Installing pyqz is best done via pip. You should then be able to import the package and check its version from within any Python shell:
In [20]:
%matplotlib inline
import pyqz
import numpy as np
From v0.8.0 onwards, the plotting functions have been placed in a distinct module, which must be import separately, if you wish to exploit them.
In [27]:
import pyqz.pyqz_plots as pyqzp
pyqz gives you easy access to specific MAPPINGS strong nebular line ratio diagnostic diagrams using pyqz.get_grid():
In [4]:
a_grid = pyqz.get_grid('[NII]/[SII]+;[OIII]/[SII]+', sampling=1)
The main parameters of the MAPPINGS simulations can be specified via the following keywords:
Pk let's you define the pressure of the simulated HII regions,struct allows you to choose between plane-parallel ('pp') and spherical ('sph') HII regions, andkappa lets you define the value of $\kappa$ (from the so-called $\kappa$-distribution).All these values must match an existing set of MAPPINGS simulations inside the pyqz.pyqzm.pyqz_grid_dir folder, or pyqz will issue an error. In other words, pyqz will never be running new MAPPINGS simulations for you.
So, if one wanted to access the MAPPINGS simulations for plane-parallel HII regions, with Maxwell-Boltzmann electron density distribution, Pk =5.0 (these are the default parameters), one should type:
In [5]:
a_grid = pyqz.get_grid('[NII]/[SII]+;[OIII]/[SII]+', struct = 'pp', Pk = 5, kappa = 'inf')
If you want to check how a given line ratio diagnostic diagram looks (and e.g. check whether the MAPPINGS grid is flat, or wrapped) for line ratios of your choice, you can use pyqz_plots.plot_grid():
In [33]:
pyqzp.plot_grid('[NII]/[OII]+;[OIII]/[OII]+', struct = 'pp', Pk = 5, kappa = 'inf')
You can check which version of MAPPINGS was used to generate the grids currently inside pyqz as follows:
In [7]:
fn = pyqz.pyqz_tools.get_MVphotogrid_fn(Pk = 5.0, calibs = 'GCZO', kappa = np.inf, struct = 'pp', sampling = 1)
info = pyqz.pyqz_tools.get_MVphotogrid_metadata(fn)
print 'MAPPINGS id: %s' % info['MV_id']
print 'Model created: %s' % info['date']
print 'Model parameters: %s' % info['params'].split(': ')[1]
An important feature of pyqz is the auto-detection of wraps in the diagnostic grids, marked with red segments in the diagram, and returned as an array by the function pyqz.check_grid().
The default MAPPINGS grids shipped with pyqz are coarse. For various reasons better explained elsewhere (see the MAPPINGS documentation), only a few abundance values have matching stellar tracks AND stellar atmospheres. Hence, only a few abundance points can be simulated in a consistent fashion.
Rather than 1) interpolating between stellar tracks and stellar atmospheres in the abundance space and 2) running extra MAPPINGS models (which would use inconsistent & interpolated input), pyqz can directly resample each diagnostic grid (using the function pyqzt.refine_MVphotogrid(), see the docs for more info). The resampling is performed in the {LogQ and Tot[O+12] vs line ratio} space for all line ratios returned by MAPPINGS using Akima splines. Resampled grids can be accessed via the sampling keyword. Diagnostic grids resampled 2x2 times are shipped in the default pyqz package and are directly accessible, e.g.:
In [34]:
pyqzp.plot_grid('[NII]/[OII]+;[OIII]/[OII]+', struct = 'pp', Pk = 5, kappa = 'inf', sampling=2)
At the core of pyqz lies pyqz.interp_qz(), which is the basic routine used to interpolate a given line ratio diagnostic grid. The function is being fed by line ratios stored inside numpy arrays, and will only return a value for line ratios landing on valid and un-wrapped regions of the grid:
In [9]:
niioii = np.array([-0.65])
oiiisii = np.array([-0.1])
z = pyqz.interp_qz('Tot[O]+12',[niioii, oiiisii],'[NII]/[OII]+;[OIII]/[SII]+',
sampling=1,struct='pp')
print 'Tot[O]+12 = %.2f' % z
# The result can be visualized using pyqz_plots.plot_grid()
pyqzp.plot_grid('[NII]/[OII]+;[OIII]/[SII]+',sampling = 1, struct='pp', data = [niioii,oiiisii], interp_data=z)
Of course, one usually wants to compute both LogQ and Tot[O+12]or gas[O+12] for a large set of strong emission line fluxes, combining the estimates from different line ratio diagnostics diagrams. This is exactly what the function pyqz.get_global_qz() allows you to do.
