In [1]:

    

%matplotlib inline


    

In [2]:

    

from starutils.populations import Raghavan_BinaryPopulation
pop = Raghavan_BinaryPopulation(1, n=100)
pop.save_hdf('test_raghavan.h5', overwrite=True)
pop2 = Raghavan_BinaryPopulation().load_hdf('test_raghavan.h5')


    

In [3]:

    

from starutils.populations import MultipleStarPopulation
pop = MultipleStarPopulation(1, n=100)
pop.save_hdf('test_multiple.h5', overwrite=True)
pop2 = MultipleStarPopulation().load_hdf('test_multiple.h5')


    

In [4]:

    

from starutils.populations import BGStarPopulation_TRILEGAL
ra, dec = (289.21749900000003, 47.884459999999997) #Kepler-22
pop = BGStarPopulation_TRILEGAL('kepler22b.h5', ra, dec)
pop.save_hdf('test_bg.h5', overwrite=True)
pop2 = BGStarPopulation_TRILEGAL().load_hdf('test_bgpop.h5')


    

In [5]:

    

from starutils.populations import ColormatchMultipleStarPopulation
mags = {'H': 10.211, 'J': 10.523, 'K': 10.152000000000001} #Kepler-22
pop = ColormatchMultipleStarPopulation(mags, starfield='kepler22b.h5', n=100)
pop.save_hdf('test_colormatch.h5', overwrite=True)
pop2 = ColormatchMultipleStarPopulation().load_hdf('test_colormatch.h5')


    

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