Source code for pystellibs.kurucz
import numpy as np
from .stellib import AtmosphereLib
from .config import libsdir
from .simpletable import SimpleTable
try:
from astropy.io import fits as pyfits
except ImportError:
import pyfits
[docs]class Kurucz(AtmosphereLib):
"""
The stellar atmosphere models by Castelli and Kurucz 2004 or ATLAS9
* LTE
* PP
* line blanketing
"""
def __init__(self, *args, **kwargs):
self.name = 'Kurucz 2004'
self.source = libsdir + '/kurucz2004.grid.fits'
self._load_()
AtmosphereLib.__init__(self, *args, **kwargs)
def _load_(self):
with pyfits.open(self.source) as f:
# load data
self._getWaveLength_(f)
self._getTGZ_(f)
self._getSpectra_(f)
self._getWaveLength_units(f)
def _getWaveLength_units(self, f):
self.wavelength_unit = 'angstrom'
def _getWaveLength_(self, f):
self._wavelength = f[0].data[-1]
def _getTGZ_(self, f):
self.grid = SimpleTable(f[1].data)
self.grid.header.update(f[1].header.items())
self.grid.header['NAME'] = 'TGZ'
def _getSpectra_(self, f):
self.spectra = f[0].data[:-1]
[docs] def bbox(self, dlogT=0.05, dlogg=0.25):
""" Boundary of Kurucz 2004 library
Parameters
----------
dlogT: float
log-temperature tolerance before extrapolation limit
dlogg: float
log-g tolerance before extrapolation limit
Returns
-------
bbox: ndarray
(logT, logg) edges of the bounding polygon
"""
bbox = [(3.54406 - dlogT, 5.000 + dlogg),
(3.55403 - dlogT, 0.000 - dlogg),
(3.778, 0.000 - dlogg),
(3.778 + dlogT, 0.000),
(3.875 + dlogT, 0.500),
(3.929 + dlogT, 1.000),
(3.954 + dlogT, 1.500),
(4.146, 2.000 - dlogg),
(4.146 + dlogT, 2.000),
(4.279 + dlogT, 2.500),
(4.415 + dlogT, 3.000),
(4.491 + dlogT, 3.500),
(4.591 + dlogT, 4.000),
(4.689 + dlogT, 4.500),
(4.699 + dlogT, 5.000 + dlogg),
(3.544 - dlogT, 5.000 + dlogg) ]
return np.array(bbox)
@property
def logT(self):
return self.grid['logT']
@property
def logg(self):
return self.grid['logg']
@property
def Teff(self):
return self.grid['Teff']
@property
def Z(self):
return self.grid['Z']
@property
def logZ(self):
return self.grid['logz']