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