save raw flux in fits file and display
fix rebase display on main
This commit is contained in:
@@ -133,6 +133,12 @@ def plot_obs(data_array, headers, rectangle=None, shifts=None, savename=None, pl
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ax_curr.arrow(x, y, dx, dy, length_includes_head=True, width=0.1, head_width=0.3, color="g")
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ax_curr.plot([x, x], [0, data.shape[0] - 1], "--", lw=2, color="g", alpha=0.85)
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ax_curr.plot([0, data.shape[1] - 1], [y, y], "--", lw=2, color="g", alpha=0.85)
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# position of centroid
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ax_curr.plot([data.shape[1] / 2, data.shape[1] / 2], [0, data.shape[0] - 1], "--", lw=2, color="b", alpha=0.85)
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ax_curr.plot([0, data.shape[1] - 1], [data.shape[0] / 2, data.shape[0] / 2], "--", lw=2, color="b", alpha=0.85)
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cr_x, cr_y = head["CRPIX1"], head["CRPIX2"]
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# Plot WCS reference point
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ax_curr.plot([cr_x], [cr_y], "+", lw=2, color="r", alpha=0.85)
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if rectangle is not None:
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x, y, width, height, angle, color = rectangle[i]
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ax_curr.add_patch(Rectangle((x, y), width, height, angle=angle, edgecolor=color, fill=False))
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@@ -189,7 +195,7 @@ def plot_Stokes(Stokes, savename=None, plots_folder=""):
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for dataset in [stkI, stkQ, stkU]:
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dataset[np.logical_not(data_mask)] = np.nan
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wcs = WCS(Stokes[0]).deepcopy()
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wcs = WCS(Stokes["I_STOKES"]).deepcopy()
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# Plot figure
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plt.rcParams.update({"font.size": 14})
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@@ -288,6 +294,9 @@ def polarization_map(
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The figure and ax created for interactive contour maps.
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"""
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# Get data
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flux = Stokes[0].data[0].copy() * Stokes[0].header["PHOTFLAM"]
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flux_error = Stokes[0].data[1].copy() * Stokes[0].header["PHOTFLAM"]
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flux_mask = Stokes[0].data[2].astype(bool).copy()
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stkI = Stokes["I_stokes"].data.copy()
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stkQ = Stokes["Q_stokes"].data.copy()
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stkU = Stokes["U_stokes"].data.copy()
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@@ -302,6 +311,20 @@ def polarization_map(
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data_mask = np.zeros(stkI.shape).astype(bool)
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data_mask[stkI > 0.0] = True
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wcs = WCS(Stokes["I_STOKES"]).deepcopy()
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pivot_wav = Stokes["I_STOKES"].header["photplam"]
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convert_flux = Stokes["I_STOKES"].header["photflam"]
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# Get integrated flux values from sum
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I_diluted = stkI[data_mask].sum() * convert_flux
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I_diluted_err = np.sqrt(np.sum(stk_cov[0, 0][data_mask])) * convert_flux
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# Get integrated polarization values from header
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P_diluted = Stokes["I_STOKES"].header["P_int"]
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P_diluted_err = Stokes["I_STOKES"].header["sP_int"]
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PA_diluted = Stokes["I_STOKES"].header["PA_int"]
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PA_diluted_err = Stokes["I_STOKES"].header["sPA_int"]
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# Compute confidence level map
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QN, UN, QN_ERR, UN_ERR = np.full((4, stkI.shape[0], stkI.shape[1]), np.nan)
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for nflux, sflux in zip([QN, UN, QN_ERR, UN_ERR], [stkQ, stkU, np.sqrt(stk_cov[1, 1]), np.sqrt(stk_cov[2, 2])]):
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@@ -314,12 +337,8 @@ def polarization_map(
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for j in range(3):
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stk_cov[i][j][np.logical_not(data_mask)] = np.nan
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wcs = WCS(Stokes[0]).deepcopy()
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pivot_wav = Stokes[0].header["photplam"]
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convert_flux = Stokes[0].header["photflam"]
