
array([0. , 0.5 , 0.70710678, 0.8660254 , 1. ])
```

As for the intervals, values outside the [0:1] range can be treated
differently depending on the `clip`

argument. By default, output
values are clipped to the [0:1] range:

```
>>> stretch([-1., 0., 0.5, 1., 1.5])
array([0. , 0. , 0.70710678, 1. , 1. ])
```

but this can be disabled:

```
>>> stretch([-1., 0., 0.5, 1., 1.5], clip=False)
array([ nan, 0. , 0.70710678, 1. , 1.22474487])
```

Note

The stretch functions are similar but not always strictly
identical to those used in e.g. DS9 (although they should have
the same behavior). The equations for the DS9 stretches can be
found here and can be
compared to the equations for our stretches provided in the
`astropy.visualization`

API section. The main difference between
our stretches and DS9 is that we have adjusted them so that the
[0:1] range always maps exactly to the [0:1] range.

## Combining transformations¶

Any intervals and stretches can be chained by using the `+`

operator, which returns a new transformation. When combining intervals
and stretches, the stretch object must come before the interval
object. For example, to apply normalization based on a percentile
value, followed by a square root stretch, you can do:

```
>>> transform = SqrtStretch() + PercentileInterval(90.)
>>> transform([1, 3, 4, 5, 6])
array([0. , 0.60302269, 0.76870611, 0.90453403, 1. ])
```

As before, the combined transformation can also accept a `clip`

argument (which is `True`

by default).

## Matplotlib normalization¶

Matplotlib allows a custom normalization and stretch to be used when
displaying data by passing a `matplotlib.colors.Normalize`

object, e.g. to `imshow()`

. The
`astropy.visualization`

module provides an
`ImageNormalize`

class
that wraps the interval (see Intervals and Normalization) and
stretch (see Stretching) objects into an object Matplotlib
understands.

The inputs to the
`ImageNormalize`

class are
the data and the interval and stretch objects:

```
import numpy as np
import matplotlib.pyplot as plt
from astropy.visualization import (MinMaxInterval, SqrtStretch,
ImageNormalize)
# Generate a test image
image = np.arange(65536).reshape((256, 256))
# Create an ImageNormalize object
norm = ImageNormalize(image, interval=MinMaxInterval(),
stretch=SqrtStretch())
# or equivalently using positional arguments
# norm = ImageNormalize(image, MinMaxInterval(), SqrtStretch())
# Display the image
fig = plt.figure()
ax = fig.add_subplot(1, 1, 1)
im = ax.imshow(image, origin='lower', norm=norm)
fig.colorbar(im)
```

As shown above, the colorbar ticks are automatically adjusted.

The input image to `ImageNormalize`

is typically the one to be displayed, so there is a convenience function
`imshow_norm()`

to ease this use case:

```
import numpy as np
import matplotlib.pyplot as plt
from astropy.visualization import imshow_norm, MinMaxInterval, SqrtStretch
# Generate a test image
image = np.arange(65536).reshape((256, 256))
# Display the exact same thing as the above plot
fig = plt.figure()
ax = fig.add_subplot(1, 1, 1)
im, norm = imshow_norm(image, ax, origin='lower',
interval=MinMaxInterval(), stretch=SqrtStretch())
fig.colorbar(im)
```

While this is the simplest case, it is also possible for a completely different image to be used to establish the normalization (e.g. if one wants to display several images with exactly the same normalization and stretch).

The inputs to the
`ImageNormalize`

class can
also be the vmin and vmax limits, which you can determine from the
Intervals and Normalization classes, and the stretch object:

```
import numpy as np
import matplotlib.pyplot as plt
from astropy.visualization import (MinMaxInterval, SqrtStretch,
ImageNormalize)
# Generate a test image
image = np.arange(65536).reshape((256, 256))
# Create interval object
interval = MinMaxInterval()
vmin, vmax = interval.get_limits(image)
# Create an ImageNormalize object using a SqrtStretch object
norm = ImageNormalize(vmin=vmin, vmax=vmax, stretch=SqrtStretch())
# Display the image
fig = plt.figure()
ax = fig.add_subplot(1, 1, 1)
im = ax.imshow(image, origin='lower', norm=norm)
fig.colorbar(im)
```

Finally, we also provide a convenience
`simple_norm()`

function that
can be useful for quick interactive analysis (it is also used by the
`fits2bitmap`

command-line script). However, it is not recommended
to be used in scripted programs; it’s better to use
`ImageNormalize`

directly:

```
import numpy as np
import matplotlib.pyplot as plt
from astropy.visualization import simple_norm
# Generate a test image
image = np.arange(65536).reshape((256, 256))
# Create an ImageNormalize object
norm = simple_norm(image, 'sqrt')
# Display the image
fig = plt.figure()
ax = fig.add_subplot(1, 1, 1)
im = ax.imshow(image, origin='lower', norm=norm)
fig.colorbar(im)
```