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old-saburly-wagtail-web/env/lib/python3.10/site-packages/PIL/__pycache__/Image.cpython-310.pyc

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Initial commit
2024-08-27 20:33:44 +02:00
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Gets the number of individual bands for this mode.
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This class represents an image object. To create
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* :py:func:`~PIL.Image.open`
* :py:func:`~PIL.Image.new`
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Closes the file pointer, if possible.
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The image data will be unusable afterward.
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Return image as a bytes object.
.. warning::
This method returns the raw image data from the internal
storage. For compressed image data (e.g. PNG, JPEG) use
:meth:`~.save`, with a BytesIO parameter for in-memory
data.
:param encoder_name: What encoder to use. The default is to
use the standard "raw" encoder.
A list of C encoders can be seen under
codecs section of the function array in
:file:`_imaging.c`. Python encoders are
registered within the relevant plugins.
:param args: Extra arguments to the encoder.
:returns: A :py:class:`bytes` object.
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Returns the image converted to an X11 bitmap.
.. note:: This method only works for mode "1" images.
:param name: The name prefix to use for the bitmap variables.
:returns: A string containing an X11 bitmap.
:raises ValueError: If the mode is not "1"
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Loads this image with pixel data from a bytes object.
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Allocates storage for the image and loads the pixel data. In
normal cases, you don't need to call this method, since the
Image class automatically loads an opened image when it is
accessed for the first time.
If the file associated with the image was opened by Pillow, then this
method will close it. The exception to this is if the image has
multiple frames, in which case the file will be left open for seek
operations. See :ref:`file-handling` for more information.
:returns: An image access object.
:rtype: :py:class:`.PixelAccess` or :py:class:`.PyAccess`
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Verifies the contents of a file. For data read from a file, this
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problems, it raises suitable exceptions. If you need to load
the image after using this method, you must reopen the image
file.
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Returns a converted copy of this image. For the "P" mode, this
method translates pixels through the palette. If mode is
omitted, a mode is chosen so that all information in the image
and the palette can be represented without a palette.
This supports all possible conversions between "L", "RGB" and "CMYK". The
``matrix`` argument only supports "L" and "RGB".
When translating a color image to grayscale (mode "L"),
the library uses the ITU-R 601-2 luma transform::
L = R * 299/1000 + G * 587/1000 + B * 114/1000
The default method of converting a grayscale ("L") or "RGB"
image into a bilevel (mode "1") image uses Floyd-Steinberg
dither to approximate the original image luminosity levels. If
dither is ``None``, all values larger than 127 are set to 255 (white),
all other values to 0 (black). To use other thresholds, use the
:py:meth:`~PIL.Image.Image.point` method.
When converting from "RGBA" to "P" without a ``matrix`` argument,
this passes the operation to :py:meth:`~PIL.Image.Image.quantize`,
and ``dither`` and ``palette`` are ignored.
When converting from "PA", if an "RGBA" palette is present, the alpha
channel from the image will be used instead of the values from the palette.
:param mode: The requested mode. See: :ref:`concept-modes`.
:param matrix: An optional conversion matrix. If given, this
should be 4- or 12-tuple containing floating point values.
:param dither: Dithering method, used when converting from
mode "RGB" to "P" or from "RGB" or "L" to "1".
Available methods are :data:`Dither.NONE` or :data:`Dither.FLOYDSTEINBERG`
(default). Note that this is not used when ``matrix`` is supplied.
:param palette: Palette to use when converting from mode "RGB"
to "P". Available palettes are :data:`Palette.WEB` or
:data:`Palette.ADAPTIVE`.
:param colors: Number of colors to use for the :data:`Palette.ADAPTIVE`
palette. Defaults to 256.
:rtype: :py:class:`~PIL.Image.Image`
:returns: An :py:class:`~PIL.Image.Image` object.
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Convert the image to 'P' mode with the specified number
of colors.
:param colors: The desired number of colors, <= 256
:param method: :data:`Quantize.MEDIANCUT` (median cut),
:data:`Quantize.MAXCOVERAGE` (maximum coverage),
:data:`Quantize.FASTOCTREE` (fast octree),
:data:`Quantize.LIBIMAGEQUANT` (libimagequant; check support
using :py:func:`PIL.features.check_feature` with
``feature="libimagequant"``).
By default, :data:`Quantize.MEDIANCUT` will be used.
The exception to this is RGBA images. :data:`Quantize.MEDIANCUT`
and :data:`Quantize.MAXCOVERAGE` do not support RGBA images, so
:data:`Quantize.FASTOCTREE` is used by default instead.
:param kmeans: Integer greater than or equal to zero.
:param palette: Quantize to the palette of given
:py:class:`PIL.Image.Image`.
:param dither: Dithering method, used when converting from
mode "RGB" to "P" or from "RGB" or "L" to "1".
Available methods are :data:`Dither.NONE` or :data:`Dither.FLOYDSTEINBERG`
(default).
:returns: A new image
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Copies this image. Use this method if you wish to paste things
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:rtype: :py:class:`~PIL.Image.Image`
:returns: An :py:class:`~PIL.Image.Image` object.
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Image.copy<70>box<6F>(tuple[float, float, float, float] | NonecCsd|dur|<00><00>S|d|dkrd}t|<02><01>|d|dkr$d}t|<02><01>|<00><02>|<00>|<00>|j|<01><02>S)a<>
Returns a rectangular region from this image. The box is a
4-tuple defining the left, upper, right, and lower pixel
coordinate. See :ref:`coordinate-system`.
Note: Prior to Pillow 3.4.0, this was a lazy operation.
:param box: The crop rectangle, as a (left, upper, right, lower)-tuple.
:rtype: :py:class:`~PIL.Image.Image`
:returns: An :py:class:`~PIL.Image.Image` object.
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Returns a rectangular region from the core image object im.
This is equivalent to calling im.crop((x0, y0, x1, y1)), but
includes additional sanity checks.
:param im: a core image object
:param box: The crop rectangle, as a (left, upper, right, lower)-tuple.
:returns: A core image object.
