Spectra
Spectrum
Bases: SimpleSpectrum
A simple spectrum class using wavelengths and weights.
UML
Attributes:
Name | Type | Description |
---|---|---|
wavelengths |
(Array, metres)
|
The array of wavelengths at which the spectrum is defined. |
weights |
Array
|
The relative weights of each wavelength. |
Source code in src/dLux/spectra.py
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__init__(wavelengths, weights=None)
Parameters:
Name | Type | Description | Default |
---|---|---|---|
wavelengths
|
(Array, metres)
|
The array of wavelengths at which the spectrum is defined. |
required |
weights
|
Array = None
|
The relative weights of each wavelength. Input weights are automatically normalised to a sum of 1. |
None
|
Source code in src/dLux/spectra.py
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normalise()
Returns a normalised spectrum object, where the weights are normalised to a sum of 1.
Returns:
Name | Type | Description |
---|---|---|
spectrum |
Spectrum
|
The spectrum object with the normalised spectrum. |
Source code in src/dLux/spectra.py
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PolySpectrum
Bases: SimpleSpectrum
Implements a generic polynomial spectrum, such as a linear spectrum.
This implements a polynomial as follows: f(x) = c0 + c1x + c2x^2 + ... + cn*x^n
UML
Attributes:
Name | Type | Description |
---|---|---|
wavelengths |
(Array, metres)
|
The array of wavelengths at which the spectrum is defined. |
coefficients |
Array
|
The array of polynomial coefficient values. |
Source code in src/dLux/spectra.py
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|
weights: Array
property
Gets the relative spectral weights by evaluating the polynomial function at the internal wavelengths. Output weights are automatically normalised to a sum of 1.
Returns:
Name | Type | Description |
---|---|---|
weights |
Array
|
The normalised relative weights of each wavelength. |
__init__(wavelengths, coefficients)
Parameters:
Name | Type | Description | Default |
---|---|---|---|
wavelengths
|
(Array, metres)
|
The array of wavelengths at which the spectrum is defined. |
required |
coefficients
|
Array
|
The array of polynomial coefficient values. |
required |
Source code in src/dLux/spectra.py
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normalise()
Calculated weights are automatically normalised, so this method simply returns an unmodified object.
Returns:
Name | Type | Description |
---|---|---|
spectrum |
Spectrum
|
The unmodified spectrum object |
Source code in src/dLux/spectra.py
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