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casa::FluxCalcLogFreqPolynomial Class Reference

FluxCalcLogFreqPolynomial: Implementation base class for flux standards which are polynomials of log10(frequency). More...

#include <FluxCalcLogFreqPolynomial.h>

Inheritance diagram for casa::FluxCalcLogFreqPolynomial:
casa::FluxCalcQS casa::FluxCalcLogFreqBrokenPolynomial casa::FluxStdBaars casa::FluxStdPerley90 casa::FluxStdPerleyTaylor95 casa::FluxStdPerleyButler2010 casa::FluxStdPerleyButler2013 casa::FluxStdPerleyTaylor99

List of all members.

Public Types

typedef RigidVector< Float, 3 > RVF3
 Some abbreviations, since the classes derived from this have to define many polynomial coefficients.
typedef RigidVector< Float, 4 > RVF4
typedef RigidVector< Float, 5 > RVF5

Public Member Functions

virtual Bool operator() (Flux< Double > &value, Flux< Double > &error, const MFrequency &mfreq)
 Set the log10(frequency) polynomial coefficients for calculating the flux density and its uncertainty, and the unit (typically "MHz" or "GHz") that the coefficients assume.
virtual Bool setSource (const String &sourceName)
 Sets srcEnum_p = srcNameToEnum(sourceName), and returns srcEnum_p != FCQS::UNKNOWN_SOURCE.
void setFreqUnit (const String &freqUnit)
template<Int lford, Int errord>
void fill_coeffs (const RigidVector< Float, lford > &lfrv, const RigidVector< Float, errord > &errrv)
 Functions for setting up coeffs_p by taking a bunch of numbers (packaged in RigidVectors) and formatting them into coeffs_p.
template<Int lford>
void fill_coeffs (const RigidVector< Float, lford > &lfrv)
 Like fill_coeffs(lfrv, errrv), but it only takes the flux density coefficients, and substitutes an empty Vector for the error coefficients.
void fill_coeffs (const Vector< Float > &lfv)

Private Member Functions

virtual Bool setSourceCoeffs ()=0

Private Attributes

RigidVector< Vector< Float >, 2 > coeffs_p
 The first element of this pair of Vectors is a Vector of coefficients for the flux density polynomial (of log10(frequency)).
String freqUnit_p
 The frequency unit (e.g.

Detailed Description

FluxCalcLogFreqPolynomial: Implementation base class for flux standards which are polynomials of log10(frequency).

Intended use:

Public interface

Prerequisite

Etymology

From "flux density", "calculator", "log10(frequency)", and "polynomial".

Synopsis

The FluxCalcLogFreqPolynomial class provides machinery to compute total flux densities for specified non-variable sources where the flux density is well described by a low order polynomial of log(frequency).

Example

Motivation

Encapsulate the machinery for most of the flux density standards in one class.

The flux standards for cm astronomy are deliberately chosen to be distant, non-varying, and bright around 1 GHz. Since such objects tend to be dominated by synchrotron radiation their flux density is usually described by a polynomial of log(frequency).

Definition at line 79 of file FluxCalcLogFreqPolynomial.h.


Member Typedef Documentation

Some abbreviations, since the classes derived from this have to define many polynomial coefficients.

Definition at line 83 of file FluxCalcLogFreqPolynomial.h.

Definition at line 84 of file FluxCalcLogFreqPolynomial.h.

Definition at line 85 of file FluxCalcLogFreqPolynomial.h.


Member Function Documentation

template<Int lford, Int errord>
void casa::FluxCalcLogFreqPolynomial::fill_coeffs ( const RigidVector< Float, lford > &  lfrv,
const RigidVector< Float, errord > &  errrv 
)

Functions for setting up coeffs_p by taking a bunch of numbers (packaged in RigidVectors) and formatting them into coeffs_p.

Takes a RigidVector for the flux density coefficients and second one for the uncertainty coefficients, and fills coeffs_p with them.

template<Int lford>
void casa::FluxCalcLogFreqPolynomial::fill_coeffs ( const RigidVector< Float, lford > &  lfrv)

Like fill_coeffs(lfrv, errrv), but it only takes the flux density coefficients, and substitutes an empty Vector for the error coefficients.

virtual Bool casa::FluxCalcLogFreqPolynomial::operator() ( Flux< Double > &  value,
Flux< Double > &  error,
const MFrequency mfreq 
) [virtual]

Set the log10(frequency) polynomial coefficients for calculating the flux density and its uncertainty, and the unit (typically "MHz" or "GHz") that the coefficients assume.

Note that errcoeffs does not have to have the same number of terms as lfcoeffs, or any terms at all, and that each term in its polynomial is (errcoeff[order] * pow(log10(freq), order))**2. FluxCalcLogFreqPolynomial(const String& freqUnit, const Vector<Double>& lfcoeffs, const Vector<Double>& errcoeffs);

Set value and error with the expected flux density and its uncertainty (0.0 if unknown) at mfreq.

Implements casa::FluxCalcQS.

Reimplemented in casa::FluxCalcLogFreqBrokenPolynomial.

virtual Bool casa::FluxCalcLogFreqPolynomial::setSource ( const String sourceName) [virtual]

Sets srcEnum_p = srcNameToEnum(sourceName), and returns srcEnum_p != FCQS::UNKNOWN_SOURCE.

Reimplemented from casa::FluxCalcQS.

virtual Bool casa::FluxCalcLogFreqPolynomial::setSourceCoeffs ( ) [private, pure virtual]

Member Data Documentation

The first element of this pair of Vectors is a Vector of coefficients for the flux density polynomial (of log10(frequency)).

The second element is for estimating the flux density's uncertainty with a similar polynomial, but each term is (coeff * log10(freq))**2. It does not need to have the same number of coefficients as the first element, or even any coefficients. Both Vectors start with the 0th order term.

Definition at line 128 of file FluxCalcLogFreqPolynomial.h.

The frequency unit (e.g.

"MHz" or "GHz") assumed by coeffs_p.

Definition at line 131 of file FluxCalcLogFreqPolynomial.h.


The documentation for this class was generated from the following file: