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<a name="image.colorspace"></a>
## Color Space Conversions ##
This section includes functions for performing conversions between
different color spaces.
<a name="image.rgb2lab"></a>
### [res] image.rgb2lab([dst,] src) ###
Converts a `src` RGB image to [Lab](https://en.wikipedia.org/wiki/Lab_color_space).
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.rgb2yuv"></a>
### [res] image.rgb2yuv([dst,] src) ###
Converts a RGB image to YUV. If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.yuv2rgb"></a>
### [res] image.yuv2rgb([dst,] src) ###
Converts a YUV image to RGB. If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.rgb2y"></a>
### [res] image.rgb2y([dst,] src) ###
Converts a RGB image to Y (discard U and V).
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.rgb2hsl"></a>
### [res] image.rgb2hsl([dst,] src) ###
Converts a RGB image to [HSL](https://en.wikipedia.org/wiki/HSL_and_HSV).
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.hsl2rgb"></a>
### [res] image.hsl2rgb([dst,] src) ###
Converts a HSL image to RGB.
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.rgb2hsv"></a>
### [res] image.rgb2hsv([dst,] src) ###
Converts a RGB image to [HSV](https://en.wikipedia.org/wiki/HSL_and_HSV).
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.hsv2rgb"></a>
### [res] image.hsv2rgb([dst,] src) ###
Converts a HSV image to RGB.
If `dst` is provided, it is used to store the output
image. Otherwise, returns a new `res` Tensor.
<a name="image.rgb2nrgb"></a>
### [res] image.rgb2nrgb([dst,] src) ###
Converts an RGB image to normalized-RGB.
<a name="image.y2jet"></a>
### [res] image.y2jet([dst,] src) ###
Converts a L-levels (1 to L) greyscale image into a L-levels jet heat-map.
If `dst` is provided, it is used to store the output image. Otherwise, returns a new `res` Tensor.
This is particulary helpful for understanding the magnitude of the values of a matrix, or easily spot peaks in scalar field (like probability densities over a 2D area).
For example, you can run it as
```lua
image.display{image=image.y2jet(torch.linspace(1,10,10)), zoom=50}
```
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