Uses of Interface
vec_math.Function

Packages that use Function

astro
astro.fits
jview
stella.ccd
stella.jview
stella.parameter
stella.sql
stella.util
vec_math

Uses of Function in astro

Classes in astro that implement Function

class	JulianDate The julian date converts java time stamps into jd and vice versa via its inverse function.
class	ModifiedJulianDate The julian date converts java time stamps into jd and vice versa via its inverse function.
class	TruncatedJulianDate The julian date converts java time stamps into jd and vice versa via its inverse function.

Fields in astro declared as Function

private Function[]

SpectralFits.wavelength The wavelength solution for the orders, parsed from the header.

Methods in astro that return Function

protected abstract Function[]

SpectralFits.parseWavelengthSolution(nom.tam.fits.Header h) Parses the wavelength soultion from the header.

Uses of Function in astro.fits

Classes in astro.fits that implement Function

static class

Gl586.DiffMag Function to get the differences in the Δm in to wavelength as a function of Temperature of the main star and ΔT to the second, according to

Methods in astro.fits with parameters of type Function

private static double[]	Overscan.getBestOverscanModel(int s0, Vector2D[] ovscn, double[] exp, Function legendre, double[] average, int window, int min, int overlap, int max, double rms) From the exponential and the Legendre fit on one hand, and from the running average on the other hand, we decide which fit is best to model the overscan.
private static int	Overscan.searchCrossing(int row, int width, Function legendre, double[] expsolve, double rms) Starting from the row given, we scan at most overlap rows to the top and bottom, searching for the index where the exponential fit and the Legendre fit cross.
static GeneralLinearRegression	Overscan.setupFit(Function[] legendre, int min, int max, Vector2D[] adu) Converts an adu with the fit axis on the first index plus the fitting functions into a general linear regression.
static nom.tam.fits.Fits	FitsTools.transform(nom.tam.fits.Fits image, Function eval) Extracts ADU's from an Image HDU, transforms them according to the given function f(ADU), and constructs an Image HDU of likewise type.
static nom.tam.fits.ImageHDU	FitsTools.transform(nom.tam.fits.ImageHDU in, Function eval) Extracts ADU's from an Image HDU, transforms them according to the given function f(ADU), and constructs an Image HDU of likewise type.

Uses of Function in jview

Fields in jview declared as Function

private Function	JSliderProperty.convert The conversion of displayed slider value to property value.
private Function	JDataModelDisplay.efunc Transfer function for err(y), normally d(yfunc)/d(y).
private Function	JDataModelDisplay.rfunc Transfer function for residuals.
private Function	JDataModelDisplay.yfunc Transfer function for y.

Fields in jview with type parameters of type Function

private List<Function>

JAbstractAnalyser.transfer If set, we use these functions to transfer set data to analyser input.

Constructors in jview with parameters of type Function

JSliderProperty(PropertySupplying p, String k, Class<?> v, Function f)
Creates a jslider property.

Uses of Function in stella.ccd

Fields in stella.ccd with type parameters of type Function

private Map<String,Function>	WifsipMaster.colortable Additional correction to focus star and the color of focus star.
private Map<String,Function>	WifsipMaster.exposuretable The exposure time from the focus star and filter.

Uses of Function in stella.jview

Classes in stella.jview that implement Function

private static class	SesFits.Dispersion The functions used in a single order, parsed from s tring buffer.
static class	SesFits.Wavelength This class represents a soultion to an aperture.

Fields in stella.jview declared as Function

private Function

SesFits.Dispersion.lambda

Fields in stella.jview with type parameters of type Function

private List<Function>

SesFits.Wavelength.f

Methods in stella.jview that return Function

protected Function[]

SesFits.parseWavelengthSolution(nom.tam.fits.Header h) Parses the wavelength soultion from the header.

Uses of Function in stella.parameter

Classes in stella.parameter that implement Function

static class

SerialValue.DewarPressure Dewar pressure conversion function.

Fields in stella.parameter declared as Function

private Function	SerialValue.convert The function to calculate the true value out of the reading.
private Function	TargetFunction.z The function we evaluate.

Fields in stella.parameter with type parameters of type Function

private Map<String,Function>

FlatExposureTime.luxtime The expressions on how we calculate from lux to exposure time.

Methods in stella.parameter that return Function

private Function

TargetFunction.extractFunction(TargetDefinition star) From a target, we rty to extract the function.

