def _data_stretch(image, vmin=None, vmax=None, pmin=0.25, pmax=99.75,
stretch='linear', vmid=None, exponent=2):
if vmin is None or vmax is None:
interval = AsymmetricPercentileInterval(pmin, pmax, n_samples=10000)
try:
vmin_auto, vmax_auto = interval.get_limits(image)
except IndexError: # no valid values
vmin_auto = vmax_auto = 0
if vmin is None:
log.info("vmin = %10.3e (auto)" % vmin_auto)
vmin = vmin_auto
else:
log.info("vmin = %10.3e" % vmin)
if vmax is None:
log.info("vmax = %10.3e (auto)" % vmax_auto)
vmax = vmax_auto
else:
log.info("vmax = %10.3e" % vmax)
if stretch == 'arcsinh':
stretch = 'asinh'
normalizer = simple_norm(image, stretch=stretch, power=exponent,
asinh_a=vmid, min_cut=vmin, max_cut=vmax, clip=False)
data = normalizer(image, clip=True).filled(0)
data = np.nan_to_num(data)
data = np.clip(data * 255., 0., 255.)
return data.astype(np.uint8)
def starfind(setup,
path_to_image,
reduction_metadata,
plot_it=False,
log=None):
"""
The routine will quickly identify stars in a given image and return
a star list and image quality parameters. The output is to be used
to select suitable candidate images for constructing a template
reference image.
:param object setup: this is an instance of the ReductionSetup class. See
reduction_control.py
:param string path_to_image: The full path to the image to be processed.
:param object reduction_metadata: The reduction metadata object from
which to extract the saturation value.
:param boolean plot_it: Do you want to plot the selected stars?
:param string log: Full The full path to the log file.
:return status, report, params: the first two are strings reporting whether
the stage was completed successfully. params is
a dictionary with the image quality parameters.
:rtype string, string, dictionary
"""
imname = path_to_image.split('/')[-1]
if log != None:
log.info('Starting starfind')
params = {
'sky': 0.0,
'fwhm_y': 0.0,
'fwhm_x': 0.0,
'corr_xy': 0.0,
'nstars': 0,
'sat_frac': 0.0,
'symmetry': 1.
}
t0 = time.time()
im = fits.open(path_to_image)
header = im[0].header
scidata = im[0].data
# Get size of image
ymax, xmax = scidata.shape
# If it is a large image, consider 250x250 pixel subregions and
# choose the one with the fewest saturated pixels to evaluate stats
try:
saturation = reduction_metadata.reduction_parameters[1]['MAXVAL']
except:
if log != None:
status = 'ERROR'
report = ('Could not extract the saturation parameter '
'from the configuration file.')
log.info(report)
return status, report, params
nr_sat_pix = 100000
bestx1 = -1
bestx2 = -1
besty1 = -1
besty2 = -1
regionsx = np.arange(0, xmax, 250)
regionsy = np.arange(0, ymax, 250)
for i in regionsx[0:-1]:
x1 = i
x2 = i + 250
for j in regionsy[0:-1]:
y1 = j
y2 = j + 250
nr_pix = len(
scidata[y1:y2,
x1:x2][np.where(scidata[y1:y2, x1:x2] > saturation)])
#print x1, x2, y1, y2, nr_pix
if nr_pix < nr_sat_pix:
nr_sat_pix = nr_pix
bestx1 = x1
bestx2 = x2
besty1 = y1
besty2 = y2
#mean, median, std = sigma_clipped_stats(scidata[1:ymax, 1:xmax], sigma=3.0, iters=5)
# Evaluate mean, median and standard deviation for the selected subregion
mean, median, std = sigma_clipped_stats(scidata[besty1:besty2,
bestx1:bestx2],
sigma=3.0,
iters=5)
# Identify stars
daofind = DAOStarFinder(fwhm=3.0, threshold=5. * std)
sources = daofind(scidata[besty1:besty2, bestx1:bestx2] - median)
# Write steps to a log file
if log != None:
log.info("Identifying sources on image %s ...\n" %
path_to_image.split('/')[-1])
log.info("Found %s sources.\n" % str(len(sources)))
if len(sources) == 0:
status = 'ERROR'
report = 'Insufficient number of sources found. Stopping execution.'
log.info(report)
return status, report, params
elif (len(sources) > 0 and len(sources) <= 5):
log.info('WARNING: Too few sources detected on image.')
else:
log.info('Using best sources to determine FWHM (up to 30).')
