vice.yields.ccsne.NKT13
=======================

Nomoto, Kobayashi & Tominaga (2013), ARA&A, 51, 457 core collapse supernova
yields

**Signature**: from vice.yields.ccsne import NKT13

.. versionadded:: 1.2.0

Importing this module will automatically set the CCSN yield settings for all
elements to the IMF-averaged yields calculated with the Nomoto, Kobayashi &
Tominaga (2013) yield table for [M/H] = 0.15 stars. This will adopt an upper
mass limit of 40 :math:`M_\odot`.

We provide core collapse supernova yields for non-rotating progenitors as
reported Nomoto, Kobayashi & Tominaga (2013) at metallicities relative to
solar of :math:`\log_{10}(Z / Z_\odot)` =

	- -inf
	- -1.15
	- -0.54
	- -0.24
	- 0.15
	- 0.55

assuming :math:`Z_\odot` = 0.014 according to Asplund et al. (2009) [1]_.

.. tip:: By importing this module, the user does not sacrifice the ability to
	specify their yield settings directly.

.. note:: This module is not imported with a simple ``import vice`` statement.

.. note:: When this module is imported, the yields will be updated with a
	maximum of 10^5 bins in quadrature to decrease computational overhead. For
	some elements, the yield calculation may not converge. To rerun the yield
	calculation with higher numerical precision, simply call ``set_params``
	with a new value for the keyword ``Nmax`` (see below).

Contents
--------
set_params : <function>
	Update the parameters with which the yields are calcualted.

.. [1] Asplund et al. (2009), ARA&A, 47, 481




.. toctree::
	:titlesonly:
	:maxdepth: 5

	vice.yields.ccsne.NKT13.set_params