Пример #1
0
def strehlframe(image, primary, secondary, dimension, f_number, pixel_scale,
        lambda_mean, growth_step, find_source, xcenter, ycenter, fwhmpsf,
        threshold, quiet):
    start_time = time.time()
    info("Started at:", start_time)
    if not os.path.exists(image):
        raise RuntimeError("No file named {0}".format(image))
    # Were we given coordinates, or do we need to find the source?
    if find_source:
        bright = daofind_brightest(image, fwhmpsf, threshold)
        center_col, center_row = bright['XCENTER'], bright['YCENTER']
    else:
        center_col, center_row = xcenter, ycenter
    
    scale_to_physical, plate_scale_px, min_radius_real = compute_psf_scale(
        dimension,
        primary,
        secondary,
        f_number,
        lambda_mean,
        pixel_scale
    )
    
    scaled_psf, scaled_psf_ctr, max_aperture_radius = generate_scaled_psf(
        dimension,
        primary,
        secondary,
        scale_to_physical
    )
    
    # wrap psf in a frame
    psf = Frame(scaled_psf, scaled_psf_ctr)
    # precompute CoG and profile to be rescaled later
    curve_of_growth(psf, max_aperture_radius, step=growth_step, quiet=quiet)
    profile_from_growthcurve(psf)
    
    # values and functions to rescale our PSF Frame computed values
    # to physical counts
    max_extent_px = 2.5 / plate_scale_px # After 2.5" we're almost certainly measuring noise
    debug("after 2.5'' or", max_extent_px, "px we're almost certainly measuring noise")
    
    def max_flux(frame):
        """Frame max integrated flux (for a radius less than 2.5'')"""
        return np.max(frame.fluxes[frame.radii <= max_extent_px])
    
    def scale_psf_fluxes(frame, psf):
        """
        Returns a profile and curve of growth values for the ideal PSF
        scaled such that the total integrated flux is equivalent to the
        maximum flux in the frame passed as the first argument.
        """
        scale_factor = (max_flux(frame) / max_flux(psf))
        return psf.profile * scale_factor, psf.fluxes * scale_factor

    image_base = os.path.splitext(os.path.basename(image))[0]
    frame = Frame(pyfits.getdata(image), (float(center_col), float(center_row)))
    debug("loaded frame from", image)
    # subtract median row to handle light/charge leakage biasing measurements
    exclude_from, exclude_to = frame.ybounds(r=int(max_extent_px)) # exclude region of max_extent_px around center of frame
    avgrow_median_subtract(frame, exclude_from, exclude_to)
    debug("median subtracted frame")
    curve_of_growth(frame, max_aperture_radius, step=growth_step, quiet=quiet)
    debug("curve of growth generated")
    profile_from_growthcurve(frame)
    debug("profile generated")
    
    # scale psf.fluxes and psf.profile to a max value determined from frame
    ideal_profile, ideal_fluxes = scale_psf_fluxes(frame, psf)
    
    write_table("{0}_strehl.dat".format(image_base), (
        ("Pixel Radius", frame.radii),
        ("Enclosed Pixels", frame.npix),
        ("Image Enclosed Energy (counts)", frame.fluxes),
        ("Ideal Enclosed Energy (counts)", ideal_fluxes),
        ("Strehl Ratio (for peak in this radius)", frame.fluxes / ideal_fluxes),
        ("Image Radial Profile (counts at radius)", frame.profile),
        ("Ideal Radial Profile (counts at radius)", ideal_profile)
    ))
    
    # Plot Curve of Growth with twinned axis in arcseconds
    
    plot_with_arcseconds(
        image_base + "_growth.pdf",
        psf.radii,
        frame.fluxes,
        ideal_fluxes,
        min_radius_real,
        max_extent_px,
        plate_scale_px,
        ylabel="Enclosed Flux at Radius"
    )
    
    # fig, host = plt.subplots()
    # 
    # plt.plot(frame.radii, frame.fluxes, 'r', label="Science Image")
    # plt.plot(psf.radii, ideal_fluxes, 'g', label="Ideal PSF")
    # plt.axvspan(0, min_radius_real, facecolor='g', alpha=0.25)
    # 
    # plt.ylabel("Enclosed Flux at Radius")
    # plt.xlabel("Radius (pixels from center)")
    # 
    # plt.xlim(1, max_extent_px)
    # plt.ylim(0, np.max(ideal_fluxes))
    # xfrom, xto = fig.axes[0].get_xlim()
    # par1 = host.twiny()
    # par1.axes.set_xlabel("Radius (arcseconds from center)")
    # par1.set_xlim((xfrom * plate_scale_px, xto * plate_scale_px))
    # par1.grid()
    # host.legend(loc=4)
    # 
    # plt.savefig('{0}_growth.pdf'.format(image_base))
    # debug("saved plot to", '{0}_growth.pdf'.format(image_base))
    # 
    
    # Plot profile with twinned axis in arcseconds
    
    plot_with_arcseconds(
        image_base + "_profile.pdf",
        psf.radii,
        frame.profile,
        ideal_profile,
        min_radius_real,
        10, # xlim max
        plate_scale_px,
        ylabel="Flux at Radius",
        marker="."
    )
    