# Discount saturated stars
sources = sources[np.where(sources['peak'] < saturation)]
sources.sort('peak')
sources.reverse()
# Store the number of identified sources and fraction of saturated pixels
nstars = len(sources)
sat_frac = nr_sat_pix / (250. * 250.)
# Discount stars too close to the edges of the image
sources = sources[np.where((sources['xcentroid'] > 10)
& (sources['xcentroid'] < 240)
& (sources['ycentroid'] < 240)
& (sources['ycentroid'] > 30))]
# Keep only up to 100 stars
sources = sources[0:100]
sources_with_close_stars_ids = []
# Discount stars with close neighbours (within r=10 pix)
for i in np.arange(len(sources)):
source_i = sources[i]
for other_source in sources[i + 1:]:
if (np.sqrt(
(source_i['xcentroid'] - other_source['xcentroid'])**2 +
(source_i['ycentroid'] - other_source['ycentroid'])**2) <= 10):
sources_with_close_stars_ids.append(i)
#print source_i, other_source
continue
# Keep up to 30 isolated sources only (may be fewer)
sources.remove_rows(sources_with_close_stars_ids)
sources = sources[0:30]
if log != None:
log.info("Kept %s sources.\n" % str(len(sources)))
#return sources
# Uncomment the following line to display source list in browser window:
#sources.show_in_browser()
# Fit a model to identified sources and estimate PSF shape parameters
sky_arr = []
fwhm_x_arr = []
fwhm_y_arr = []
corr_xy_arr = []
i = 0
while (i <= len(sources) - 1):
try:
i_peak = sources[i]['peak']
position = [sources[i]['xcentroid'], sources[i]['ycentroid']]
#print position
stamp_size = (20, 20)
cutout = Cutout2D(scidata[besty1:besty2, bestx1:bestx2], position,
stamp_size) # in pixels
yc, xc = cutout.position_cutout
yy, xx = np.indices(cutout.data.shape)
fit = psf.fit_star(cutout.data,
yy,
xx,
psf_model='BivariateNormal')
fit_params = fit[0]
fit_errors = fit[1].diagonal()**0.5
biv = psf.BivariateNormal()
background = psf.ConstantBackground()
fit_residuals = psf.error_star_fit_function(
fit_params, cutout.data, biv, background, yy, xx)
fit_residuals = fit_residuals.reshape(cutout.data.shape)
cov = fit[1] * np.sum(fit_residuals**2) / ((stamp_size[0])**2 - 6)
fit_errors = cov.diagonal()**0.5
#print fit_params
model = biv.psf_model(yy, xx, fit_params)
fwhm_y_arr.append(fit_params[3])
fwhm_x_arr.append(fit_params[4])
corr_xy_arr.append(fit_params[5])
sky_arr.append(fit_params[6])
if plot_it == True:
plt.figure(figsize=(3, 8))
plt.subplot(3, 1, 1)
plt.imshow(cutout.data, cmap='gray', origin='lower')
plt.colorbar()
plt.title("Data")
plt.subplot(3, 1, 2)
plt.imshow(model, cmap='gray', origin='lower')
plt.colorbar()
plt.title("Model")
plt.subplot(3, 1, 3)
plt.imshow(fit_residuals, cmap='gray', origin='lower')
plt.title("Residual")
plt.colorbar()
plt.savefig(path.join(setup.red_dir, 'starfind_model.png'))
except:
if log != None:
log.info("Could not fit source: %s." % str(i))
i = i + 1
# Estimate the median values for the parameters over the stars identified
params['sky'] = np.median(sky_arr)
params['fwhm_y'] = np.median(fwhm_y_arr)
params['fwhm_x'] = np.median(fwhm_x_arr)
params['corr_xy'] = np.median(corr_xy_arr)
params['nstars'] = nstars
params['sat_frac'] = sat_frac
try:
if xmax > 200 and ymax > 200:
psf_emp, psf_error_emp = empirical_psf_simple.empirical_psf_median(
np.copy(scidata)[:200, :200], 20, saturation)
else:
psf_emp, psf_error_emp = empirical_psf_simple.empirical_psf_median(
np.copy(scidata), 20, saturation)
#imgname = os.path.basename(path_to_image)
#hduout=fits.PrimaryHDU(psf_emp)
#hduout.writeto('psf_'+imgname,overwrite = True)
symmetry_metric = empirical_psf_simple.symmetry_check(psf_emp)
params['symmetry'] = symmetry_metric
