Integer, Intent (In)	::	n, wtype, ns, fcall
Integer, Intent (Inout)	::	ifail
Real (Kind=nag_wp), Intent (In)	::	x(n)
Real (Kind=nag_wp), Intent (Inout)	::	window, slo, shi, rcomm(ns+20)
Real (Kind=nag_wp), Intent (Out)	::	smooth(ns), t(ns)

C Header Interface

#include <nag.h>

void	g10bbf_ (const Integer n, const double x[], const Integer wtype, double window, double slo, double shi, const Integer ns, double smooth[], double t[], const Integer fcall, double rcomm[], Integer ifail)

The routine may be called by the names g10bbf or nagf_smooth_kerndens_gauss.

3 Description

Given a sample of

n

observations,

x_{1}, x_{2}, \dots, x_{n}

, from a distribution with unknown density function,

f (x)

, an estimate of the density function,

\hat{f} (x)

, may be required. The simplest form of density estimator is the histogram. This may be defined by:

\hat{f} (x) = \frac{1}{n h} n_{j}, a + (j - 1) h < x < a + j h, j = 1, 2, \dots, n_{s},

where

n_{j}

is the number of observations falling in the interval

a + (j - 1) h

a + j h

a

is the lower bound to the histogram,

b = n_{s} h

is the upper bound and

n_{s}

is the total number of intervals. The value

h

is known as the window width. To produce a smoother density estimate a kernel method can be used. A kernel function,

K (t)

, satisfies the conditions:

\int_{- \infty}^{\infty} K (t) d t = 1 and K (t) \geq 0 .

The kernel density estimator is then defined as

\hat{f} (x) = \frac{1}{n h} \sum_{i = 1}^{n} K (\frac{x - x_{i}}{h}) .

The choice of

K

is usually not important but to ease the computational burden use can be made of the Gaussian kernel defined as

K (t) = \frac{1}{\sqrt{2 π}} e^{- t^{2} / 2} .

The smoothness of the estimator depends on the window width

h

. The larger the value of

h

the smoother the density estimate. The value of

h

can be chosen by examining plots of the smoothed density for different values of

h

or by using cross-validation methods (see Silverman (1990)).

Silverman (1982) and Silverman (1990) show how the Gaussian kernel density estimator can be computed using a fast Fourier transform (FFT). In order to compute the kernel density estimate over the range

a

b

the following steps are required.

(i)Discretize the data to give $n_{s}$ equally spaced points $t_{l}$ with weights $ξ_{l}$ (see Jones and Lotwick (1984)).
(ii)Compute the FFT of the weights $ξ_{l}$ to give $Y_{l}$ .
(iii)Compute $ζ_{l} = e^{- \frac{1}{2} h^{2} s_{l}^{2}} Y_{l}$ where $s_{l} = 2 π l / (b - a)$ .
(iv)Find the inverse FFT of $ζ_{l}$ to give $\hat{f} (x)$ .

To compute the kernel density estimate for further values of

h

only steps (iii) and (iv) need be repeated.

4 References

Jones M C and Lotwick H W (1984) Remark AS R50. A remark on algorithm AS 176. Kernel density estimation using the Fast Fourier Transform Appl. Statist. 33 120–122

Silverman B W (1982) Algorithm AS 176. Kernel density estimation using the fast Fourier transform Appl. Statist. 31 93–99

Silverman B W (1990) Density Estimation Chapman and Hall

5 Arguments

1: $n$ – Integer Input

On entry:

n

, the number of observations in the sample.

fcall = 0

, n must be unchanged since the last call to g10bbf.

Constraint:

n > 0

2: $x (n)$ – Real (Kind=nag_wp) array Input

On entry:

x_{i}

, for

i = 1, 2, \dots, n

fcall = 0

, x must be unchanged since the last call to g10bbf.

3: $wtype$ – Integer Input

On entry: how the window width,

h

, is to be calculated:

$wtype = 1$

h

is supplied in window.

