Making some plots:

NUV-M24 vs R24/Rd
R24 vs 24um Sersic index
Main sequence plot on full LIR sample

But first, import some modules...



In [7]:

    
import numpy as np
from matplotlib import pyplot as plt
%matplotlib inline
import warnings
warnings.filterwarnings('ignore')

NUV-M24 vs R24/Rd



In [13]:

    
%run ~/github/LCS/python/Python3/LCS_MS_rf_plots.py









    



normalizing by radius of disk
(1800, 1800)



In [14]:

    
g.plotNUV24_vs_sizeratio()

Why is this important?

I think I wanted to confirm that galaxies with smaller R24/Rd were more obscured. This plot confirms that statement.

We are plotting all galaxies in the galfit sample.

are NUV and M24 correlated?

Sersic Index @24um vs R_{24}



In [38]:

    
%run ~/github/LCS/python/Python3/LCS_MS_rf_plots.py









    



normalizing by radius of disk
(1800, 1800)






    





<Figure size 489.6x360 with 0 Axes>



In [39]:

    
g.plotn24_vs_R24()









    



(-0.2313164488878101, 5.07216743635945, -0.4290500018745661, 9.758050080016256)

Summary

Objects with smaller R24 (less than 0.5 pixel) have higher sersic indices (>2). These objects are unresolved.

The other sources have sersic indices consistent with disk (ignoring the collection at n=5, which indicates there was some problem fitting, perhaps contamination by a neighbor).



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