Skip to content

Instantly share code, notes, and snippets.

@Samreay
Created January 31, 2019 01:25
Show Gist options
  • Save Samreay/2af3b94f640cae3e94056762cff33df1 to your computer and use it in GitHub Desktop.
Save Samreay/2af3b94f640cae3e94056762cff33df1 to your computer and use it in GitHub Desktop.
import numpy as np
import matplotlib.pyplot as plt
def get_data(filename="OzDES_GRC_2019_01_23.fits", source='DES_AAOmega'):
from astropy.io import fits
fit = fits.open(filename)
data = fit[1].data
if source is not None:
mask = data['source'] == source
data = data[mask]
fit.close()
return np.array(data)
# Get data
data = get_data()
zs = data['z']
qops = data['flag'].astype(np.int)
# Plot redshift distribution for qop 4 and 3
b = np.linspace(0, 2, 500)
fig, axes = plt.subplots(nrows=2, figsize=(14,6), sharex=True)
for ax, q, c in zip(axes, [4,3], ["#1976D2", "#8BC34A"]):
ax.hist(zs[qops == q], histtype="step", bins=b, label="QOP %d" % q, color=c)
ax.legend(frameon=False)
ax.set_ylabel("N")
axes[1].set_xlabel("z")
fig.subplots_adjust(hspace=0.07)
fig.savefig("output.png", dpi=300, bbox_inches="tight", transparent=True)
Sign up for free to join this conversation on GitHub. Already have an account? Sign in to comment