$wtype = 2$

h

is to be calculated from the data, with

h = m \times (\frac{0.9 \times \min (q_{75} - q_{25}, σ)}{n^{0.2}})

where

q_{75} - q_{25}

is the inter-quartile range and

σ

the standard deviation of the sample,

x

, and

m

is a multipler supplied in window. The

25 %

and

75 %

quartiles,

q_{25}

and

q_{75}

, are calculated using g01amf. This is the "rule-of-thumb" suggested by Silverman (1990).

Suggested value:

wtype = 2

and

window = 1.0

Constraint:

wtype = 1

2

4: $window$ – Real (Kind=nag_wp) Input/Output

On entry: if

wtype = 1

, then

h

, the window width. Otherwise,

m

, the multiplier used in the calculation of

h

Suggested value:

window = 1.0

and

wtype = 2

On exit:

h

, the window width actually used.

Constraint:

window > 0.0

5: $slo$ – Real (Kind=nag_wp) Input/Output

On entry: if

slo < shi

then

a

, the lower limit of the interval on which the estimate is calculated. Otherwise,

a

and

b

, the lower and upper limits of the interval, are calculated as follows:

\begin{matrix} a & = & \min_{i} \{x_{i}\} - slo \times h \\ b & = & \max_{i} \{x_{i}\} + slo \times h \end{matrix}

where

h

is the window width.

For most applications

a

should be at least three window widths below the lowest data point.

fcall = 0

, slo must be unchanged since the last call to g10bbf.

Suggested value:

slo = 3.0

and

shi = 0.0

which would cause

a

and

b

to be set

3

window widths below and above the lowest and highest data points respectively.

On exit:

a

, the lower limit actually used.

6: $shi$ – Real (Kind=nag_wp) Input/Output

On entry: if

slo < shi

then

b

, the upper limit of the interval on which the estimate is calculated. Otherwise a value for

b

is calculated from the data as stated in the description of slo and the value supplied in shi is not used.

For most applications

b

should be at least three window widths above the highest data point.

fcall = 0

, shi must be unchanged since the last call to g10bbf.

On exit:

b

, the upper limit actually used.

7: $ns$ – Integer Input

On entry:

n_{s}

, the number of points at which the estimate is calculated.

fcall = 0

, ns must be unchanged since the last call to g10bbf.

Suggested value:

ns = 512

Constraint:

ns \geq 2

8: $smooth (ns)$ – Real (Kind=nag_wp) array Output

On exit:

\hat{f} (t_{l})

, for

l = 1, 2, \dots, n_{s}

, the

n_{s}

values of the density estimate.

9: $t (ns)$ – Real (Kind=nag_wp) array Output

On exit:

t_{l}

, for

l = 1, 2, \dots, n_{s}

, the points at which the estimate is calculated.

10: $fcall$ – Integer Input

On entry: if

fcall = 1

then the values of

Y_{l}

are to be calculated by this call to g10bbf, otherwise it is assumed that the values of

Y_{l}

were calculated by a previous call to this routine and the relevant information is stored in rcomm.

Constraint:

fcall = 0

1

11: $rcomm (ns + 20)$ – Real (Kind=nag_wp) array Communication Array

On entry: communication array, used to store information between calls to g10bbf.

fcall = 0

, rcomm must be unchanged since the last call to g10bbf.

On exit: the last ns elements of rcomm contain the fast Fourier transform of the weights of the discretized data, that is

rcomm (l + 20) = Y_{l}

, for

l = 1, 2, \dots, n_{s}

12: $ifail$ – Integer Input/Output

On entry: ifail must be set to

0

- 1 or 1

. If you are unfamiliar with this argument you should refer to Section 4 in the Introduction to the NAG Library FL Interface for details.

For environments where it might be inappropriate to halt program execution when an error is detected, the value

- 1 or 1

is recommended. If the output of error messages is undesirable, then the value

1

is recommended. Otherwise, because for this routine the values of the output arguments may be useful even if

ifail \neq 0

on exit, the recommended value is

- 1

. When the value $- 1 or 1$ is used it is essential to test the value of ifail on exit.