)r r<><00>round<6E>abs<62>_decompression_bomb_checkr<6B>)r<>r3r<><00>x0<78>y0<79>x1<78>y1<79>absolute_valuesr%r%r&r<>sz Image._cropr<70><00>tuple[int, int] | None<6E>0tuple[str, tuple[int, int, float, float]] | NonecCrm)aY
Configures the image file loader so it returns a version of the
image that as closely as possible matches the given mode and
size. For example, you can use this method to convert a color
JPEG to grayscale while loading it.
If any changes are made, returns a tuple with the chosen ``mode`` and
``box`` with coordinates of the original image within the altered one.
Note that this method modifies the :py:class:`~PIL.Image.Image` object
in place. If the image has already been loaded, this method has no
effect.
Note: This method is not implemented for most images. It is
currently implemented only for JPEG and MPO images.
:param mode: The requested mode.
:param size: The requested size in pixels, as a 2-tuple:
(width, height).
Nr%)r<>rtr<>r%r%r&<00>draft.sz Image.draft<66>xmargin<69>ymargincCs(|dur|}|<00><00>|<00>|j<02>||<02><02>Sr<>)rrr3<00>expand)r<>r<>r<>r%r%r&<00>_expandGsz Image._expandr<00><01> ImageFilter<65>filter<65>-ImageFilter.Filter | type[ImageFilter.Filter]cs<>ddlm}<00><01><02>t<03><00>r<11><00><00>t<04>d<03>sd}t|<03><01>t<06>|j<07>}<04>jj dks*|r3<72><01>
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Filters this image using the given filter. For a list of
available filters, see the :py:mod:`~PIL.ImageFilter` module.
:param filter: Filter kernel.
:returns: An :py:class:`~PIL.Image.Image` object.rr<>r<>z>filter argument should be ImageFilter.Filter instance or classc s$g|]}<01><01><00><00><01>j<02>|<01><01><01><01>qSr%)rr<>r3<00>getband)r<><00>c<>r<>r<>r%r&<00>
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Returns a tuple containing the name of each band in this image.
For example, ``getbands`` on an RGB image returns ("R", "G", "B").
:returns: A tuple containing band names.
:rtype: tuple
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alpha_onlyr<EFBFBD><00> tuple[int, int, int, int] | NonecCs|<00><00>|j<01>|<01>S)aG
Calculates the bounding box of the non-zero regions in the
image.
:param alpha_only: Optional flag, defaulting to ``True``.
If ``True`` and the image has an alpha channel, trim transparent pixels.
Otherwise, trim pixels when all channels are zero.
Keyword-only argument.
:returns: The bounding box is returned as a 4-tuple defining the
left, upper, right, and lower pixel coordinate. See
:ref:`coordinate-system`. If the image is completely empty, this
method returns None.
)rr3<00>getbbox)r<>r<>r%r%r&r<>us z Image.getbbox<6F> maxcolorscsR|<00><00>|jdvr#|j<02><03><00><00>fdd<03>td<04>D<00>}t|<02>|kr!dS|S|j<02>|<01>S)a<>
Returns a list of colors used in this image.
The colors will be in the image's mode. For example, an RGB image will
return a tuple of (red, green, blue) color values, and a P image will
return the index of the color in the palette.
:param maxcolors: Maximum number of colors. If this number is
exceeded, this method returns None. The default limit is
256 colors.
:returns: An unsorted list of (count, pixel) values.
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  zImage.getcolors<72>bandcCs"|<00><00>|dur|j<01>|<01>S|jS)a<>
Returns the contents of this image as a sequence object
containing pixel values. The sequence object is flattened, so
that values for line one follow directly after the values of
line zero, and so on.
Note that the sequence object returned by this method is an
internal PIL data type, which only supports certain sequence
operations. To convert it to an ordinary sequence (e.g. for
printing), use ``list(im.getdata())``.
:param band: What band to return. The default is to return
all bands. To return a single band, pass in the index
value (e.g. 0 to get the "R" band from an "RGB" image).
:returns: A sequence-like object.
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Gets the minimum and maximum pixel values for each band in
the image.
:returns: For a single-band image, a 2-tuple containing the
minimum and maximum pixel value. For a multi-band image,
a tuple containing one 2-tuple for each band.
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Returns a dictionary containing the XMP tags.
Requires defusedxml to be installed.
:returns: XMP tags in a dictionary.
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Returns the image palette as a list.
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.. versionadded:: 9.1.0
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image has no palette.
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Determine if an image has transparency data, whether in the form of an
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Returns the pixel value at a given position.
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Get projection to x and y axes
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Returns a histogram for the image. The histogram is returned as a
list of pixel counts, one for each pixel value in the source
image. Counts are grouped into 256 bins for each band, even if
the image has more than 8 bits per band. If the image has more
than one band, the histograms for all bands are concatenated (for
example, the histogram for an "RGB" image contains 768 values).
A bilevel image (mode "1") is treated as a grayscale ("L") image
by this method.
If a mask is provided, the method returns a histogram for those
parts of the image where the mask image is non-zero. The mask
image must have the same size as the image, and be either a
bi-level image (mode "1") or a grayscale image ("L").
:param mask: An optional mask.
:param extrema: An optional tuple of manually-specified extrema.
:returns: A list containing pixel counts.
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Calculates and returns the entropy for the image.
A bilevel image (mode "1") is treated as a grayscale ("L")
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those parts of the image where the mask image is non-zero.
The mask image must have the same size as the image, and be
either a bi-level image (mode "1") or a grayscale image ("L").
:param mask: An optional mask.
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:returns: A float value representing the image entropy
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Pastes another image into this image. The box argument is either
a 2-tuple giving the upper left corner, a 4-tuple defining the
left, upper, right, and lower pixel coordinate, or None (same as
(0, 0)). See :ref:`coordinate-system`. If a 4-tuple is given, the size
of the pasted image must match the size of the region.
If the modes don't match, the pasted image is converted to the mode of
this image (see the :py:meth:`~PIL.Image.Image.convert` method for
details).
Instead of an image, the source can be a integer or tuple
containing pixel values. The method then fills the region
with the given color. When creating RGB images, you can
also use color strings as supported by the ImageColor module.