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# Plot Stokes parameters map
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if display is None or display.lower() in ["default"]:
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if display is None or display.lower() in ["pol", "polarization", "polarisation", "pol_deg", "p"]:
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plot_Stokes(Stokes, savename=savename, plots_folder=plots_folder)
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# Compute SNR and apply cuts
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@@ -363,7 +382,7 @@ def polarization_map(
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fig = plt.figure(figsize=(7 * ratiox, 7 * ratioy), layout="constrained")
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if ax is None:
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ax = fig.add_subplot(111, projection=wcs)
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ax.set(aspect="equal", fc="k")
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ax.set(aspect="equal", fc="k", xlim=(0, stkI.shape[1]), ylim=(0, stkI.shape[0]))
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# fig.subplots_adjust(hspace=0, wspace=0, left=0.102, right=1.02)
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# ax.coords.grid(True, color='white', ls='dotted', alpha=0.5)
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@@ -409,7 +428,25 @@ def polarization_map(
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ax.set_facecolor("white")
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font_color = "black"
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if display.lower() in ["i", "intensity"]:
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if display.lower() in ["f", "flux", "fluxdensity"]:
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# If no display selected, show intensity map
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display = "f"
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if flux_lim is not None:
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vmin, vmax = flux_lim
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else:
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vmin, vmax = np.max(flux[flux > 0.0]) / 2e3, np.max(flux[flux > 0.0])
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imflux, cr = flux.copy(), WCS(Stokes[0].header).wcs.crpix.astype(int)
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imflux[cr[1] - 1 : cr[1] + 2, cr[0] - 1 : cr[0] + 2] = np.nan
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im = ax.imshow(
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imflux, transform=ax.get_transform(WCS(Stokes[0].header).celestial), norm=LogNorm(vmin, vmax), aspect="equal", cmap=kwargs["cmap"], alpha=1.0
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)
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fig.colorbar(im, ax=ax, aspect=50, shrink=0.60, pad=0.025, label=r"$F_{\lambda}$ [$ergs \cdot cm^{-2} \cdot s^{-1} \cdot \AA$]")
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levelsF = np.array([0.8, 2.0, 5.0, 10.0, 20.0, 50.0]) / 100.0 * vmax
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print("Flux density contour levels : ", levelsF)
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ax.contour(flux, levels=levelsF, transform=ax.get_transform(WCS(Stokes[0].header).celestial), colors="grey", linewidths=0.5)
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ax.plot(*WCS(Stokes[1]).wcs.crpix, "g+")
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I_diluted, I_diluted_err = np.sum(flux[flux_mask]), np.sqrt(np.sum(flux_error[flux_mask] ** 2))
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elif display.lower() in ["i", "intensity"]:
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# If no display selected, show intensity map
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display = "i"
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if flux_lim is not None:
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@@ -420,9 +457,12 @@ def polarization_map(
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vmin, vmax = 1.0 / 2.0 * np.median(np.sqrt(stk_cov[0, 0][stkI > 0.0]) * convert_flux), np.max(stkI[stkI > 0.0] * convert_flux)
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im = ax.imshow(stkI * convert_flux, norm=LogNorm(vmin, vmax), aspect="equal", cmap=kwargs["cmap"], alpha=1.0)
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fig.colorbar(im, ax=ax, aspect=50, shrink=0.60, pad=0.025, label=r"$F_{\lambda}$ [$ergs \cdot cm^{-2} \cdot s^{-1} \cdot \AA^{-1}$]")
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levelsI = np.array([0.8, 2.0, 5.0, 10.0, 20.0, 50.0]) / 100.0 * vmax
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print("Flux density contour levels : ", levelsI)
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ax.contour(stkI * convert_flux, levels=levelsI, colors="grey", linewidths=0.5)
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# levelsI = np.array([0.8, 2.0, 5.0, 10.0, 20.0, 50.0]) / 100.0 * vmax
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# print("Stokes I contour levels : ", levelsI)
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# ax.contour(stkI * convert_flux, levels=levelsI, colors="grey", linewidths=0.5)
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levelsF = np.array([0.8, 2.0, 5.0, 10.0, 20.0, 50.0]) / 100.0 * np.max(flux[flux > 0.0])
