synthesizer.utils.util_funcs¶
A module containing general utility functions.
Example usage:
planck(frequency, temperature=10000 * K) rebin_1d(arr, 10, func=np.sum)
Functions
- synthesizer.utils.util_funcs.parse_grid_id(grid_id)[source]¶
Parse a grid name for the properties of the grid.
This is used for parsing a grid ID to return the SPS model, version, and IMF
- Parameters:
grid_id (str) – string grid identifier
- synthesizer.utils.util_funcs.planck(frequency, temperature)[source]¶
Compute the planck distribution for a given frequency and temperature.
This function computes the spectral radiance of a black body at a given frequency and temperature using Planck’s law. The spectral radiance is then converted to spectral luminosity density assuming a luminosity distance of 10 pc.
- Parameters:
frequency (float or unyt_quantity) – Frequency of the radiation in Hz.
temperature (float or unyt_quantity) – Temperature in Kelvin.
- Returns:
Spectral luminosity density in erg/s/Hz.
- Return type:
unyt_quantity
- synthesizer.utils.util_funcs.rebin_1d(arr, resample_factor, func=<function sum>)[source]¶
A simple function for rebinning a 1D array using a specificed function (e.g. sum or mean).
- Parameters:
arr (array-like) – The input 1D array.
resample_factor (int) – The integer rebinning factor, i.e. how many bins to rebin by.
func (func) – The function to use (e.g. mean or sum).
- Returns:
- array-like
The input array resampled by i.
- synthesizer.utils.util_funcs.value_to_array(value)[source]¶
A helper functions for converting a single value to an array holding a single value.
- Parameters:
value (float/unyt_quantity) – The value to wrapped into an array.
- Returns:
- array-like/unyt_array
An array containing the single value
- Raises:
InconsistentArguments – If the argument is not a float or unyt_quantity.
- synthesizer.utils.util_funcs.wavelength_to_rgba(wavelength, gamma=0.8, fill_red=(0, 0, 0, 0.5), fill_blue=(0, 0, 0, 0.5), alpha=1.0)[source]¶
Convert wavelength float to RGBA tuple.
Taken from https://stackoverflow.com/questions/44959955/ matplotlib-color-under-curve-based-on-spectral-color
Who originally took it from http://www.noah.org/wiki/ Wavelength_to_RGB_in_Python
- Parameters:
wavelength (float) – Wavelength in nm.
gamma (float) – Gamma value.
fill_red (bool or tuple) – The colour (RGBA) to use for wavelengths red of the visible. If None use final nearest visible colour.
fill_blue (bool or tuple) – The colour (RGBA) to use for wavelengths red of the visible. If None use final nearest visible colour.
alpha (float) – The value of the alpha channel (between 0 and 1).
- Returns:
- rgba (tuple)
RGBA tuple.