In [1]:
import batman
import numpy as np
import matplotlib.pyplot as plt
% matplotlib inline

In [2]:
params = batman.TransitParams()
params.t0 = 0.                       #time of inferior conjunction
params.per = 1.                      #orbital period
params.rp = 0.1                      #planet radius (in units of stellar radii)
params.a = 15.                       #semi-major axis (in units of stellar radii)
params.inc = 87.                     #orbital inclination (in degrees)
params.ecc = 0.                      #eccentricity
params.w = 90.                       #longitude of periastron (in degrees)
params.u = [0.1, 0.3]                #limb darkening coefficients
params.limb_dark = "quadratic"       #limb darkening model

In [3]:
t = np.linspace(-0.05, 0.05, 100)

In [4]:
m = batman.TransitModel(params, t)    #initializes model
flux = m.light_curve(params)          #calculates light curve

In [5]:
plt.plot(t, flux)
plt.xlabel("Time from central transit")
plt.ylabel("Relative flux")
plt.ylim((0.989, 1.001))
plt.savefig("lc.png")
plt.show()



In [ ]:
params = batman.TransitParams()
params.t0 = 0.0                       #time of inferior conjunction
params.per = 1.63                      #orbital period
params.rp = 0.01                      #planet radius (in units of stellar radii)
params.a = 16.0                       #semi-major axis (in units of stellar radii)
params.inc = 87.                     #orbital inclination (in degrees)
params.ecc = 0.0                      #eccentricity
params.w = 90.0                       #longitude of periastron (in degrees)
params.u = [0.1, 0.3]                #limb darkening coefficients
params.limb_dark = "quadratic"

In [ ]:
t = np.linspace(-0.05, 0.05, 100)
m = batman.TransitModel(params, t)    #initializes model
flux = m.light_curve(params)

In [ ]:
plt.title("GJ 1132 b")
plt.plot(t, flux)
plt.xlabel("Time from central transit")
plt.ylabel("Relative flux")
plt.ylim((0.989, 1.001))
plt.savefig("lc.png")
plt.show()