.. _further_examples:

===================
Further Examples
===================
Additional Jupyter notebooks with tutorials to produce the plots shown
in the SPISEA paper (`Hosek et al. (2020)
<https://ui.adsabs.harvard.edu/abs/2020arXiv200606691H/abstract>`_) can be found `here
<https://github.com/astropy/SPISEA/tree/main/docs/paper_examples>`_.

Figure 2: HR-Diagrams with Different Evolution Models; CMDs with different Extinction Laws
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.. figure:: images/iso_comp_example.png
	    :align: center


Figure 3: CMDs in Different Filters at Different Metallicities
----------------------------------------------------------------------------
.. figure:: images/iso_cmd_example.png
	    :align: center

Figure 4: Clusters with Multiplicity vs. Differential Extinction
--------------------------------------------------------------------
.. figure:: images/cluster_cmd_example.png
	    :align: center

Figure 5: Clusters with Different IMFs: Luminosity Function + BH Mass Function
--------------------------------------------------------------------------------------------------------------------

.. figure:: images/imf_comp_example.png
	    :align: center


Figure 6: Wolf-Rayet Star Populations with Different Evolution Models
---------------------------------------------------------------------
.. figure:: images/WRstars_example.png
	    :align: center
		    
Figure 7: Unresolved Cluster Spectra at Different Ages
----------------------------------------------------------
.. figure:: images/clust_unresolved_example.png
	    :align: center