On exit:

ifail = 0

unless the routine detects an error or a warning has been flagged (see Section 6).

6 Error Indicators and Warnings

If on entry

ifail = 0

- 1

, explanatory error messages are output on the current error message unit (as defined by x04aaf).

Errors or warnings detected by the routine:

Note: in some cases g10bbf may return useful information.

$ifail = 11$: On entry, $n = 〈value〉$ .
Constraint: $n > 0$ .

$ifail = 12$: On entry, $n = 〈value〉$ .
On entry at previous call, $n = 〈value〉$ .
Constraint: if $fcall = 0$ , n must be unchanged since previous call.

$ifail = 31$: On entry, $wtype = 〈value〉$ .
Constraint: $wtype = 1$ or $2$ .

$ifail = 41$: On entry, $window = 〈value〉$ .
Constraint: $window > 0.0$ .

$ifail = 51$: On entry, $slo = 〈value〉$ .
On exit from previous call, $slo = 〈value〉$ .
Constraint: if $fcall = 0$ , slo must be unchanged since previous call.

$ifail = 61$: On entry, $slo = 〈value〉$ and $shi = 〈value〉$ .
On entry, $\min (x) = 〈value〉$ and $\max (x) = 〈value〉$ .
Expected values of at least $〈value〉$ and $〈value〉$ for slo and shi.
slo should be at least three window widths below the lowest data point or shi should be at least three window widths above the highest data point. All output values have been returned.

$ifail = 62$: On entry, $shi = 〈value〉$ .
On exit from previous call, $shi = 〈value〉$ .
Constraint: if $fcall = 0$ , shi must be unchanged since previous call.

$ifail = 71$: On entry, $ns = 〈value〉$ .
Constraint: $ns \geq 2$ .

$ifail = 74$: On entry, $ns = 〈value〉$ .
On entry at previous call, $ns = 〈value〉$ .
Constraint: if $fcall = 0$ , ns must be unchanged since previous call.

$ifail = 101$: On entry, $fcall = 〈value〉$ .
Constraint: $fcall = 0$ or $1$ .

$ifail = 111$: rcomm has been corrupted between calls.

$ifail = - 99$: An unexpected error has been triggered by this routine. Please contact NAG.
See Section 7 in the Introduction to the NAG Library FL Interface for further information.

$ifail = - 399$: Your licence key may have expired or may not have been installed correctly.
See Section 8 in the Introduction to the NAG Library FL Interface for further information.

$ifail = - 999$: Dynamic memory allocation failed.
See Section 9 in the Introduction to the NAG Library FL Interface for further information.

7 Accuracy

See Jones and Lotwick (1984) for a discussion of the accuracy of this method.

8 Parallelism and Performance

g10bbf is threaded by NAG for parallel execution in multithreaded implementations of the NAG Library.

g10bbf makes calls to BLAS and/or LAPACK routines, which may be threaded within the vendor library used by this implementation. Consult the documentation for the vendor library for further information.

Please consult the X06 Chapter Introduction for information on how to control and interrogate the OpenMP environment used within this routine. Please also consult the Users' Note for your implementation for any additional implementation-specific information.

9 Further Comments

The time for computing the weights of the discretized data is of order

n

, while the time for computing the FFT is of order

n_{s} \log (n_{s})

, as is the time for computing the inverse of the FFT.

10 Example

Data is read from a file and the density estimated. The first

20

values are then printed.

This plot shows the estimated density function for the example data for several window widths.

NAG Library Manual, Mark 27

Interfaces: FL CL AD

NAG FL Interface Introduction

G10 (Smooth) Chapter Contents

G10 (Smooth) Chapter Introduction

g10bb: FL CL AD

NAG FL Interfaceg10bbf (kerndens_​gauss)

▸▿ Contents

1 Purpose

2 Specification

3 Description

4 References

5 Arguments

6 Error Indicators and Warnings

7 Accuracy

8 Parallelism and Performance

9 Further Comments

10 Example

10.1 Program Text

10.2 Program Data

10.3 Program Results

NAG FL Interface
g10bbf (kerndens_gauss)