If a mask is given, this method updates only the regions
indicated by the mask. You can use either "1", "L", "LA", "RGBA"
or "RGBa" images (if present, the alpha band is used as mask).
Where the mask is 255, the given image is copied as is. Where
the mask is 0, the current value is preserved. Intermediate
values will mix the two images together, including their alpha
channels if they have them.
See :py:meth:`~PIL.Image.Image.alpha_composite` if you want to
combine images with respect to their alpha channels.
:param im: Source image or pixel value (integer, float or tuple).
:param box: An optional 4-tuple giving the region to paste into.
If a 2-tuple is used instead, it's treated as the upper left
corner. If omitted or None, the source is pasted into the
upper left corner.
If an image is given as the second argument and there is no
third, the box defaults to (0, 0), and the second argument
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:param source: Optional 2 (left, top) tuple for the upper left
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zImage.alpha_composite<74>lut<75><Sequence[float] | Callable[[int], float] | ImagePointHandlercs<>|<00><00>t<01>t<02>r<0E><00>|<00>St<04><00>r7|jdvr't<06><00>\}}|<00>|j<08> ||<04><02>S<00>fdd<03>t
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Maps this image through a lookup table or function.
:param lut: A lookup table, containing 256 (or 65536 if
self.mode=="I" and mode == "L") values per band in the
image. A function can be used instead, it should take a
single argument. The function is called once for each
possible pixel value, and the resulting table is applied to
all bands of the image.
It may also be an :py:class:`~PIL.Image.ImagePointHandler`
object::
class Example(Image.ImagePointHandler):
def point(self, data):
# Return result
:param mode: Output mode (default is same as input). This can only be used if
the source image has mode "L" or "P", and the output has mode "1" or the
source image mode is "I" and the output mode is "L".
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Adds or replaces the alpha layer in this image. If the image
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:param alpha: The new alpha layer. This can either be an "L" or "1"
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Copies pixel data from a flattened sequence object into the image. The
values should start at the upper left corner (0, 0), continue to the
end of the line, followed directly by the first value of the second
line, and so on. Data will be read until either the image or the
sequence ends. The scale and offset values are used to adjust the
sequence values: **pixel = value*scale + offset**.
:param data: A flattened sequence object.
:param scale: An optional scale value. The default is 1.0.
:param offset: An optional offset value. The default is 0.0.
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Attaches a palette to this image. The image must be a "P", "PA", "L"
or "LA" image.
The palette sequence must contain at most 256 colors, made up of one
integer value for each channel in the raw mode.
For example, if the raw mode is "RGB", then it can contain at most 768
values, made up of red, green and blue values for the corresponding pixel
index in the 256 colors.
If the raw mode is "RGBA", then it can contain at most 1024 values,
containing red, green, blue and alpha values.
Alternatively, an 8-bit string may be used instead of an integer sequence.
:param data: A palette sequence (either a list or a string).
:param rawmode: The raw mode of the palette. Either "RGB", "RGBA", or a mode
that can be transformed to "RGB" or "RGBA" (e.g. "R", "BGR;15", "RGBA;L").
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Modifies the pixel at the given position. The color is given as
a single numerical value for single-band images, and a tuple for
multi-band images. In addition to this, RGB and RGBA tuples are
accepted for P and PA images.
Note that this method is relatively slow. For more extensive changes,
use :py:meth:`~PIL.Image.Image.paste` or the :py:mod:`~PIL.ImageDraw`
module instead.
See:
* :py:meth:`~PIL.Image.Image.paste`
* :py:meth:`~PIL.Image.Image.putdata`
* :py:mod:`~PIL.ImageDraw`
:param xy: The pixel coordinate, given as (x, y). See
:ref:`coordinate-system`.
:param value: The pixel value.
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Rewrites the image to reorder the palette.
:param dest_map: A list of indexes into the original palette.
e.g. ``[1,0]`` would swap a two item palette, and ``list(range(256))``
is the identity transform.
:param source_palette: Bytes or None.
:returns: An :py:class:`~PIL.Image.Image` object.
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Returns a resized copy of this image.
:param size: The requested size in pixels, as a 2-tuple:
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one of :py:data:`Resampling.NEAREST`, :py:data:`Resampling.BOX`,
:py:data:`Resampling.BILINEAR`, :py:data:`Resampling.HAMMING`,
:py:data:`Resampling.BICUBIC` or :py:data:`Resampling.LANCZOS`.
If the image has mode "1" or "P", it is always set to
:py:data:`Resampling.NEAREST`. If the image mode specifies a number
of bits, such as "I;16", then the default filter is
:py:data:`Resampling.NEAREST`. Otherwise, the default filter is
:py:data:`Resampling.BICUBIC`. See: :ref:`concept-filters`.
:param box: An optional 4-tuple of floats providing
the source image region to be scaled.
The values must be within (0, 0, width, height) rectangle.
If omitted or None, the entire source is used.
:param reducing_gap: Apply optimization by resizing the image
in two steps. First, reducing the image by integer times
using :py:meth:`~PIL.Image.Image.reduce`.
Second, resizing using regular resampling. The last step
changes size no less than by ``reducing_gap`` times.
``reducing_gap`` may be None (no first step is performed)
or should be greater than 1.0. The bigger ``reducing_gap``,
the closer the result to the fair resampling.
The smaller ``reducing_gap``, the faster resizing.
With ``reducing_gap`` greater or equal to 3.0, the result is
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The default value is None (no optimization).
:returns: An :py:class:`~PIL.Image.Image` object.
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Returns a copy of the image reduced ``factor`` times.
If the size of the image is not dividable by ``factor``,
the resulting size will be rounded up.
:param factor: A greater than 0 integer or tuple of two integers
for width and height separately.
:param box: An optional 4-tuple of ints providing
the source image region to be reduced.
The values must be within ``(0, 0, width, height)`` rectangle.
If omitted or ``None``, the entire source is used.
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Returns a rotated copy of this image. This method returns a
copy of this image, rotated the given number of degrees counter
clockwise around its centre.
:param angle: In degrees counter clockwise.