The function is being fed the individual line fluxes and associated errors in the form of numpy arrays and lists. ID tags for each dataset can also be given to the function (these are then used if/when saving the different diagrams to files).
In [21]:
pyqz.get_global_qz(np.array([[ 1.00e+00, 5.00e-02, 2.38e+00, 1.19e-01, 5.07e+00, 2.53e-01,
5.67e-01, 2.84e-02, 5.11e-01, 2.55e-02, 2.88e+00, 1.44e-01]]),
['Hb','stdHb','[OIII]','std[OIII]','[OII]+','std[OII]+',
'[NII]','std[NII]','[SII]+','std[SII]+','Ha','stdHa'],
['[NII]/[SII]+;[OIII]/Hb','[NII]/[OII]+;[OIII]/[SII]+'],
ids = ['NGC_1234'],
KDE_method = 'multiv',
KDE_qz_sampling = 201j,
struct = 'pp',
sampling = 1,
verbose = True)
Out[21]:
By default, all line flux errors are assumed to be gaussian, where the input std value is the 1 standard deviation. Alternatively, line fluxes can be tagged as upper-limits by setting their errors to -1.
The outcome of get_global_qz() can be visualized using pyqz_plots.plot_global_qz(), but only if KDE_pickle_loc is set in the first one. This keyword defines the location in which to save a pickle file that contains all the relevant pieces of information associated with a given function call, i.e.: the single and global KDE, the srs random realizations of the line fluxes, etc ...
In [16]:
out = pyqz.get_global_qz(np.array([[ 1.00e+00, 5.00e-02, 2.38e+00, 1.19e-01, 5.07e+00, 2.53e-01,
5.67e-01, 2.84e-02, 5.11e-01, 2.55e-02, 2.88e+00, 1.44e-01]]),
['Hb','stdHb','[OIII]','std[OIII]','[OII]+','std[OII]+',
'[NII]','std[NII]','[SII]+','std[SII]+','Ha','stdHa'],
['[NII]/[SII]+;[OIII]/Hb','[NII]/[OII]+;[OIII]/[SII]+'],
ids = ['NGC_1234'],
KDE_method = 'multiv',
KDE_qz_sampling = 201j,
KDE_pickle_loc = './examples/',
struct = 'pp',
sampling = 1,
verbose = True)
import glob
fn = glob.glob('./examples/*NGC_1234*.pkl')
# pyqz_plots.get_global_qz() takes the pickle filename as argument.
pyqzp.plot_global_qz(fn[0], show_plots=True, save_loc = './examples/', do_all_diags=True)
Users less keen on using Python extensively can alternatively feed their data to pyqz via an appropriately structured .csv file and receive another .csv file in return (as well as a numpy array):
In [24]:
import os
# The example file is shipped with pyqz, and stored here:
example_csv_file = os.path.join(pyqz.pyqzm.pyqz_dir,'tests','test_arena','example_input.csv')
print example_csv_file
# Now, feed it to the code
pyqz.get_global_qz_ff(example_csv_file,
['[NII]/[SII]+;[OIII]/Hb','[NII]/[OII]+;[OIII]/[SII]+'],
struct='pp',
KDE_method='multiv',
KDE_qz_sampling = 201j,
sampling=1)
Out[24]:
The first line of the input file must contain the name of each column, following the pyqz convention. The order itself does not matter, e.g.:
Id,[OII]+,std[OII]+,Hb,stdHb,[OIII],std[OIII],[OI],std[OI],Ha,stdHa,[NII],std[NII],[SII]+,std[SII]+
The Id (optional) can be used to add a tag (i.e. a string) to each set of line fluxes. This tag will be used in the filenames of the diagrams (if some are saved) and in the output .csv file as well.
Commented line begin with #, missing values are marked with $$$ (set with the missing_values keyword), and the decimal precision in the output file is set with decimals (default=5).
At this point, it must be stressed that pyqz.get_global_qz() can only exploit a finite set of diagnostic grids, namely:
In [19]:
pyqz.pyqzm.diagnostics.keys()
Out[19]:
These specific diagnostic diagrams are chosen to be largely flat, i.e. they are able to cleanly disentangle the influence of LogQ and Tot[O]+12. One does not need to use all the grids together. For example, if one knows that an [OII] line flux measurement is corrupted, one ought to simply use the diagnostic grids that do not rely on this line to derive the estimates of LogQ and Tot[O]+12.
Users can easily add new diagnostics to this list (defined inside pyqz_metadata.py), but will do so at their own risk.