except Exception as e:
if log != None:
report = ('Could not extract the symmetry based on the PSF ')
log.info(report)
if log != None:
log.info('Measured median values:')
log.info('Sky background = ' + str(params['sky']))
log.info('FWHM X = ' + str(params['fwhm_x']))
log.info('FWHM Y = ' + str(params['fwhm_y']))
log.info('Corr XY = ' + str(params['corr_xy']))
log.info('Nstars = ' + str(params['nstars']))
log.info('Saturation fraction = ' + str(params['sat_frac']))
log.info('symmetry = ' + str(params['symmetry']))
# If plot_it is True, plot the sources found
if plot_it == True:
temp = np.copy(scidata[besty1:besty2, bestx1:bestx2])
temp[np.where(temp < median)] = median
temp[np.where(temp > 25000)] = 25000
positions = (sources['xcentroid'], sources['ycentroid'])
apertures = CircularAperture(positions, r=4.)
norm = ImageNormalize(interval=AsymmetricPercentileInterval(10, 40),
stretch=SqrtStretch())
plt.imshow(temp, cmap='gray', origin='lower', norm=norm)
plt.title("Data")
#plt.colorbar()
apertures.plot(color='red', lw=1.2, alpha=0.5)
plt.savefig(path.join(setup.red_dir, 'stars250x250.png'))
im.close()
if log != None:
log.info("Finished processing image %s in %.3f seconds.\n" %
(str(imname), (time.time() - t0)))
status = 'OK'
report = 'Completed successfully'
return status, report, params
async def get(self, object_id: str = None):
"""
---
summary: Serve alert cutout as fits or png
tags:
- alerts
- kowalski
parameters:
- in: query
name: instrument
required: false
schema:
type: str
- in: query
name: candid
description: "ZTF alert candid"
required: true
schema:
type: integer
- in: query
name: cutout
description: "retrieve science, template, or difference cutout image?"
required: true
schema:
type: string
enum: [science, template, difference]
- in: query
name: file_format
description: "response file format: original loss-less FITS or rendered png"
required: true
default: png
schema:
type: string
enum: [fits, png]
- in: query
name: interval
description: "Interval to use when rendering png"
required: false
schema:
type: string
enum: [min_max, zscale]
- in: query
name: stretch
description: "Stretch to use when rendering png"
required: false
schema:
type: string
enum: [linear, log, asinh, sqrt]
- in: query
name: cmap
description: "Color map to use when rendering png"
required: false
schema:
type: string
enum: [bone, gray, cividis, viridis, magma]
responses:
'200':
description: retrieved cutout
content:
image/fits:
schema:
type: string
format: binary
image/png:
schema:
type: string
format: binary
'400':
description: retrieval failed
content:
application/json:
schema: Error
"""
instrument = self.get_query_argument("instrument", "ZTF").upper()
if instrument not in INSTRUMENTS:
raise ValueError("Instrument name not recognised")
# allow access to public data only by default
selector = {1}
for stream in self.associated_user_object.streams:
if "ztf" in stream.name.lower():
selector.update(set(stream.altdata.get("selector", [])))
selector = list(selector)
try:
candid = int(self.get_argument("candid"))
cutout = self.get_argument("cutout").capitalize()
file_format = self.get_argument("file_format", "png").lower()
interval = self.get_argument("interval", default=None)
stretch = self.get_argument("stretch", default=None)
cmap = self.get_argument("cmap", default=None)
known_cutouts = ["Science", "Template", "Difference"]
if cutout not in known_cutouts:
return self.error(
f"Cutout {cutout} of {object_id}/{candid} not in {str(known_cutouts)}"
)
known_file_formats = ["fits", "png"]
if file_format not in known_file_formats:
return self.error(
f"File format {file_format} of {object_id}/{candid}/{cutout} not in {str(known_file_formats)}"
)
normalization_methods = {
"asymmetric_percentile": AsymmetricPercentileInterval(
lower_percentile=1, upper_percentile=100
),
"min_max": MinMaxInterval(),
"zscale": ZScaleInterval(nsamples=600, contrast=0.045, krej=2.5),
}
if interval is None:
interval = "asymmetric_percentile"
normalizer = normalization_methods.get(
interval.lower(),
AsymmetricPercentileInterval(lower_percentile=1, upper_percentile=100),
)
stretching_methods = {
"linear": LinearStretch,
"log": LogStretch,
"asinh": AsinhStretch,
"sqrt": SqrtStretch,
}
if stretch is None:
stretch = "log" if cutout != "Difference" else "linear"
stretcher = stretching_methods.get(stretch.lower(), LogStretch)()
if (cmap is None) or (
cmap.lower() not in ["bone", "gray", "cividis", "viridis", "magma"]
):
cmap = "bone"
else:
cmap = cmap.lower()
query = {
"query_type": "find",
"query": {
"catalog": "ZTF_alerts",
"filter": {
"candid": candid,
"candidate.programid": {"$in": selector},
},
"projection": {"_id": 0, f"cutout{cutout}": 1},
},
"kwargs": {"limit": 1, "max_time_ms": 5000},
}
response = kowalski.query(query=query)
if response.get("status", "error") == "success":
alert = response.get("data", [dict()])[0]
else:
return self.error("No cutout found.")
cutout_data = bj.loads(bj.dumps([alert[f"cutout{cutout}"]["stampData"]]))[0]
# unzipped fits name
fits_name = pathlib.Path(alert[f"cutout{cutout}"]["fileName"]).with_suffix(
""
)
# unzip and flip about y axis on the server side
with gzip.open(io.BytesIO(cutout_data), "rb") as f:
with fits.open(io.BytesIO(f.read())) as hdu:
header = hdu[0].header
data_flipped_y = np.flipud(hdu[0].data)
if file_format == "fits":
hdu = fits.PrimaryHDU(data_flipped_y, header=header)
hdul = fits.HDUList([hdu])
stamp_fits = io.BytesIO()
hdul.writeto(fileobj=stamp_fits)
self.set_header("Content-Type", "image/fits")
self.set_header(
"Content-Disposition", f"Attachment;filename={fits_name}"
)
self.write(stamp_fits.getvalue())
if file_format == "png":
buff = io.BytesIO()
plt.close("all")
fig, ax = plt.subplots(figsize=(4, 4))
fig.subplots_adjust(0, 0, 1, 1)
ax.set_axis_off()
# replace nans with median:
img = np.array(data_flipped_y)
# replace dubiously large values
xl = np.greater(np.abs(img), 1e20, where=~np.isnan(img))
if img[xl].any():
img[xl] = np.nan
if np.isnan(img).any():
median = float(np.nanmean(img.flatten()))
img = np.nan_to_num(img, nan=median)
norm = ImageNormalize(img, stretch=stretcher)
img_norm = norm(img)
vmin, vmax = normalizer.get_limits(img_norm)
ax.imshow(img_norm, cmap=cmap, origin="lower", vmin=vmin, vmax=vmax)
plt.savefig(buff, dpi=42)
buff.seek(0)
plt.close("all")
self.set_header("Content-Type", "image/png")
self.write(buff.getvalue())
except Exception:
_err = traceback.format_exc()
return self.error(f"failure: {_err}")
def display_single(img,
pixel_scale=0.168,
physical_scale=None,
xsize=8,
ysize=8,
ax=None,
alpha=1.0,
stretch='arcsinh',
scale='zscale',
zmin=None,
zmax=None,
contrast=0.25,
no_negative=False,
lower_percentile=1.0,
upper_percentile=99.0,
cmap=IMG_CMAP,
scale_bar=True,
scale_bar_length=5.0,
scale_bar_fontsize=20,
scale_bar_y_offset=0.5,
scale_bar_color='w',
scale_bar_loc='left',
color_bar=False,
color_bar_loc=1,
color_bar_width='75%',
color_bar_height='5%',
color_bar_fontsize=18,
color_bar_color='w',
add_text=None,
text_fontsize=30,
text_color='w'):
"""Display single image.
Parameters
----------
img: np 2-D array for image
xsize: int, default = 8
Width of the image.
ysize: int, default = 8
Height of the image.