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print("Flux density contour levels : ", levelsF)
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ax.contour(flux, levels=levelsF, transform=ax.get_transform(WCS(Stokes[0].header).celestial), colors="grey", linewidths=0.5)
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elif display.lower() in ["pf", "pol_flux"]:
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# Display polarization flux
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display = "pf"
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@@ -512,22 +552,18 @@ def polarization_map(
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# Defaults to intensity map
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if flux_lim is not None:
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vmin, vmax = flux_lim
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elif mask.sum() > 0.0:
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vmin, vmax = 1.0 * np.mean(np.sqrt(stk_cov[0, 0][mask]) * convert_flux), np.max(stkI[stkI > 0.0] * convert_flux)
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else:
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vmin, vmax = 1.0 * np.mean(np.sqrt(stk_cov[0, 0][stkI > 0.0]) * convert_flux), np.max(stkI[stkI > 0.0] * convert_flux)
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im = ax.imshow(stkI * convert_flux, norm=LogNorm(vmin, vmax), aspect="equal", cmap=kwargs["cmap"], alpha=1.0)
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vmin, vmax = np.max(flux[flux > 0.0] * convert_flux) / 2e3, np.max(flux[flux > 0.0] * convert_flux)
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im = ax.imshow(
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flux * Stokes[0].header["PHOTFLAM"],
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transform=ax.get_transform(WCS(Stokes[0].header).celestial),
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norm=LogNorm(vmin, vmax),
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aspect="equal",
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cmap=kwargs["cmap"],
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alpha=1.0,
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)
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fig.colorbar(im, ax=ax, aspect=50, shrink=0.60, pad=0.025, label=r"$F_{\lambda}$ [$ergs \cdot cm^{-2} \cdot s^{-1} \cdot \AA$]")
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# Get integrated flux values from sum
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I_diluted = stkI[data_mask].sum()
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I_diluted_err = np.sqrt(np.sum(stk_cov[0, 0][data_mask]))
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# Get integrated polarization values from header
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P_diluted = Stokes[0].header["P_int"]
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P_diluted_err = Stokes[0].header["sP_int"]
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PA_diluted = Stokes[0].header["PA_int"]
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PA_diluted_err = Stokes[0].header["sPA_int"]
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I_diluted, I_diluted_err = np.sum(flux[flux_mask]), np.sqrt(np.sum(flux_error[flux_mask] ** 2))
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plt.rcParams.update({"font.size": 11})
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px_size = wcs.wcs.get_cdelt()[0] * 3600.0
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@@ -545,12 +581,12 @@ def polarization_map(
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back_length=0.0,
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head_length=7.0,
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head_width=7.0,
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angle=-Stokes[0].header["orientat"],
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angle=-Stokes["I_STOKES"].header["orientat"],
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text_props={"ec": "k", "fc": font_color, "alpha": 1, "lw": 0.5},
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arrow_props={"ec": "k", "fc": font_color, "alpha": 1, "lw": 1},
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)
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if display.lower() in ["i", "s_i", "snri", "pf", "p", "pa", "s_p", "snrp", "confp"] and step_vec != 0:
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if display.lower() in ["f", "i", "s_i", "snri", "pf", "p", "pa", "s_p", "snrp", "confp"] and step_vec != 0:
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if scale_vec == -1:
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poldata[np.isfinite(poldata)] = 1.0 / 2.0
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step_vec = 1
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@@ -1174,6 +1210,8 @@ class overplot_chandra(align_maps):
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other_data = deepcopy(self.other_data)
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other_wcs = self.other_wcs.deepcopy()
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if zoom != 1:
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from scipy.ndimage import zoom as sc_zoom
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other_data = sc_zoom(other_data, zoom)
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other_wcs.wcs.crpix *= zoom
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other_wcs.wcs.cdelt /= zoom
