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FOC_Reduction/package/overplot_IC5063.py

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2.4 KiB
Python
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#!/usr/bin/python3
import numpy as np
from astropy.io import fits
from lib.plots import overplot_pol, overplot_radio
from matplotlib.colors import LogNorm
Stokes_UV = fits.open("./data/IC5063/5918/IC5063_FOC_b0.10arcsec_c0.20arcsec.fits")
Stokes_18GHz = fits.open("./data/IC5063/radio/IC5063_18GHz.fits")
Stokes_24GHz = fits.open("./data/IC5063/radio/IC5063_24GHz.fits")
Stokes_103GHz = fits.open("./data/IC5063/radio/IC5063_103GHz.fits")
Stokes_229GHz = fits.open("./data/IC5063/radio/IC5063_229GHz.fits")
Stokes_357GHz = fits.open("./data/IC5063/radio/IC5063_357GHz.fits")
# Stokes_S2 = fits.open("./data/IC5063/POLARIZATION_COMPARISON/S2_rot_crop.fits")
Stokes_IR = fits.open("./data/IC5063/IR/u2e65g01t_c0f_rot.fits")
# levelsMorganti = np.array([1.,2.,3.,8.,16.,32.,64.,128.])
levelsMorganti = np.logspace(-0.1249, 1.97, 7) / 100.0
levels18GHz = levelsMorganti * Stokes_18GHz[0].data.max()
A = overplot_radio(Stokes_UV, Stokes_18GHz)
A.plot(levels=levels18GHz, SNRp_cut=2.0, SNRi_cut=10.0, savename="./plots/IC5063/18GHz_overplot.pdf", vec_scale=None)
levels24GHz = levelsMorganti * Stokes_24GHz[0].data.max()
B = overplot_radio(Stokes_UV, Stokes_24GHz)
B.plot(levels=levels24GHz, SNRp_cut=2.0, SNRi_cut=10.0, savename="./plots/IC5063/24GHz_overplot.pdf", vec_scale=None)
levels103GHz = levelsMorganti * Stokes_103GHz[0].data.max()
C = overplot_radio(Stokes_UV, Stokes_103GHz)
C.plot(levels=levels103GHz, SNRp_cut=2.0, SNRi_cut=10.0, savename="./plots/IC5063/103GHz_overplot.pdf", vec_scale=None)
levels229GHz = levelsMorganti * Stokes_229GHz[0].data.max()
D = overplot_radio(Stokes_UV, Stokes_229GHz)
D.plot(levels=levels229GHz, SNRp_cut=2.0, SNRi_cut=10.0, savename="./plots/IC5063/229GHz_overplot.pdf", vec_scale=None)
levels357GHz = levelsMorganti * Stokes_357GHz[0].data.max()
E = overplot_radio(Stokes_UV, Stokes_357GHz)
E.plot(levels=levels357GHz, SNRp_cut=2.0, SNRi_cut=10.0, savename="./plots/IC5063/357GHz_overplot.pdf", vec_scale=None)
# F = overplot_pol(Stokes_UV, Stokes_S2)
# F.plot(SNRp_cut=3.0, SNRi_cut=80.0, savename='./plots/IC5063/S2_overplot.pdf', norm=LogNorm(vmin=5e-20,vmax=5e-18))
G = overplot_pol(Stokes_UV, Stokes_IR, cmap="inferno")
G.plot(
SNRp_cut=2.0,
SNRi_cut=10.0,
savename="./plots/IC5063/IR_overplot.pdf",
vec_scale=None,
norm=LogNorm(Stokes_IR[0].data.max() * Stokes_IR[0].header["photflam"] / 1e3, Stokes_IR[0].data.max() * Stokes_IR[0].header["photflam"]),
cmap="inferno_r",
)