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import astropy.table as tab | |
import matplotlib.pyplot as plt | |
if __name__ == "__main__": | |
# read in the data | |
f95_table = tab.Table.read("f95_data_for_Ben.fits") | |
f89_table = tab.Table.read("f89_data_for_Ben.fits") | |
# first, f95 | |
f95_fig = plt.figure(figsize=(16.42, 4.49)) | |
plt.subplot(311) | |
plt.plot(f95_table["MEANMJDOBS"], f95_table["JAPERMAG3"], "b.", ms=3) | |
plt.ylim(16.7, 16) | |
plt.ylabel("J") | |
plt.axvline(56201, alpha=0.33) | |
plt.axvline(56357, alpha=0.33) | |
plt.subplot(312) | |
plt.plot(f95_table["MEANMJDOBS"], f95_table["HAPERMAG3"], "g.", ms=3) | |
plt.ylim(14.6, 14.1) | |
plt.ylabel("H") | |
plt.axvline(56201, alpha=0.33) | |
plt.axvline(56357, alpha=0.33) | |
plt.subplot(313) | |
plt.plot(f95_table["MEANMJDOBS"], f95_table["KAPERMAG3"], "r.", ms=3) | |
plt.ylim(13.2, 12.7) | |
plt.ylabel("K") | |
plt.axvline(56201, alpha=0.33) | |
plt.axvline(56357, alpha=0.33) | |
plt.xlabel("Modified Julian Date") | |
plt.savefig("fig_f95_for_Ben.pdf") | |
plt.savefig("fig_f95_for_Ben.png") | |
# next, f89, which never has J data. | |
f89_fig = plt.figure(figsize=(13.65, 3.09)) | |
plt.subplot(211) | |
plt.plot(f89_table["MEANMJDOBS"], f89_table["HAPERMAG3"], "g.", ms=3) | |
plt.ylim(15, 12) | |
plt.ylabel("H") | |
plt.subplot(212) | |
plt.plot(f89_table["MEANMJDOBS"], f89_table["KAPERMAG3"], "r.", ms=3) | |
plt.ylim(11.2, 8.7) | |
plt.ylabel("K") | |
plt.xlabel("Modified Julian Date") | |
plt.savefig("fig_f89_for_Ben.pdf", bbox_inches='tight') | |
plt.savefig("fig_f89_for_Ben.png", bbox_inches='tight') |
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