synthesizer.photoionisation.cloudy17¶
Given an SED (from an SPS model, for example), generate a cloudy atmosphere grid. Can optionally generate an array of input files for selected parameters.
Functions
- synthesizer.photoionisation.cloudy17.convert_cloudy_wavelength(x)[source]¶
Convert a cloudy wavelength string (e.g. 6562.81A, 1.008m) to a wavelength float in units of angstroms.
- Parameters:
x (str) – A cloudy wavelength string
- Returns:
- float
The wavelength in Angstroms
- synthesizer.photoionisation.cloudy17.create_cloudy_input(model_name, shape_commands, abundances, output_dir='./', **kwargs)[source]¶
A generic function for creating a cloudy input file
- Parameters:
model_name (str) – The model name. Used in the naming of the outputs
shape_commands (list) – List of strings describing the cloudy input commands
abundances – (Abundances object) A synthsizer Abundances object
output_dir (str) – The output dir
- Returns:
- list
A list of cloudy commands
- synthesizer.photoionisation.cloudy17.read_continuum(filename, return_dict=False)[source]¶
Extract just the spectra from a cloudy.cont file
- Parameters:
filename (str) – The cloudy filename
- Returns:
- lam (array-like, float)
The wavelength grid
- nu (array-like, float)
The frequency grid
- incident (array-like, float)
The incident spectrum
- transmitted (array-like, float)
The transmitted spectrum
- nebular (array-like, float)
The nebular spectrum
- nebular_continuum (array-like, float)
The nebular continuum spectrum
- total (array-like, float)
The total spectrum
- linecont (array-like, float)
The line contribution spectrum
alternatively returns a dictionary
- synthesizer.photoionisation.cloudy17.read_linelist(filename, extension='elin')[source]¶
- Parameters:
filename (str) – The cloudy filename
extension (str) – The extension of the file
- Returns:
- line_ids (list)
A list of line identificaitons
- wavelengths (list)
A list of the line wavelengths
- luminosities (list)
A list of the luminosities
- synthesizer.photoionisation.cloudy17.read_lines(filename, extension='lines')[source]¶
Read a full line list from a cloudy output file.
- Parameters:
filename (str) – The cloudy filename
extension (str) – The extension of the file
- Returns:
- line_ids (list)
A list of line identificaitons
- blends (list)
A list containing flags whether the line is a blend
- wavelengths (list)
A list of the line wavelengths
- intrinsic (list)
A list of the intrinsic luminosities
- emergent (list)
A list of emergent luminosities
- synthesizer.photoionisation.cloudy17.read_wavelength(filename)[source]¶
Extract just the wavelength grid from cloudy .cont file and reverse the order
- Parameters:
filename (str) – The cloudy filename
- Returns:
- ndnarray
The wavelength grid
Classes
- class synthesizer.photoionisation.cloudy17.ShapeCommands[source]¶
A class for holding different cloudy shape commands
- cloudy_agn(aox=-1.4, auv=-0.5, ax=-1.35)[source]¶
A function for specifying the cloudy AGN model. See 6.2 Hazy1.pdf.
- Parameters:
model_name (str) – User defined name of the model used for cloudy inputs and outputs
TBB (float) – The Big Bump temperature
aox (float) – The x-ray slope (default value from Calabro CEERS AGN model)
auv (float) – The uv-slope (default value from Calabro CEERS AGN model)
ax (float) – Slope normalisation
- Returns:
- list
a list of strings with the cloudy input commands
- table_sed(lam, lnu, output_dir='./')[source]¶
A function for creating a cloudy input file using a tabulated SED.
TODO: allow the user to instead specify nu and to automatically convert units if provided
- Parameters:
model_name (str) – User defined name of the model used for cloudy inputs and outputs.
lam (array or unyt_array) – Wavelength grid with or without units (via unyt)
lnu (array) – Spectral luminosity density
output_dir (str) – Output directory path
- Returns:
- list
a list of strings with the cloudy input commands