Note
Go to the end to download the full example code.
Plot spectra example¶
This example demonstrates how to extract a spectra directly from a grid and plots all the available spectra.
NOTE: this only works on 2D grids at the moment
![plot spectra](../../_images/sphx_glr_plot_spectra_001.png)
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 21.49
log10(Bolometric luminosity/erg/s):36.84609875911521----------
/opt/hostedtoolcache/Python/3.10.14/x64/lib/python3.10/site-packages/unyt/array.py:1824: RuntimeWarning: divide by zero encountered in log10
out_arr = func(np.asarray(inp), out=out_func, **kwargs)
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 24.41
log10(Bolometric luminosity/erg/s):36.166199101822286----------
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 24.44
log10(Bolometric luminosity/erg/s):36.59752277341082----------
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 21.39
log10(Bolometric luminosity/erg/s):36.487843672084175----------
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 24.44
log10(Bolometric luminosity/erg/s):36.84716642614972----------
----------
SUMMARY OF SED
Number of wavelength points: 9244
Wavelength range: [0.00 Å, 299293000000.00 Å]
log10(Peak luminosity/erg/(Hz*s)): 23.26
log10(Bolometric luminosity/erg/s):36.39658434503608----------
import argparse
import matplotlib.pyplot as plt
import numpy as np
from synthesizer.grid import Grid
if __name__ == "__main__":
# Get the location of this script, __file__ is the absolute path of this
# script, however we just want to directory
# script_path = os.path.abspath(os.path.dirname(__file__))
# define the test grid dir
# test_grid_dir = script_path + "/../../tests/test_grid/"
test_grid_dir = "../../tests/test_grid/"
# initialise argument parser
parser = argparse.ArgumentParser(
description=(
"Create a plot of all spectra types for a given metallicity and \
age"
)
)
# The name of the grid. Defaults to the test grid.
parser.add_argument(
"-grid_name",
"--grid_name",
type=str,
required=False,
default="test_grid",
)
# The path to the grid directory. Defaults to the test grid directory.
parser.add_argument(
"-grid_dir",
"--grid_dir",
type=str,
required=False,
default=test_grid_dir,
)
# The target metallicity. The code function will find the closest
# metallicity and report it back. The rationale behind this is
# that this code can easily be adapted to explore other grids.
parser.add_argument(
"-metallicity", type=float, required=False, default=0.01
)
# The target log10(age/yr). The code function will find the closest
# metallicity and report it back. The rationale behind this is that
# this code can easily be adapted to explore other grids.
parser.add_argument("-log10age", type=float, required=False, default=6.0)
# Get dictionary of arguments
args = parser.parse_args()
# initialise grid
grid = Grid(args.grid_name, grid_dir=args.grid_dir)
# get the grid point for this log10age and metallicity
grid_point = grid.get_grid_point((args.log10age, args.metallicity))
# loop over available spectra and plot
for spec_name in grid.available_spectra:
# get Sed object
sed = grid.get_spectra(grid_point, spectra_id=spec_name)
# print summary of SED object
print(sed)
plt.plot(
np.log10(sed.lam),
np.log10(sed.lnu),
lw=1,
alpha=0.8,
label=spec_name,
)
plt.xlim([2.0, 4.0])
plt.ylim([18.0, 23])
plt.legend(fontsize=8, labelspacing=0.0)
plt.xlabel(r"$\rm log_{10}(\lambda/\AA)$")
plt.ylabel(r"$\rm log_{10}(L_{\nu}/erg\ s^{-1}\ Hz^{-1} M_{\odot}^{-1})$")
plt.show()
Total running time of the script: (0 minutes 0.266 seconds)