Anscombe transform explained

In statistics, the Anscombe transform, named after Francis Anscombe, is a variance-stabilizing transformation that transforms a random variable with a Poisson distribution into one with an approximately standard Gaussian distribution. The Anscombe transform is widely used in photon-limited imaging (astronomy, X-ray) where images naturally follow the Poisson law. The Anscombe transform is usually used to pre-process the data in order to make the standard deviation approximately constant. Then denoising algorithms designed for the framework of additive white Gaussian noise are used; the final estimate is then obtained by applying an inverse Anscombe transformation to the denoised data.

Definition

For the Poisson distribution the mean

m

and variance

v

are not independent:

m=v

. The Anscombe transform

A:x\mapsto2\sqrt{x+\tfrac{3}{8}}

aims at transforming the data so that the variance is set approximately 1 for large enough mean; for mean zero, the variance is still zero.

It transforms Poissonian data

x

(with mean

m

) to approximately Gaussian data of mean

2\sqrt{m+\tfrac{3}{8}}-\tfrac{1}{4m1/2

} + O\left(\tfrac\right) and standard deviation

1+O\left(\tfrac{1}{m2}\right)

. This approximation gets more accurate for larger

m

, as can be also seen in the figure.

For a transformed variable of the form

2\sqrt{x+c}

, the expression for the variance has an additional term
\tfrac{3
8

-c}{m}

; it is reduced to zero at

c=\tfrac{3}{8}

, which is exactly the reason why this value was picked.

Inversion

When the Anscombe transform is used in denoising (i.e. when the goal is to obtain from

x

an estimate of

m

), its inverse transform is also neededin order to return the variance-stabilized and denoised data

y

to the original range.Applying the algebraic inverse

A-1:y\mapsto\left(

y
2

\right)2-

3
8

usually introduces undesired bias to the estimate of the mean

m

, because the forward square-roottransform is not linear. Sometimes using the asymptotically unbiased inverse

y\mapsto\left(

y
2

\right)2-

1
8

mitigates the issue of bias, but this is not the case in photon-limited imaging, for whichthe exact unbiased inverse given by the implicit mapping

\operatorname{E}\left[2\sqrt{x+\tfrac{3}{8}}\midm\right]=2

+infty
\sum
x=0

\left(\sqrt{x+\tfrac{3}{8}}

mxe-m
x!

\right)\mapstom

should be used. A closed-form approximation of this exact unbiased inverse is

y\mapsto

1
4

y2-

1
8

+

1\sqrt{
4
3
2
} y^ - \frac y^ + \frac \sqrt y^.

Alternatives

There are many other possible variance-stabilizing transformations for the Poisson distribution. Bar-Lev and Enis report a family of such transformations which includes the Anscombe transform. Another member of the family is the Freeman-Tukey transformation

A:x\mapsto\sqrt{x+1}+\sqrt{x}.

A simplified transformation, obtained as the primitive of the reciprocal of the standard deviation of the data, is

A:x\mapsto2\sqrt{x}

which, while it is not quite so good at stabilizing the variance, has the advantage of being more easily understood.Indeed, from the delta method,

V[2\sqrt{x}]\left(

d(2\sqrt{m
)}{d

m}\right)2V[x]=\left(

1
\sqrt{m
} \right)^2 m = 1 .

Generalization

While the Anscombe transform is appropriate for pure Poisson data, in many applications the data presents also an additive Gaussian component. These cases are treated by a Generalized Anscombe transform[1] and its asymptotically unbiased or exact unbiased inverses.

See also

Notes and References

  1. Book: Starck . J.L. . Murtagh . F. . Bijaoui . A. . 1998 . Image Processing and Data Analysis . registration . 9780521599146 . Cambridge University Press.