    # fig, host = plt.subplots()
    # 
    # plt.plot(frame.radii, frame.profile, c='r', marker=".", label="Science Image")
    # plt.plot(psf.radii, ideal_profile, c='g', marker='.', label="Ideal PSF")
    # plt.axvspan(0, min_radius_real, facecolor='g', alpha=0.25)
    # 
    # plt.ylabel("Flux at Radius")
    # plt.xlabel("Radius (pixels from center)")
    # 
    # plt.xlim(1, 10)
    # plt.ylim(0, np.max(ideal_profile))
    # xfrom, xto = fig.axes[0].get_xlim()
    # par1 = host.twiny()
    # par1.axes.set_xlabel("Radius (arcseconds from center)")
    # par1.set_xlim((xfrom * plate_scale_px, xto * plate_scale_px))
    # par1.grid()
    # host.legend(loc=4)
    # 
    # plt.savefig('{0}_profile.pdf'.format(image_base))
    # debug("saved plot to", '{0}_profile.pdf'.format(image_base))
    info("Completed at:", time.time())
    info("Total time:", time.time() - start_time)
Пример #2
0
def strehlcube(cubefile, rangespec, primary, secondary, dimension, f_number,
        pixel_scale, lambda_mean, growth_step, fwhmpsf, threshold, quiet):
    start_time = time.time()
    info("Started at:", start_time)
    if not os.path.exists(cubefile):
        raise RuntimeError("No file named {0}".format(cubefile))
    cubefile_base = os.path.splitext(os.path.basename(cubefile))[0]
    # I: compute ideal psf
    
    scale_to_physical, plate_scale_px, min_radius_real = compute_psf_scale(
        dimension,
        primary,
        secondary,
        f_number,
        lambda_mean,
        pixel_scale
    )
    
    scaled_psf, scaled_psf_ctr, max_aperture_radius = generate_scaled_psf(
        dimension,
        primary,
        secondary,
        scale_to_physical
    )
    
    # wrap psf in a frame
    psf = Frame(scaled_psf, scaled_psf_ctr)
    # precompute CoG and profile to be rescaled later
    curve_of_growth(psf, max_aperture_radius, step=growth_step, quiet=quiet)
    profile_from_growthcurve(psf)
    
    # II: analyze images
    
    # values and functions to rescale our PSF Frame computed values
    # to physical counts
    max_extent_px = 2.5 / plate_scale_px # After 2.5" we're almost certainly measuring noise
    debug("after 2.5'' or", max_extent_px, "px we're almost certainly measuring noise")
    
    def max_flux(frame):
        """Frame max integrated flux (for a radius less than 2.5'')"""
        return np.max(frame.fluxes[frame.radii <= max_extent_px])
    
    def scale_psf_fluxes(frame, psf):
        """
        Returns a profile and curve of growth values for the ideal PSF
        scaled such that the total integrated flux is equivalent to the
        maximum flux in the frame passed as the first argument.
        """
        scale_factor = (max_flux(frame) / max_flux(psf))
        return psf.profile * scale_factor, psf.fluxes * scale_factor

    tmp_target_dir = tempfile.mkdtemp()
    ranges = parse_ranges(rangespec)
    debug("splitting ranges", ranges)
    fits_frames = split_frames(cubefile, ranges, tmp_target_dir)
    debug("working in", tmp_target_dir, "with frames", fits_frames)

    # set up array to hold each frame's analysis data
    radii_count = psf.radii.shape[0]
    frame_count = len(fits_frames)
    shape = (frame_count, 5, radii_count)
    analysis_frames = np.zeros(shape)
    # [cog x count, prof x count, ideal x count, idealprof x count, strehl x count] x frames
    
    strehl_rows = []
    
    for fits_frame in fits_frames:
        bright = daofind_brightest(fits_frame, fwhmpsf, threshold)
        center_col, center_row = bright['XCENTER'], bright['YCENTER']
        # this is slightly dumb... parse the frame # out of the filename
        frame_num = int(re.findall(r'\d+', os.path.basename(fits_frame))[0])
        debug("frame #", frame_num, "has brightest at", center_col, center_row)
        frame = Frame(pyfits.getdata(fits_frame), (float(center_col), float(center_row)))
        debug("loaded frame from", fits_frame)
    
        # subtract median row to handle light/charge leakage biasing measurements
        exclude_from, exclude_to = frame.ybounds(r=int(max_extent_px)) # exclude region of max_extent_px around center of frame
        avgrow_median_subtract(frame, exclude_from, exclude_to)
        debug("median subtracted frame")
        curve_of_growth(frame, max_aperture_radius, step=growth_step, quiet=quiet)
        debug("curve of growth generated")
        profile_from_growthcurve(frame)
        debug("profile generated")
    
        # scale psf.fluxes and psf.profile to a max value determined from frame
        ideal_profile, ideal_fluxes = scale_psf_fluxes(frame, psf)
        strehls_for_all_radii = frame.fluxes / ideal_fluxes
        strehl_rows.append((frame_num, strehls_for_all_radii))

    outfile = "{0}_{1}_strehlseries.txt".format(cubefile_base, rangespec)
    debug("writing strehl series to", outfile)
    with open(outfile, 'w') as f:
        f.write("# columns 2 and up are the pixel radii at which we computed the Strehl ratio")
        f.write("# frameidx\t")
        f.write('\t'.join(map(str, psf.radii)))
        f.write('\n')
        for idx, ratios in strehl_rows:
            f.write(str(idx))
            f.write('\t')
            f.write('\t'.join(map(str, ratios)))
            f.write('\n')

    debug("removing exploded cube from", tmp_target_dir)
    shutil.rmtree(tmp_target_dir)

    info("Completed at:", time.time())
    info("Total time:", time.time() - start_time)