"""
if ax is None:
fig = plt.figure(figsize=(xsize, ysize))
ax1 = fig.add_subplot(111)
else:
ax1 = ax
# Stretch option
if stretch.strip() == 'arcsinh':
img_scale = np.arcsinh(img)
if zmin is not None:
zmin = np.arcsinh(zmin)
if zmax is not None:
zmax = np.arcsinh(zmax)
elif stretch.strip() == 'log':
if no_negative:
img[img <= 0.0] = 1.0E-10
img_scale = np.log(img)
if zmin is not None:
zmin = np.log(zmin)
if zmax is not None:
zmax = np.log(zmax)
elif stretch.strip() == 'log10':
if no_negative:
img[img <= 0.0] = 1.0E-10
img_scale = np.log10(img)
if zmin is not None:
zmin = np.log10(zmin)
if zmax is not None:
zmax = np.log10(zmax)
elif stretch.strip() == 'linear':
img_scale = img
else:
raise Exception("# Wrong stretch option.")
# Scale option
if scale.strip() == 'zscale':
try:
vmin, vmax = ZScaleInterval(
contrast=contrast).get_limits(img_scale)
except IndexError:
# TODO: Deal with problematic image
vmin, vmax = -1.0, 1.0
elif scale.strip() == 'percentile':
try:
vmin, vmax = AsymmetricPercentileInterval(
lower_percentile=lower_percentile,
upper_percentile=upper_percentile).get_limits(img_scale)
except IndexError:
# TODO: Deal with problematic image
vmin, vmax = -1.0, 1.0
elif scale.strip() == 'minmax':
vmin, vmax = np.nanmin(img_scale), np.nanmax(img_scale)
else:
vmin, vmax = np.nanmin(img_scale), np.nanmax(img_scale)
if zmin is not None:
vmin = zmin
if zmax is not None:
vmax = zmax
show = ax1.imshow(img_scale,
origin='lower',
cmap=cmap,
interpolation='none',
vmin=vmin,
vmax=vmax,
alpha=alpha)
# Hide ticks and tick labels
ax1.tick_params(labelbottom=False,
labelleft=False,
axis=u'both',
which=u'both',
length=0)
# Put scale bar on the image
(img_size_x, img_size_y) = img.shape
if physical_scale is not None:
pixel_scale *= physical_scale
if scale_bar:
if scale_bar_loc == 'left':
scale_bar_x_0 = int(img_size_x * 0.04)
scale_bar_x_1 = int(img_size_x * 0.04 +
(scale_bar_length / pixel_scale))
else:
scale_bar_x_0 = int(img_size_x * 0.95 -
(scale_bar_length / pixel_scale))
scale_bar_x_1 = int(img_size_x * 0.95)
scale_bar_y = int(img_size_y * 0.10)
scale_bar_text_x = (scale_bar_x_0 + scale_bar_x_1) / 2
scale_bar_text_y = (scale_bar_y * scale_bar_y_offset)
if physical_scale is not None:
scale_bar_text = r'$%d\ \mathrm{kpc}$' % int(scale_bar_length)
else:
scale_bar_text = r'$%d^{\prime\prime}$' % int(scale_bar_length)
scale_bar_text_size = scale_bar_fontsize
ax1.plot([scale_bar_x_0, scale_bar_x_1], [scale_bar_y, scale_bar_y],
linewidth=3,
c=scale_bar_color,
alpha=1.0)
ax1.text(scale_bar_text_x,
scale_bar_text_y,
scale_bar_text,
fontsize=scale_bar_text_size,
horizontalalignment='center',
color=scale_bar_color)
if add_text is not None:
text_x_0 = int(img_size_x * 0.08)
text_y_0 = int(img_size_y * 0.80)
ax1.text(text_x_0,
text_y_0,
r'$\mathrm{' + add_text + '}$',
fontsize=text_fontsize,
color=text_color)
# Put a color bar on the image
if color_bar:
ax_cbar = inset_axes(ax1,
width=color_bar_width,
height=color_bar_height,
loc=color_bar_loc)
if ax is None:
cbar = plt.colorbar(show,
ax=ax1,
cax=ax_cbar,
orientation='horizontal')
else:
cbar = plt.colorbar(show,
ax=ax,
cax=ax_cbar,
orientation='horizontal')
cbar.ax.xaxis.set_tick_params(color=color_bar_color)
cbar.ax.yaxis.set_tick_params(color=color_bar_color)