:param resample: An optional resampling filter. This can be
one of :py:data:`Resampling.NEAREST` (use nearest neighbour),
:py:data:`Resampling.BILINEAR` (linear interpolation in a 2x2
environment), or :py:data:`Resampling.BICUBIC` (cubic spline
interpolation in a 4x4 environment). If omitted, or if the image has
mode "1" or "P", it is set to :py:data:`Resampling.NEAREST`.
See :ref:`concept-filters`.
:param expand: Optional expansion flag. If true, expands the output
image to make it large enough to hold the entire rotated image.
If false or omitted, make the output image the same size as the
input image. Note that the expand flag assumes rotation around
the center and no translation.
:param center: Optional center of rotation (a 2-tuple). Origin is
the upper left corner. Default is the center of the image.
:param translate: An optional post-rotate translation (a 2-tuple).
:param fillcolor: An optional color for area outside the rotated image.
:returns: An :py:class:`~PIL.Image.Image` object.
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Saves this image under the given filename. If no format is
specified, the format to use is determined from the filename
extension, if possible.
Keyword options can be used to provide additional instructions
to the writer. If a writer doesn't recognise an option, it is
silently ignored. The available options are described in the
:doc:`image format documentation
<../handbook/image-file-formats>` for each writer.
You can use a file object instead of a filename. In this case,
you must always specify the format. The file object must
implement the ``seek``, ``tell``, and ``write``
methods, and be opened in binary mode.
:param fp: A filename (string), os.PathLike object or file object.
:param format: Optional format override. If omitted, the
format to use is determined from the filename extension.
If a file object was used instead of a filename, this
parameter should always be used.
:param params: Extra parameters to the image writer.
:returns: None
:exception ValueError: If the output format could not be determined
from the file name. Use the format option to solve this.
:exception OSError: If the file could not be written. The file
may have been created, and may contain partial data.
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Seeks to the given frame in this sequence file. If you seek
beyond the end of the sequence, the method raises an
``EOFError`` exception. When a sequence file is opened, the
library automatically seeks to frame 0.
See :py:meth:`~PIL.Image.Image.tell`.
If defined, :attr:`~PIL.Image.Image.n_frames` refers to the
number of available frames.
:param frame: Frame number, starting at 0.
:exception EOFError: If the call attempts to seek beyond the end
of the sequence.
rzno more images in fileN)<01>EOFError)r<>r<>r<>r%r%r&r 
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Image.seek<65>titlecCst||d<01>dS)a<>
Displays this image. This method is mainly intended for debugging purposes.
This method calls :py:func:`PIL.ImageShow.show` internally. You can use
:py:func:`PIL.ImageShow.register` to override its default behaviour.
The image is first saved to a temporary file. By default, it will be in
PNG format.
On Unix, the image is then opened using the **xdg-open**, **display**,
**gm**, **eog** or **xv** utility, depending on which one can be found.
On macOS, the image is opened with the native Preview application.
On Windows, the image is opened with the standard PNG display utility.
:param title: Optional title to use for the image window, where possible.
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Image.show<6F>tuple[Image, ...]cCs4|<00><00>|jjdkr|<00><03>fStt|j|j<01><07><00><02>S)a<>
Split this image into individual bands. This method returns a
tuple of individual image bands from an image. For example,
splitting an "RGB" image creates three new images each
containing a copy of one of the original bands (red, green,
blue).
If you need only one band, :py:meth:`~PIL.Image.Image.getchannel`
method can be more convenient and faster.
:returns: A tuple containing bands.
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Returns an image containing a single channel of the source image.
:param channel: What channel to return. Could be index
(0 for "R" channel of "RGB") or channel name
("A" for alpha channel of "RGBA").
:returns: An image in "L" mode.
.. versionadded:: 4.3.0
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Returns the current frame number. See :py:meth:`~PIL.Image.Image.seek`.
If defined, :attr:`~PIL.Image.Image.n_frames` refers to the
number of available frames.
:returns: Frame number, starting with 0.
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Make this image into a thumbnail. This method modifies the
image to contain a thumbnail version of itself, no larger than
the given size. This method calculates an appropriate thumbnail
size to preserve the aspect of the image, calls the
:py:meth:`~PIL.Image.Image.draft` method to configure the file reader
(where applicable), and finally resizes the image.
Note that this function modifies the :py:class:`~PIL.Image.Image`
object in place. If you need to use the full resolution image as well,
apply this method to a :py:meth:`~PIL.Image.Image.copy` of the original
image.
:param size: The requested size in pixels, as a 2-tuple:
(width, height).
:param resample: Optional resampling filter. This can be one
of :py:data:`Resampling.NEAREST`, :py:data:`Resampling.BOX`,
:py:data:`Resampling.BILINEAR`, :py:data:`Resampling.HAMMING`,
:py:data:`Resampling.BICUBIC` or :py:data:`Resampling.LANCZOS`.
If omitted, it defaults to :py:data:`Resampling.BICUBIC`.
(was :py:data:`Resampling.NEAREST` prior to version 2.5.0).
See: :ref:`concept-filters`.
:param reducing_gap: Apply optimization by resizing the image
in two steps. First, reducing the image by integer times
using :py:meth:`~PIL.Image.Image.reduce` or
:py:meth:`~PIL.Image.Image.draft` for JPEG images.
Second, resizing using regular resampling. The last step
changes size no less than by ``reducing_gap`` times.
``reducing_gap`` may be None (no first step is performed)
or should be greater than 1.0. The bigger ``reducing_gap``,
the closer the result to the fair resampling.
The smaller ``reducing_gap``, the faster resizing.
With ``reducing_gap`` greater or equal to 3.0, the result is
indistinguishable from fair resampling in most cases.
The default value is 2.0 (very close to fair resampling
while still being faster in many cases).
:returns: None
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zImage.thumbnail<69>3Transform | ImageTransformHandler | SupportsGetData<74>Sequence[Any] | None<6E>fillc
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Transforms this image. This method creates a new image with the
given size, and the same mode as the original, and copies data
to the new image using the given transform.
:param size: The output size in pixels, as a 2-tuple:
(width, height).