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@@ -2439,9 +2477,9 @@ class pol_map(object):
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self.conf = PCconf(self.QN, self.UN, self.QN_ERR, self.UN_ERR)
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# Get data
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self.targ = self.Stokes[0].header["targname"]
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self.pivot_wav = self.Stokes[0].header["photplam"]
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self.map_convert = self.Stokes[0].header["photflam"]
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self.targ = self.Stokes["I_STOKES"].header["targname"]
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self.pivot_wav = self.Stokes["I_STOKES"].header["photplam"]
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self.map_convert = self.Stokes["I_STOKES"].header["photflam"]
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# Create figure
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plt.rcParams.update({"font.size": 10})
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@@ -2535,7 +2573,7 @@ class pol_map(object):
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def select_roi(event):
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if self.data is None:
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self.data = self.Stokes[0].data
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self.data = self.Stokes["I_STOKES"].data
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if self.selected:
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self.selected = False
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self.region = deepcopy(self.select_instance.mask.astype(bool))
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@@ -2577,7 +2615,7 @@ class pol_map(object):
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def select_aperture(event):
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if self.data is None:
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self.data = self.Stokes[0].data
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self.data = self.Stokes["I_STOKES"].data
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if self.selected:
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self.selected = False
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self.select_instance.update_mask()
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@@ -2634,7 +2672,7 @@ class pol_map(object):
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def select_slit(event):
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if self.data is None:
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self.data = self.Stokes[0].data
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self.data = self.Stokes["I_STOKES"].data
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if self.selected:
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self.selected = False
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self.select_instance.update_mask()
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@@ -2911,7 +2949,19 @@ class pol_map(object):
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@property
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def wcs(self):
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return WCS(self.Stokes[0].header).celestial.deepcopy()
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return WCS(self.Stokes["I_STOKES"].header).celestial.deepcopy()
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@property
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def Flux(self):
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return self.Stokes[0].data[0] * self.Stokes[0].header["PHOTFLAM"]
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@property
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def Flux_err(self):
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return self.Stokes[0].data[1] * self.Stokes[0].header["PHOTFLAM"]
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@property
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def Flux_mask(self):
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return self.Stokes[0].data[2].astype(bool)
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@property
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def I(self):
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@@ -2975,7 +3025,7 @@ class pol_map(object):
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@property
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def data_mask(self):
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return self.Stokes["DATA_MASK"].data
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return self.Stokes["DATA_MASK"].data.astype(bool)
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def set_data_mask(self, mask):
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self.Stokes[np.argmax([self.Stokes[i].header["datatype"] == "Data_mask" for i in range(len(self.Stokes))])].data = mask.astype(float)
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@@ -3046,7 +3096,7 @@ class pol_map(object):
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back_length=0.0,
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head_length=10.0,
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head_width=10.0,
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angle=-self.Stokes[0].header["orientat"],
