Psfs¤
PSF
dLux.psfs.PSF
¤
Bases: Base
A simple class that holds the state of a PSF as it is transformed by detector layers.
UML

Attributes:
| Name | Type | Description |
|---|---|---|
data |
Array
|
The PSF as it is transformed by the detector. |
pixel_scale |
Array
|
The pixel scale of the PSF. |
npixels |
(int, property)
|
Derived property from |
ndim |
(int, property)
|
Derived property from |
Source code in dLux/psfs.py
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ndim
property
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Returns the number of dimensions of the PSF. This is used to track the vectorised version of the PSF returned from vmapping.
Returns:
| Name | Type | Description |
|---|---|---|
ndim |
int
|
The dimensionality of the PSF. |
npixels
property
¤
Returns the side length of the arrays currently representing the PSF.
Returns:
| Name | Type | Description |
|---|---|---|
npixels |
int
|
The number of pixels that represent the |
__add__(other)
¤
Allows arrays or PSFs to be added together. None values are ignored.
Source code in dLux/psfs.py
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__iadd__(other)
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In-place addition.
Source code in dLux/psfs.py
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__imul__(other)
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In-place multiplication.
Source code in dLux/psfs.py
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__init__(data, pixel_scale)
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Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
data
|
Array
|
The PSF to be transformed by the detector. |
required |
pixel_scale
|
Array
|
The pixel scale of the PSF. |
required |
Source code in dLux/psfs.py
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__isub__(other)
¤
In-place subtraction.
Source code in dLux/psfs.py
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__itruediv__(other)
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In-place division.
Source code in dLux/psfs.py
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__mul__(other)
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Allows arrays or PSFs to be multiplied. None values are ignored.
Source code in dLux/psfs.py
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__sub__(other)
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Allows arrays or PSFs to be subtracted. None values are ignored.
Source code in dLux/psfs.py
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__truediv__(other)
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Allows arrays or PSFs to be divided. None values are ignored.
Source code in dLux/psfs.py
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convolve(other, method='auto')
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Convolves the PSF with an input array.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
other
|
Array
|
The array to convolve with the PSF. |
required |
method
|
str = "auto"
|
The method to use for the convolution. Can be "auto", "direct", or "fft". Is "auto" by default, which calls "direct". |
'auto'
|
Returns:
| Name | Type | Description |
|---|---|---|
psf |
PSF
|
The convolved PSF. |
Source code in dLux/psfs.py
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downsample(n)
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Downsamples the PSF by a factor of n. This is done by summing the PSF pixels in n x n blocks.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
n
|
int
|
The factor by which to downsample the PSF. |
required |
Returns:
| Name | Type | Description |
|---|---|---|
psf |
PSF
|
The downsampled PSF. |
Source code in dLux/psfs.py
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flip(axis)
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Flips the PSF along the specified axes. Note we use 'ij' indexing, so axis 0 is the y-axis and axis 1 is the x-axis.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
axis
|
tuple
|
The axes along which to flip the PSF. |
required |
Returns:
| Name | Type | Description |
|---|---|---|
psf |
PSF
|
The new flipped PSF. |
Source code in dLux/psfs.py
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resize(npixels)
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Resizes the PSF via a zero-padding or cropping operation.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
npixels
|
int
|
The size to resize the PSF to. |
required |
Returns:
| Name | Type | Description |
|---|---|---|
psf |
PSF
|
The resized PSF. |
Source code in dLux/psfs.py
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rotate(angle, method='linear')
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Rotates the PSF by a given angle via interpolation.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
angle
|
float
|
The angle by which to rotate the PSF. |
required |
method
|
str = "linear"
|
The interpolation method. |
'linear'
|
Returns:
| Name | Type | Description |
|---|---|---|
psf |
PSF
|
The rotated PSF. |
Source code in dLux/psfs.py
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