:param method: The transformation method. This is one of
:py:data:`Transform.EXTENT` (cut out a rectangular subregion),
:py:data:`Transform.AFFINE` (affine transform),
:py:data:`Transform.PERSPECTIVE` (perspective transform),
:py:data:`Transform.QUAD` (map a quadrilateral to a rectangle), or
:py:data:`Transform.MESH` (map a number of source quadrilaterals
in one operation).
It may also be an :py:class:`~PIL.Image.ImageTransformHandler`
object::
class Example(Image.ImageTransformHandler):
def transform(self, size, data, resample, fill=1):
# Return result
Implementations of :py:class:`~PIL.Image.ImageTransformHandler`
for some of the :py:class:`Transform` methods are provided
in :py:mod:`~PIL.ImageTransform`.
It may also be an object with a ``method.getdata`` method
that returns a tuple supplying new ``method`` and ``data`` values::
class Example:
def getdata(self):
method = Image.Transform.EXTENT
data = (0, 0, 100, 100)
return method, data
:param data: Extra data to the transformation method.
:param resample: Optional resampling filter. It can be one of
:py:data:`Resampling.NEAREST` (use nearest neighbour),
:py:data:`Resampling.BILINEAR` (linear interpolation in a 2x2
environment), or :py:data:`Resampling.BICUBIC` (cubic spline
interpolation in a 4x4 environment). If omitted, or if the image
has mode "1" or "P", it is set to :py:data:`Resampling.NEAREST`.
See: :ref:`concept-filters`.
:param fill: If ``method`` is an
:py:class:`~PIL.Image.ImageTransformHandler` object, this is one of
the arguments passed to it. Otherwise, it is unused.
:param fillcolor: Optional fill color for the area outside the
transform in the output image.
:returns: An :py:class:`~PIL.Image.Image` object.
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<06> <02><06>& zImage.__transformerr6cC<01>|<00><00>|<00>|j<02>|<01><01>S)a<>
Transpose image (flip or rotate in 90 degree steps)
:param method: One of :py:data:`Transpose.FLIP_LEFT_RIGHT`,
:py:data:`Transpose.FLIP_TOP_BOTTOM`, :py:data:`Transpose.ROTATE_90`,
:py:data:`Transpose.ROTATE_180`, :py:data:`Transpose.ROTATE_270`,
:py:data:`Transpose.TRANSPOSE` or :py:data:`Transpose.TRANSVERSE`.
:returns: Returns a flipped or rotated copy of this image.
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Randomly spread pixels in an image.
:param distance: Distance to spread pixels.
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zImage.toqimagecCr<>)z$Returns a QPixmap copy of this imagerr<>r<>)r<>r<>r<>r<><00> toqpixmapr<70>r%r%r&r<><00> r<>zImage.toqpixmap<61>r1r<>)r1r<><00>r1r<>)r3r<>r1r<>r<>)NN)rr<>r<>r<>rr r1r<>)r<>rr1r))r*r<>r+r r1r,)r1r,<00>r9)r<>r<>r<>r r1rK)rX)rYr<>r1rK)r:r^r<>r<>r<>r r1r<>)r1rc) rtr<>rqrrrsrtr<>rZrur<>r1r<>)
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Used as a mixin by point transforms
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Used as a mixin by geometry transforms
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Common check to enforce type and sanity check on size tuples
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:returns: None, or raises a ValueError
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Creates a new image with the given mode and size.
:param mode: The mode to use for the new image. See:
:ref:`concept-modes`.
:param size: A 2-tuple, containing (width, height) in pixels.
:param color: What color to use for the image. Default is black.
If given, this should be a single integer or floating point value
for single-band modes, and a tuple for multi-band modes (one value
per band). When creating RGB or HSV images, you can also use color
strings as supported by the ImageColor module. If the color is
None, the image is not initialised.
:returns: An :py:class:`~PIL.Image.Image` object.
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 rr9r<>r:r^cGsrt|<01>t||<01>}|jdkr7|jdkr7|}t|<06>dkr&t|dt<06>r&|d}|dkr0|dkr0|}|<05>|||<06>|S)a<>
Creates a copy of an image memory from pixel data in a buffer.
In its simplest form, this function takes three arguments
(mode, size, and unpacked pixel data).
You can also use any pixel decoder supported by PIL. For more
information on available decoders, see the section
:ref:`Writing Your Own File Codec <file-codecs>`.
Note that this function decodes pixel data only, not entire images.
If you have an entire image in a string, wrap it in a
:py:class:`~io.BytesIO` object, and use :py:func:`~PIL.Image.open` to load
it.
:param mode: The image mode. See: :ref:`concept-modes`.
:param size: The image size.
:param data: A byte buffer containing raw data for the given mode.
:param decoder_name: What decoder to use.
:param args: Additional parameters for the given decoder.
:returns: An :py:class:`~PIL.Image.Image` object.
rrr9r%)r<>rrvrurwr<>r<>rH)rtr<>r:r<>r<>r3r`r%r%r&rH! s
rHc Gs<>t|<01>t|<04>dkrt|dt<03>r|d}|dkrS|dkr"|ddf}|dtvrSt|d<05>}|<05>t<07>|||d|<04><05>}|dkrNddl m
}|<06>
d|j <0B> d<08><01>|_ d|_|St|||||<04>S) a<>
Creates an image memory referencing pixel data in a byte buffer.
This function is similar to :py:func:`~PIL.Image.frombytes`, but uses data
in the byte buffer, where possible. This means that changes to the
original buffer object are reflected in this image). Not all modes can
share memory; supported modes include "L", "RGBX", "RGBA", and "CMYK".
Note that this function decodes pixel data only, not entire images.
If you have an entire image file in a string, wrap it in a
:py:class:`~io.BytesIO` object, and use :py:func:`~PIL.Image.open` to load it.
The default parameters used for the "raw" decoder differs from that used for
:py:func:`~PIL.Image.frombytes`. This is a bug, and will probably be fixed in a
future release. The current release issues a warning if you do this; to disable
the warning, you should provide the full set of parameters. See below for details.
:param mode: The image mode. See: :ref:`concept-modes`.