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angle=-self.Stokes["I_STOKES"].header["orientat"],
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color="white",
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text_props={"ec": None, "fc": "w", "alpha": 1, "lw": 0.4},
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arrow_props={"ec": None, "fc": "w", "alpha": 1, "lw": 1},
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@@ -3054,18 +3104,20 @@ class pol_map(object):
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ax.add_artist(self.north_dir)
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def display(self, fig=None, ax=None, flux_lim=None):
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norm = None
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if self.display_selection is None:
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self.display_selection = "total_flux"
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kwargs = dict([])
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if flux_lim is None:
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flux_lim = self.flux_lim
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if self.display_selection.lower() in ["total_flux"]:
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self.data = self.I * self.map_convert
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if self.display_selection is None or self.display_selection.lower() in ["total_flux"]:
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self.data = self.Flux # self.I * self.map_convert
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if flux_lim is None:
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vmin, vmax = (1.0 / 2.0 * np.median(self.data[self.data > 0.0]), np.max(self.data[self.data > 0.0]))
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else:
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vmin, vmax = flux_lim
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norm = LogNorm(vmin, vmax)
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kwargs["norm"] = LogNorm(vmin, vmax)
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if ax is None:
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kwargs["transform"] = self.ax.get_transform(WCS(self.Stokes[0].header).celestial)
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else:
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kwargs["transform"] = ax.get_transform(WCS(self.Stokes[0].header).celestial)
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label = r"$F_{\lambda}$ [$ergs \cdot cm^{-2} \cdot s^{-1} \cdot \AA^{-1}$]"
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elif self.display_selection.lower() in ["pol_flux"]:
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self.data = self.I * self.map_convert * self.P
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@@ -3073,28 +3125,28 @@ class pol_map(object):
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vmin, vmax = (1.0 / 2.0 * np.median(self.I[self.I > 0.0] * self.map_convert), np.max(self.I[self.I > 0.0] * self.map_convert))
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else:
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vmin, vmax = flux_lim
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norm = LogNorm(vmin, vmax)
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kwargs["norm"] = LogNorm(vmin, vmax)
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label = r"$P \cdot F_{\lambda}$ [$ergs \cdot cm^{-2} \cdot s^{-1} \cdot \AA^{-1}$]"
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elif self.display_selection.lower() in ["pol_deg"]:
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self.data = self.P * 100.0
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vmin, vmax = 0.0, np.max(self.data[self.P > self.s_P])
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kwargs["vmin"], kwargs["vmax"] = 0.0, np.max(self.data[self.P > self.s_P])
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label = r"$P$ [%]"
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elif self.display_selection.lower() in ["pol_ang"]:
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self.data = princ_angle(self.PA)
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vmin, vmax = 0, 180.0
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kwargs["vmin"], kwargs["vmax"] = 0, 180.0
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label = r"$\theta_{P}$ [°]"
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elif self.display_selection.lower() in ["snri"]:
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s_I = np.sqrt(self.IQU_cov[0, 0])
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SNRi = np.zeros(self.I.shape)
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SNRi[s_I > 0.0] = self.I[s_I > 0.0] / s_I[s_I > 0.0]
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self.data = SNRi
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vmin, vmax = 0.0, np.max(self.data[self.data > 0.0])
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kwargs["vmin"], kwargs["vmax"] = 0.0, np.max(self.data[self.data > 0.0])
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label = r"$I_{Stokes}/\sigma_{I}$"
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elif self.display_selection.lower() in ["snrp"]:
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SNRp = np.zeros(self.P.shape)
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SNRp[self.s_P > 0.0] = self.P[self.s_P > 0.0] / self.s_P[self.s_P > 0.0]
