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%matplotlib
import matplotlib.pyplot as plt
import numpy as np
from StellarSpectra.grid_tools import HDF5Interface
import h5py
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hdf5 = h5py.File("../../data/Gl51/Gl51.hdf5", "r")
fl = hdf5["fls"][:]
#ind = (fl >= 0)
wl = hdf5["wls"][:]
sigma = hdf5["sigmas"][:]
masks = hdf5["masks"][:]
#low = fl - sigma
#high = fl + sigma
hdf5.close()
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masks
Out[4]:
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plt.fill_between(wl, low, high)
#plt.plot(wl,fl)
plt.show()
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from StellarSpectra.spectrum import DataSpectrum
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myDataSpectrum = DataSpectrum.open("../../data/Gl51/Gl51.hdf5")
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print(myDataSpectrum.wls)
print(myDataSpectrum.masks)
myDataSpectrum.wls[myDataSpectrum.masks]
Out[15]:
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plt.plot(myDataSpectrum.wls[0], myDataSpectrum.fls[0])
#plt.ylim(0, 2e-13)
plt.show()
In [76]:
myInterface = HDF5Interface("../../libraries/PHOENIX_SPEX_2300.hdf5")
wl = myInterface.wl
fl = myInterface.load_flux({"temp":2300, "logg":4.5, "Z":-0.5, "alpha":0.0})
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plt.plot(wl, fl)
plt.show()
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HDF5InterfaceLA = HDF5Interface("../../libraries/PHOENIX_SPEX_2300.hdf5")
fullModelLA = Model(myDataSpectrum, myInstrument, HDF5InterfaceLA, stellar_tuple=("temp",
"logg", "Z", "vsini", "vz", "logOmega"), cheb_tuple=("c1", "c2", "c3"), cov_tuple=("sigAmp",
"logAmp", "l"), region_tuple=("loga", "mu", "sigma"))
modelLA = fullModelLA.OrderModels[0]
wl = myDataSpectrum.wls[0]
print(wl[3118:3125])
print(base[3118:3125])
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params = {"temp":3000, "logg":4.5, "Z":-0.5, "vsini":0., "vz":0, "logOmega":0.}
fullModelLA.update_Model(params)
base = modelLA.get_spectrum()
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fl = HDF5InterfaceLA.load_flux({"temp":3000, "logg":4.5, "Z":-0.5, "alpha":0.0})
wl_inter = HDF5InterfaceLA.wl
plt.plot(wl_inter, fl)
plt.show()