:param size: The image size.
:param data: A bytes or other buffer object containing raw
data for the given mode.
:param decoder_name: What decoder to use.
:param args: Additional parameters for the given decoder. For the
default encoder ("raw"), it's recommended that you provide the
full set of parameters::
frombuffer(mode, size, data, "raw", mode, 0, 1)
:returns: An :py:class:`~PIL.Image.Image` object.
.. versionadded:: 1.1.4
rrr9r%r<>r<>r<>r<>)r<>rwr<>r<><00> _MAPMODESrrr<><00>
map_bufferr<EFBFBD>r<>r3r!r<>r<>rH)rtr<>r:r<>r<>r3r<>r%r%r&<00>
frombufferO s$
 
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An object that has an ``__array_interface__`` dictionary.
r1<00>dict[str, Any]cCst<00><00>r<>)<01>NotImplementedErrorr<72>r%r%r&rC<00> r<>z*SupportsArrayInterface.__array_interface__N)r1r)r"r#r$r<>r<>rCr%r%r%r&r<00> sr<00>objr<6A>c
Csl|j}|d}t|<03>}|<02>dd<03>}|dur]zd|dd<03>|df}Wnty6}zd}t|<08>|<07>d}~wwzt|\}} Wnty\}z|\}
} d|
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vrfd} n |d krmd } nd } || kr<>d|<04>d| <0C>d<10>}t|<08><01>|dkr<>dn|d|df} |dur<>t|d<13>r<>|<00><08>}nt|d<14>r<>|<00> <09>}nd}t|<08><01>t
|| |d| dd<11>S)a 
Creates an image memory from an object exporting the array interface
(using the buffer protocol)::
from PIL import Image
import numpy as np
a = np.zeros((5, 5))
im = Image.fromarray(a)
If ``obj`` is not contiguous, then the ``tobytes`` method is called
and :py:func:`~PIL.Image.frombuffer` is used.
In the case of NumPy, be aware that Pillow modes do not always correspond
to NumPy dtypes. Pillow modes only offer 1-bit pixels, 8-bit pixels,
32-bit signed integer pixels, and 32-bit floating point pixels.
Pillow images can also be converted to arrays::
from PIL import Image
import numpy as np
im = Image.open("hopper.jpg")
a = np.asarray(im)
When converting Pillow images to arrays however, only pixel values are
transferred. This means that P and PA mode images will lose their palette.
:param obj: Object with array interface
:param mode: Optional mode to use when reading ``obj``. Will be determined from
type if ``None``.
This will not be used to convert the data after reading, but will be used to
change how the data is read::
from PIL import Image
import numpy as np
a = np.full((1, 1), 300)
im = Image.fromarray(a, mode="L")
im.getpixel((0, 0)) # 44
im = Image.fromarray(a, mode="RGB")
im.getpixel((0, 0)) # (44, 1, 0)
See: :ref:`concept-modes` for general information about modes.
:returns: An image object.
.. versionadded:: 1.1.6
r{<00>stridesNr<4E>r7ryzCannot handle this data typezCannot handle this data type: rx)r~r<>r<>r<>r<>r<>r8r9zToo many dimensions: z > r<>rrr"<00>tostringz1'strides' requires either tobytes() or tostring()r9) rCrwr<>r<>r<><00>_fromarray_typemaprr4r"rr<>)rrtrlr{<00>ndimr<00>typekeyr<79>r<>rg<00> typekey_shapery<00>ndmaxr<78>r%r%r&<00> fromarray<61> sL/ 
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r cCr<>)z-Creates an image instance from a QImage imagerr<>r<>)r<>r<>r<>r<><00>
fromqimage<EFBFBD>r3r<>r<>r%r%r&r <00> r<>r cCr<>)z.Creates an image instance from a QPixmap imagerr<>r<>)r<>r<>r<>r<><00> fromqpixmapr r%r%r&r<00> r<>r)r<>z|b1)r~z1;8)r<><00>|u1)r<>r<>)r<>z|i1)r<>zI;8)r<>z<u2)r<>r<>)r<>z>u2)r<>r<>)r<>z<i2)r<>zI;16S)r<>z>i2)r<>zI;16BS)r<>z<u4)r<>zI;32)r<>z>u4)r<>zI;32B)r<>z<i4)r<>zI;32S)r<>z>i4)r<>zI;32BS)r<>z<f4)r<>zF;32F)r<>z>f4)r<>zF;32BF)r<>z<f8)r<>zF;64F)r<>z>f8)r<>zF;64BF))rrr7r)r<>r<>))rrr8r)r<>r<>))rrr9r)r<>r<>r<><00>i4)r<>r<><00>f4)r<>r<>cCs|tdurdStd|d<00>td|d<00>}|dtkr)d|<01>ddt<00>d<06>}t|<02><01>|tkr<t<03>d|<01>dt<00>d<06>t<05>dSdS)Nrrr7z Image size (z pixels) exceeds limit of z0 pixels, could be decompression bomb DOS attack.)r,rNr(r@rAr )r<><00>pixelsr<73>r%r%r&r<> s <02><08><04>r<EFBFBD><00>rrr<><00> Literal['r']<5D>formats<74>"list[str] | tuple[str, ...] | None<6E>ImageFile.ImageFilec s<>|dkrdt|<01><01><00>}t|<03><01>t|tj<04>rd}t|<03><01>|dur"t}n t|ttf<02>s/d}t|<03><01>d<06>d}t |<00>r@t
j <0B> t
<EFBFBD> |<00><01>}|rKt<0E>|d<08>}d <09>nttt|<00>}z|<00>d
<EFBFBD>Wnttjfynt<03>|<00><17><00>}d <09>Ynw|<00>d <0B>}t<18>g<00>d<1B><01>fdd<17> }|||||<02>}|dur<>|tur<>t<05><19><00>t<1A>r<>||||t<07>fdd<19>|D<00><01><01>}|r<><72>|_|S<00>r<>|<00><1C><00>D]}t<1D>|<08>q<>d|r<>|n|}t|<03><01>)a<>
Opens and identifies the given image file.
