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simple_plot.py
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141 lines (121 loc) · 4.54 KB
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import os
import glob
import numpy as np
import scipy
import matplotlib
import matplotlib.pylab as plt
import datetime
import time
import random
import astropy
from astropy.io import fits
from astropy import units as u
from astropy import table
#import bokeh.mpl
#import mpld3
plt.rcParams['figure.figsize'] = (12,8)
def plotData(NQuery, table, FigureStrBase, SurfMin=1e-1*u.M_sun/u.pc**2,
SurfMax=1e5*u.M_sun/u.pc**2, VDispMin=1e-1*u.km/u.s,
VDispMax=3e2*u.km/u.s, RadMin=1e-2*u.pc, RadMax=1e3*u.pc,):
"""
This is where documentation needs to be added
Parameters
----------
NQuery
FigureStrBase : str
The start of the output filename, e.g. for "my_file.png" it would be
my_file
SurfMin
SurfMax
VDispMin
VDispMax
RadMin
RadMax
"""
figure = plt.figure(1)
figure.clf()
ax = figure.gca()
# d = table.Table.read("merged_table.ipac", format='ascii.ipac')
d = table
Author = d['Names']
Run = d['IDs']
SurfDens = d['SurfaceDensity']
VDisp = d['VelocityDispersion']
Rad = d['Radius']
if d['IsSimulated'].dtype == 'bool':
IsSim = d['IsSimulated']
else:
IsSim = d['IsSimulated'] == 'True'
UseSurf = (SurfDens > SurfMin) & (SurfDens < SurfMax)
UseVDisp = (VDisp > VDispMin) & (VDisp < VDispMax)
UseRad = (Rad > RadMin) & (Rad < RadMax)
Use = UseSurf & UseVDisp & UseRad
Obs = (~IsSim) & Use
Sim = IsSim & Use
UniqueAuthor = set(Author[Use])
NUniqueAuthor = len(UniqueAuthor)
#print d
#print d[Use]
#print 'Authors:', UniqueAuthor
#colors = random.sample(matplotlib.colors.cnames, NUniqueAuthor)
colors = list(plt.cm.jet(np.linspace(0,1,NUniqueAuthor)))
random.shuffle(colors)
ax.loglog()
markers = ['o','s']
for iAu,color in zip(UniqueAuthor,colors) :
UsePlot = (Author == iAu) & Use
ObsPlot = ((Author == iAu) & (~IsSim)) & Use
SimPlot = ((Author == iAu) & (IsSim)) & Use
if any(ObsPlot):
ax.scatter(SurfDens[ObsPlot], VDisp[ObsPlot], marker=markers[0],
s=(np.log(np.array(Rad[ObsPlot]))-np.log(np.array(RadMin))+0.5)**3.,
color=color, alpha=0.5)
if any(SimPlot):
ax.scatter(SurfDens[SimPlot], VDisp[SimPlot], marker=markers[1],
s=(np.log(np.array(Rad[SimPlot]))-np.log(np.array(RadMin))+0.5)**3.,
color=color, alpha=0.5)
if any(Obs):
ax.scatter(SurfDens[Obs], VDisp[Obs], marker=markers[0],
s=(np.log(np.array(Rad[Obs]))-np.log(np.array(RadMin))+0.5)**3.,
facecolors='none', edgecolors='black',
alpha=0.5)
if any(Sim):
ax.scatter(SurfDens[Sim], VDisp[Sim], marker=markers[1],
s=(np.log(np.array(Rad[Sim]))-np.log(np.array(RadMin))+0.5)**3.,
facecolors='none', edgecolors='black',
alpha=0.5)
ax.set_xlabel('$\Sigma$ [M$_{\odot}$ pc$^{-2}$]', fontsize=16)
ax.set_ylabel('$\sigma$ [km s$^{-1}$]', fontsize=16)
box = ax.get_position()
ax.set_position([box.x0, box.y0, box.width * 0.8, box.height])
#html_bokeh = bokeh.mpl.to_bokeh(fig=figure, name="bokeh_"+FigureStrBase+NQuery)
#html = mpld3.fig_to_html(figure)
#with open("mpld3_"+FigureStrBase+NQuery+'.html','w') as f:
# f.write(html)
ax.set_xlim((SurfMin.to(u.M_sun/u.pc**2).value,SurfMax.to(u.M_sun/u.pc**2).value))
ax.set_ylim((VDispMin.to(u.km/u.s).value,VDispMax.to(u.km/u.s).value))
# Put a legend to the right of the current axis
ax.legend(UniqueAuthor, loc='center left', bbox_to_anchor=(1.0, 0.5), prop={'size':12}, markerscale = .7, scatterpoints = 1)
plt.show()
figure.savefig(FigureStrBase+NQuery+'.png',bbox_inches='tight',dpi=150)
figure.savefig(FigureStrBase+NQuery+'.pdf',bbox_inches='tight',dpi=150)
return FigureStrBase+NQuery+'.png'#, html, html_bokeh
def clearPlotOutput(FigureStrBase,TooOld) :
for fl in glob.glob(FigureStrBase+"*.png") + glob.glob(FigureStrBase+"*.pdf"):
now = time.time()
if os.stat(fl).st_mtime < now - TooOld :
os.remove(fl)
def timeString() :
TimeString=datetime.datetime.now().strftime("%Y%m%d%H%M%S%f")
return TimeString
# NQuery=timeString()
# FigureStrBase='Output_Sigma_sigma_r_'
# TooOld=300
#
# clearPlotOutput(FigureStrBase,TooOld)
#
# plotData(NQuery,FigureStrBase,SurfMin,SurfMax,VDispMin,VDispMax,RadMin,RadMax)
#
# #d.show_in_browser(jsviewer=True)
#
#