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self.data = SNRp
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vmin, vmax = 0.0, np.max(self.data[self.data > 0.0])
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kwargs["vmin"], kwargs["vmax"] = 0.0, np.max(self.data[self.data > 0.0])
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label = r"$P/\sigma_{P}$"
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if fig is None:
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@@ -3105,22 +3157,17 @@ class pol_map(object):
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self.cbar.remove()
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if hasattr(self, "im"):
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self.im.remove()
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if norm is not None:
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self.im = ax.imshow(self.data, norm=norm, aspect="equal", cmap="inferno")
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else:
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self.im = ax.imshow(self.data, vmin=vmin, vmax=vmax, aspect="equal", cmap="inferno")
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self.im = ax.imshow(self.data, aspect="equal", cmap="inferno", **kwargs)
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ax.set(xlim=(0, self.I.shape[1]), ylim=(0, self.I.shape[0]))
|
||||
plt.rcParams.update({"font.size": 14})
|
||||
self.cbar = fig.colorbar(self.im, ax=ax, aspect=50, shrink=0.75, pad=0.025, label=label)
|
||||
plt.rcParams.update({"font.size": 10})
|
||||
fig.canvas.draw_idle()
|
||||
return self.im
|
||||
else:
|
||||
if norm is not None:
|
||||
im = ax.imshow(self.data, norm=norm, aspect="equal", cmap="inferno")
|
||||
else:
|
||||
im = ax.imshow(self.data, vmin=vmin, vmax=vmax, aspect="equal", cmap="inferno")
|
||||
ax.set_xlim(0, self.data.shape[1])
|
||||
ax.set_ylim(0, self.data.shape[0])
|
||||
im = ax.imshow(self.data, aspect="equal", cmap="inferno", **kwargs)
|
||||
ax.set_xlim(0, self.I.shape[1])
|
||||
ax.set_ylim(0, self.I.shape[0])
|
||||
plt.rcParams.update({"font.size": 14})
|
||||
fig.colorbar(im, ax=ax, aspect=50, shrink=0.75, pad=0.025, label=label)
|
||||
plt.rcParams.update({"font.size": 10})
|
||||
@@ -3144,24 +3191,24 @@ class pol_map(object):
|
||||
ax = self.ax
|
||||
if hasattr(self, "quiver"):
|
||||
self.quiver.remove()
|
||||
self.quiver = ax.quiver(
|
||||
X[:: self.step_vec, :: self.step_vec],
|
||||
Y[:: self.step_vec, :: self.step_vec],
|
||||
XY_U[:: self.step_vec, :: self.step_vec],
|
||||
XY_V[:: self.step_vec, :: self.step_vec],
|
||||
units="xy",
|
||||
scale=1.0 / scale_vec,
|
||||
scale_units="xy",
|
||||
pivot="mid",
|
||||
headwidth=0.0,
|
||||
headlength=0.0,
|
||||
headaxislength=0.0,
|
||||
width=0.3,
|
||||
linewidth=0.6,
|
||||
color="white",
|
||||
edgecolor="black",
|
||||
)
|
||||
if self.pa_err:
|
||||
self.quiver = ax.quiver(
|
||||
X[:: self.step_vec, :: self.step_vec],
|
||||
Y[:: self.step_vec, :: self.step_vec],
|
||||
XY_U[:: self.step_vec, :: self.step_vec],
|
||||
XY_V[:: self.step_vec, :: self.step_vec],
|
||||
units="xy",
|
||||
scale=1.0 / scale_vec,
|
||||
scale_units="xy",
|
||||
pivot="mid",
|
||||
headwidth=0.0,
|
||||
headlength=0.0,
|
||||
headaxislength=0.0,
|
||||
width=0.1,
|
||||
# linewidth=0.6,
|
||||
color="black",
|
||||
edgecolor="black",
|
||||
)
|
||||
XY_U_err1, XY_V_err1 = (
|
||||
P_cut * np.cos(np.pi / 2.0 + (self.PA + 3.0 * self.s_PA) * np.pi / 180.0),
|
||||
P_cut * np.sin(np.pi / 2.0 + (self.PA + 3.0 * self.s_PA) * np.pi / 180.0),
|
||||
@@ -3210,6 +3257,25 @@ class pol_map(object):
|
||||
edgecolor="black",
|
||||
ls="dashed",
|
||||
)
|
||||
else:
|
||||
self.quiver = ax.quiver(
|
||||
X[:: self.step_vec, :: self.step_vec],
|
||||
Y[:: self.step_vec, :: self.step_vec],
|
||||
XY_U[:: self.step_vec, :: self.step_vec],
|
||||
XY_V[:: self.step_vec, :: self.step_vec],
|
||||
units="xy",
|
||||
scale=1.0 / scale_vec,
|
||||
scale_units="xy",
|
||||
pivot="mid",
|
||||
headwidth=0.0,
|
||||
headlength=0.0,
|
||||
headaxislength=0.0,
|
||||
width=0.3,
|
||||
linewidth=0.6,
|
||||
color="white",
|
||||
edgecolor="black",
|
||||
)
|
||||
|
||||
fig.canvas.draw_idle()
|
||||
return self.quiver
|
||||
else:
|
||||
@@ -3281,12 +3347,20 @@ class pol_map(object):
|
||||
str_conf = ""
|
||||
if self.region is None:
|
||||
s_I = np.sqrt(self.IQU_cov[0, 0])
|
||||
I_reg = self.I.sum()
|
||||
I_reg_err = np.sqrt(np.sum(s_I**2))
|
||||
P_reg = self.Stokes[0].header["P_int"]
|
||||
P_reg_err = self.Stokes[0].header["sP_int"]
|
||||
PA_reg = self.Stokes[0].header["PA_int"]
|
||||
PA_reg_err = self.Stokes[0].header["sPA_int"]
|
||||
I_reg = (
|
||||
np.sum(self.Flux[self.Flux_mask]) / self.map_convert
|
||||
if self.display_selection is None or self.display_selection.lower() in ["total_flux"]
|
||||
else np.sum(self.I[self.data_mask])
|
||||
)
|
||||
I_reg_err = (
|
||||
np.sqrt(np.sum(self.Flux_err[self.Flux_mask] ** 2)) / self.map_convert
|
||||
if self.display_selection is None or self.display_selection.lower() in ["total_flux"]
|
||||
else np.sqrt(np.sum(s_I[self.data_mask] ** 2))
|
||||
)
|
||||
P_reg = self.Stokes["I_STOKES"].header["P_int"]
|
||||
P_reg_err = self.Stokes["I_STOKES"].header["sP_int"]
|
||||
PA_reg = self.Stokes["I_STOKES"].header["PA_int"]
|
||||
PA_reg_err = self.Stokes["I_STOKES"].header["sPA_int"]
|
||||
|
||||
s_I = np.sqrt(self.IQU_cov[0, 0])
|
||||
s_Q = np.sqrt(self.IQU_cov[1, 1])
|
||||
|
||||
Reference in New Issue
Block a user