This is a lazy operation; this function identifies the file, but
the file remains open and the actual image data is not read from
the file until you try to process the data (or call the
:py:meth:`~PIL.Image.Image.load` method). See
:py:func:`~PIL.Image.new`. See :ref:`file-handling`.
:param fp: A filename (string), os.PathLike object or a file object.
The file object must implement ``file.read``,
``file.seek``, and ``file.tell`` methods,
and be opened in binary mode. The file object will also seek to zero
before reading.
:param mode: The mode. If given, this argument must be "r".
:param formats: A list or tuple of formats to attempt to load the file in.
This can be used to restrict the set of formats checked.
Pass ``None`` to try all supported formats. You can print the set of
available formats by running ``python3 -m PIL`` or using
the :py:func:`PIL.features.pilinfo` function.
:returns: An :py:class:`~PIL.Image.Image` object.
:exception FileNotFoundError: If the file cannot be found.
:exception PIL.UnidentifiedImageError: If the image cannot be opened and
identified.
:exception ValueError: If the ``mode`` is not "r", or if a ``StringIO``
instance is used for ``fp``.
:exception TypeError: If ``formats`` is not ``None``, a list or a tuple.
rz bad mode zKStringIO cannot be used to open an image. Binary data must be used instead.Nzformats must be a list or tupleFr<46><00>rbTr<00>r<00> IO[bytes]r<00> str | bytes<65>prefixrKr<00>list[str] | tuple[str, ...]r1<00>ImageFile.ImageFile | Nonec
s<>|D]n}|<04><00>}|tvrt<02>z0t|\}}| p||<02>}t|t<04>r(<28><01>|<07>n|r>|<00>d<01>|||<01>}t|j<08>|WSWqt t
t t j fyc} ztrY<72><01>|dt| <09><00>WYd} ~ qd} ~ wtyp<00>ro|<00><10><00>wdS)Nrz opening failed. )r<>rgr<>r<>r<>rPr r<>r<><00> SyntaxError<6F>
IndexErrorr<EFBFBD><00>struct<63>errorr*<00> BaseExceptionr)
rrrrr<><00>factory<72>acceptr<r3r<>)<02> exclusive_fp<66>warning_messagesr%r&<00>
_open_corex s2 
 



<04><14> <02>zopen.<locals>._open_corec3s<00>|] }|<01>vr|VqdSr<>r%)r<>r<>)<01>checked_formatsr%r&r<><00> s<02>zopen.<locals>.<genexpr>zcannot identify image file %r)
rrrrrrKrrr1r) <20>reprrr<>r-<00>StringIOrfr<>r<>r<>rrr<>r<>r<>r<>r rrrKr r<><00>UnsupportedOperationr.r
r<>rr<>r
rr@rAr) rrtrr<>rrr(r3<00>messager%)r)r&r'r&r / sb" <02> <02>
<04> r <00>im1<6D>im2cCs&|<00><00>|<01><00>|<00>t<02>|j|j<04><02>S)z<>
Alpha composite im2 over im1.
:param im1: The first image. Must have mode RGBA.
:param im2: The second image. Must have mode RGBA, and the same size as
the first image.
:returns: An :py:class:`~PIL.Image.Image` object.
)rrr<>r8r3)r.r/r%r%r&r8<00> s
r8rrMcCs(|<00><00>|<01><00>|<00>t<02>|j|j|<02><03>S)a<>
Creates a new image by interpolating between two input images, using
a constant alpha::
out = image1 * (1.0 - alpha) + image2 * alpha
:param im1: The first image.
:param im2: The second image. Must have the same mode and size as
the first image.
:param alpha: The interpolation alpha factor. If alpha is 0.0, a
copy of the first image is returned. If alpha is 1.0, a copy of
the second image is returned. There are no restrictions on the
alpha value. If necessary, the result is clipped to fit into
the allowed output range.
:returns: An :py:class:`~PIL.Image.Image` object.
)rrr<><00>blendr3)r.r/rr%r%r&r0<00> sr0<00>image1<65>image2r(cCs|<01><00>}|<03>|d|<02>|S)af
Create composite image by blending images using a transparency mask.
:param image1: The first image.
:param image2: The second image. Must have the same mode and
size as the first image.
:param mask: A mask image. This image can have mode
"1", "L", or "RGBA", and must have the same size as the
other two images.
N)rr4)r1r2r(rXr%r%r&<00> composite<74> s r3cGs|<00>|d<00>S)a<>
Applies the function (which should take one argument) to each pixel
in the given image. If the image has more than one band, the same
function is applied to each band. Note that the function is
evaluated once for each possible pixel value, so you cannot use
random components or other generators.
:param image: The input image.
:param function: A function object, taking one integer argument.
:returns: An :py:class:`~PIL.Image.Image` object.
r)rB)rXr<>r%r%r&<00>eval<61> s r4rx<00>Sequence[Image]cCs<>t|<00>t|<01>ks d|vrd}t|<02><01>|dd<04>D]}|jt|<00>kr'd}t|<02><01>|j|djkr5d}t|<02><01>q|D]}|<03><06>q8|d<00>tj |gdd <09>|D<00><01>R<00><00>S)
am
Merge a set of single band images into a new multiband image.
:param mode: The mode to use for the output image. See:
:ref:`concept-modes`.
:param bands: A sequence containing one single-band image for
each band in the output image. All bands must have the
same size.
:returns: An :py:class:`~PIL.Image.Image` object.
<20>*zwrong number of bandsrNz mode mismatchrz size mismatchcSsg|]}|j<00>qSr%)r3)r<>r0r%r%r&r<>szmerge.<locals>.<listcomp>)
r<EFBFBD>rwrrtr<>r<>rrr<>r<>)rtrxr<>r<>r%r%r&r<><00> s <02>
&r<>r$r$<00>7Callable[[IO[bytes], str | bytes], ImageFile.ImageFile]r%<00>$Callable[[bytes], bool | str] | NonecCs*|<00><00>}|tvr t<01>|<00>||ft|<dS)a1
Register an image file plugin. This function should not be used
in application code.
:param id: An image format identifier.
:param factory: An image file factory method.