Uses of Function in stella.sql

Fields in stella.sql declared as Function

private static Function

TargetInfo.MAGDRAW

Method parameters in stella.sql with type arguments of type Function

void	OffLimitAlarm.addDone(List<String> donelist, List<String> doneas, Map<String,Function> f, String add, Date now) Retrieve and cache all information for the date in question.
void	OffLimitAlarm.addEnvironment(List<String> envlist, List<String> envas, Map<String,Function> f, Date now) Retrieve and cache all information for the date in question.
void	OffLimitAlarm.addJoint(List<String> jointlist, List<String> jointas, Map<String,Function> f, String add, Date now) Retrieve and cache all information for the date in question.
void	OffLimitAlarm.addObs(List<String> obslist, List<String> obsas, Map<String,Function> f, String add, Date now) Retrieve and cache all information for the date in question.
Map<String,List<DataCard>>	NightlyStatistic.getDone(List<String> col, List<String> as, Map<String,Function> f, String add, Date around)
Map<String,List<DataCard>>	NightlyStatistic.getDone(List<String> col, List<String> as, Map<String,Function> f, String add, Date around, double hset, double hrise) Returns the queried columns from the done table as mapping from 'retreived-as' columns to list of doubles.If the timestamp is queried via the start column, this is converted to a Double holding the ms since 1970.
Map<String,List<DataCard>>	NightlyStatistic.getEnvironment(List<String> col, List<String> as, Map<String,Function> f, Date around) Returns the named environement column as a list of doubles.
Map<String,List<DataCard>>	NightlyStatistic.getEnvironment(List<String> col, List<String> as, Map<String,Function> f, Date around, double hset, double hrise) Returns the named environement column as a list of doubles.
Map<String,List<DataCard>>	NightlyStatistic.getJoint(List<String> col, List<String> as, Map<String,Function> f, String add, Date around)
Map<String,List<DataCard>>	NightlyStatistic.getJoint(List<String> col, List<String> as, Map<String,Function> f, String add, Date around, double hset, double hrise) Returns the queried columns from the done and obs table as mapping from 'retreived-as' columns to list of doubles.
Map<String,List<DataCard>>	NightlyStatistic.getJoint(List<String> col, Map<String,Function> f, String add, Date around)
Map<String,List<DataCard>>	NightlyStatistic.getObs(List<String> col, List<String> as, Map<String,Function> f, String add, Date around)
Map<String,List<DataCard>>	NightlyStatistic.getObs(List<String> col, List<String> as, Map<String,Function> f, String add, Date around, double hset, double hrise) Returns the queried columns from the obs table as mapping from 'retreived-as' columns to list of doubles.
private Map<String,List<DataCard>>	NightlyStatistic.parseToMap(String id, String datekey, List<String> query, List<String> as, Map<String,Function> f, String table, String where) We parse a result set to a mapping of column names to doubles.

Uses of Function in stella.util

Fields in stella.util declared as Function

private Function	Annulus.xosc Oscillatory function in x.
private Function	Annulus.yosc Oscillatory function in y.

Uses of Function in vec_math

Subinterfaces of Function in vec_math

interface	Derivative A function that also calculates it first derivative.
interface	Differentiable A function that also allows calculating of some of its derivatives.
interface	Inverse An inverse function can calculate its argument from the function value.

Classes in vec_math that implement Function

class	Chebyshev The recursive formular for the Legendre polynomials.
class	CubicSpline Cubic spline interpolation.
class	ExpressionFunction A function from a parseable string expression.
class	Harmonics A function generating oscilatory function plus overtones.
class	IdentFunction Delivers the argument.
class	Legendre The recursive formular for the Legendre polynomials.
static class	Phasing.PhaseFunction This is the function version of it.
class	Polynom A representation of a polynomial of the form
static class	PowerSpectrum.BartlettWindow The Bartlett window function.
static class	PowerSpectrum.SquareWindow The Rectangular window function.
static class	PowerSpectrum.WelchWindow The Welch window function.
class	RecursivePolynom A recursive polynom, like Chebyshev or Legendre, are defined by a minimum and maximum of the parameter space plus the coefficients.
static class	RecursivePolynom.Constant The zero-order recursive polynom is a constant.
static class	RecursivePolynom.Linear The first-order recursive polynom is linear.
private static class	SimpleVectorIntegration.InnerIntegrand
private static class	SimpleVectorIntegration.TrivialMultidimensional
class	StepFunction A function that is piecewise constant.

Fields in vec_math declared as Function

private Function[]	GeneralLinearRegression.basef The basic functions, needed for evaluating the GLR at non-data x.
(package private) Function	AbstractDataModel.LocalM.rho

Methods in vec_math with parameters of type Function

protected Matrix	GeneralLinearRegression.deriveDesignMatrix(Function[] base, VectorG xi) Calculates the design matrix from the basic functions and the measurement times.
static double	GaussianLegendreIntegration.gaussianQuadrature(Function f, double from, double to) Convenience method for integrating a function only once.
static double	GaussianLegendreIntegration.gaussianQuadrature(Function f, double from, double to, int n)
double	GaussianLegendreIntegration.getIntegral(Function f, double from, double to) Integrates the specified function from x1 to x2 using the number of sampling points specified at construct.
static double	GaussianLegendreIntegration.integrate(Function f, double[] xi, double[] wi) Integrates the specified function with the use of the pre-calculated weights and abscissas.
static double	Statistic.kolmogorovSmirnovDistance(double[] d, Function cdf) Returns the Kolmogorov-Smirnov distance against a known cumulative distribution function.
static VectorG	PowerSpectrum.periodogram(VectorG data, int m, int k, Function window) Does a periodogram of equally sampled data points.
boolean	GeneralLinearRegression.setBasicFunctions(Function[] fitting, VectorG t) Daugther classes must interfere here.
static VectorG	PowerSpectrum.simple(VectorG data, Function window) Simple periodogramm with no error estimates.
static double	Math2.zeroBisection(Function f, double xplus, double xminus, double acc, int nmax) Uses bisection to find a root of the Function f in the intervals with given accuracy.

Constructors in vec_math with parameters of type Function

AbstractDataModel.LocalM(Function f, DataModel fit, double[] yvec, double[] sigvec)

Bootstrap(Function[] fitting, VectorG x, VectorG y, VectorG sigma)
Constructs a new bootstrap object from the supplied basic functions and the measurement with their errors.

GeneralLinearRegression(Function[] fitting, VectorG x, VectorG y, VectorG sigma)
Constructs a new general linear regression.