:param accept: An optional function that can be used to quickly
reject images having another format.
N)r<>rfrPrg)r$r$r%r%r%r&<00> register_opens
r9<00>mimetypecC<01>|t|<00><01><dS)a<>
Registers an image MIME type by populating ``Image.MIME``. This function
should not be used in application code.
``Image.MIME`` provides a mapping from image format identifiers to mime
formats, but :py:meth:`~PIL.ImageFile.ImageFile.get_format_mimetype` can
provide a different result for specific images.
:param id: An image format identifier.
:param mimetype: The image MIME type for this format.
N)rir<>)r$r:r%r%r&<00> register_mime+s r<<00>driver<65>/Callable[[Image, IO[bytes], str | bytes], None]cCr;)z<>
Registers an image save function. This function should not be
used in application code.
:param id: An image format identifier.
:param driver: A function to save images in this format.
N)rjr<><00>r$r=r%r%r&<00> register_save:s
r@cCr;)z<>
Registers an image function to save all the frames
of a multiframe format. This function should not be
used in application code.
:param id: An image format identifier.
:param driver: A function to save images in this format.
N)rkr<>r?r%r%r&<00>register_save_allGs rA<00> extensioncCs|<00><00>t|<01><02><dS)z<>
Registers an image extension. This function should not be
used in application code.
:param id: An image format identifier.
:param extension: An extension used for this format.
N)r<>rlr<>)r$rBr%r%r&<00>register_extensionU<00>rC<00>
extensionscCs|D]}t||<02>qdS)z<>
Registers image extensions. This function should not be
used in application code.
:param id: An image format identifier.
:param extensions: A list of extensions used for this format.
N)rC)r$rErBr%r%r&<00>register_extensions`s <04>rFcCs
t<00>tS)za
Returns a dictionary containing all file extensions belonging
to registered plugins
)r<>rlr%r%r%r&<00>registered_extensionslsrGrYr<><00>type[ImageFile.PyDecoder]cC<01> |t|<dS)z<>
Registers an image decoder. This function should not be
used in application code.
:param name: The name of the decoder
:param decoder: An ImageFile.PyDecoder object
.. versionadded:: 4.1.0
N)rm)rYr<>r%r%r&<00>register_decoderur<>rJr<><00>type[ImageFile.PyEncoder]cCrI)z<>
Registers an image encoder. This function should not be
used in application code.
:param name: The name of the encoder
:param encoder: An ImageFile.PyEncoder object
.. versionadded:: 4.1.0
N)rn)rYr<>r%r%r&<00>register_encoder<65>r<>rLrXrcKs"ddlm}|j|fi|<01><01>dS)Nr)<01> ImageShow)r<>rMr<>)rXrrMr%r%r&r<><00>s r<><00>extentr<74><00>qualitycCst<00><00>t<02>|||<02><03>S)a
Generate a Mandelbrot set covering the given extent.
:param size: The requested size in pixels, as a 2-tuple:
(width, height).
:param extent: The extent to cover, as a 4-tuple:
(x0, y0, x1, y1).
:param quality: Quality.
)r<>rr<><00>effect_mandelbrot)r<>rNrOr%r%r&rP<00>s rP<00>sigmacCst<00><00>t<02>||<01><02>S)z<>
Generate Gaussian noise centered around 128.
:param size: The requested size in pixels, as a 2-tuple:
(width, height).
:param sigma: Standard deviation of noise.
)r<>rr<><00> effect_noise)r<>rQr%r%r&rR<00>rDrRcC<01>t<00><00>t<02>|<00><01>S)zl
Generate 256x256 linear gradient from black to white, top to bottom.
:param mode: Input mode.
)r<>rr<><00>linear_gradientr<74>r%r%r&rT<00><00>rTcCrS)zm
Generate 256x256 radial gradient from black to white, centre to edge.
:param mode: Input mode.
)r<>rr<><00>radial_gradientr<74>r%r%r&rV<00>rUrV<00>env<6E>dict[str, str] | Nonec
Cs<>|dur|ntj}dtjfdtjfdtjffD]d\}}||vr q||<00><06>}d}dD]\}}|<04>|<06>r>|}|dt|<06> <00>}q*zt |<04>|}Wnt
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y{} zt <0B> |<02>d| <09><00><03>WYd} ~ qd} ~ wwdS)N<>PILLOW_ALIGNMENT<4E>PILLOW_BLOCK_SIZE<5A>PILLOW_BLOCKS_MAXr))r<>i)rziz is not intz: ) r<00>environr<6E><00> set_alignment<6E>set_block_size<7A>set_blocks_maxr<78>rrwr<>rr@rA)
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d d <0A>Z dd<0F>Z d1dd<11>Z dd<13>Zd2d3dd<1A>Zdd<1C>Zd4dd<1F>Zd5d!d"<22>Zd6d#d$<24>Zd%d&<26>Zd7d(d)<29>Zd4d*d+<2B>Zd8d-d.<2E>Zd/d0<64>ZdS)9r<39>a
This class provides read and write access to EXIF image data::
from PIL import Image
im = Image.open("exif.png")
exif = im.getexif() # Returns an instance of this class
Information can be read and written, iterated over or deleted::
print(exif[274]) # 1
exif[274] = 2
for k, v in exif.items():
print("Tag", k, "Value", v) # Tag 274 Value 2
del exif[274]
To access information beyond IFD0, :py:meth:`~PIL.Image.Exif.get_ifd`
returns a dictionary::
from PIL import ExifTags
im = Image.open("exif_gps.jpg")
exif = im.getexif()
gps_ifd = exif.get_ifd(ExifTags.IFD.GPSInfo)
print(gps_ifd)
Other IFDs include ``ExifTags.IFD.Exif``, ``ExifTags.IFD.Makernote``,
``ExifTags.IFD.Interop`` and ``ExifTags.IFD.IFD1``.
:py:mod:`~PIL.ExifTags` also has enum classes to provide names for data::
print(exif[ExifTags.Base.Software]) # PIL
print(gps_ifd[ExifTags.GPS.GPSDateStamp]) # 1999:99:99 99:99:99
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