cbar.outline.set_edgecolor(color_bar_color)
plt.setp(plt.getp(cbar.ax.axes, 'xticklabels'),
color=color_bar_color,
fontsize=color_bar_fontsize)
plt.setp(plt.getp(cbar.ax.axes, 'yticklabels'),
color=color_bar_color,
fontsize=color_bar_fontsize)
if ax is None:
return fig
return ax1
#kde = stats.gaussian_kde(imx)
#density = kde(imx)
#peak = max(peak,0.01)
#low_perc = max(low_perc,0.01)
# set 1% as the minimum cut
#print ("Histo Peak at %f, will use it as lower percentile (i.e. remove everything below)"%(h_peak))
#
#peak_norm = (peak - np.min(bins1))/(np.max(bins1) - np.min(bins1))
#print ("Normalized peak is at %f"%(peak_norm))
#n1, bins1, patches1 = plt.hist(image[~np.isnan(image)], 50, normed=1, facecolor='green', histtype='step',alpha=0.75)
#
#%%
fig = plt.figure(figsize=(10, 10))
norm = ImageNormalize(image,
interval=AsymmetricPercentileInterval(
mode_x * 100, 99.5),
stretch=AsinhStretch())
#norm = ImageNormalize(image,interval=PercentileInterval(98),stretch=SqrtStretch())
#norm = ImageNormalize(image,interval=PercentileInterval(99.5),stretch=LogStretch())
ax = fig.add_subplot(111)
ax.imshow(image,
cmap=cm.gray,
norm=norm,
origin="lower",
interpolation="nearest")
ax.get_xaxis().set_ticks([])
ax.get_yaxis().set_ticks([])
ax.annotate("%s, %i %s" % (target, myObsid, band),
textcoords='axes fraction',
fontsize=10,
xy=(0.05, 0.95),
def display_single(img,
pixel_scale=0.168,
physical_scale=None,
xsize=8,
ysize=8,
ax=None,
stretch='arcsinh',
scale='zscale',
scale_manual=None,
contrast=0.25,
no_negative=False,
lower_percentile=1.0,
upper_percentile=99.0,
cmap=IMG_CMAP,
scale_bar=True,
scale_bar_length=5.0,
scale_bar_fontsize=20,
scale_bar_y_offset=0.5,
scale_bar_color='w',
scale_bar_alpha=1.0,
scale_bar_loc='left',
color_bar=False,
color_bar_loc=1,
color_bar_width='75%',
color_bar_height='5%',
color_bar_fontsize=18,
color_bar_color='w',
add_text=None,
text_fontsize=30,
text_box=None,
text_facecolor='gray',
text_x_offset=0.08,
text_y_offset=0.80,
text_color='w',
text_fontweight='normal'):
"""
Display single image using ``arcsinh`` stretching, "zscale" scaling and ``viridis`` colormap as default.
This function is from ``kungpao`` https://github.com/dr-guangtou/kungpao.
Parameters:
img (numpy 2-D array): The image array.
pixel_scale (float): The pixel size, in unit of "arcsec/pixel".
physical_scale (bool): Whether show the image in physical scale.
xsize (int): Width of the image, default = 8.
ysize (int): Height of the image, default = 8.
ax (``matplotlib.pyplot.axes`` object): The user could provide axes on which the figure will be drawn.
stretch (str): Stretching schemes. Options are "arcsinh", "log", "log10" and "linear".
scale (str): Scaling schemes. Options are "zscale" and "percentile".
contrast (float): Contrast of figure.
no_negative (bool): If true, all negative pixels will be set to zero.
lower_percentile (float): Lower percentile, if using ``scale="percentile"``.
upper_percentile (float): Upper percentile, if using ``scale="percentile"``.
cmap (str): Colormap.
scale_bar (bool): Whether show scale bar or not.
scale_bar_length (float): The length of scale bar.
scale_bar_y_offset (float): Offset of scale bar on y-axis.
scale_bar_fontsize (float): Fontsize of scale bar ticks.
scale_bar_color (str): Color of scale bar.
scale_bar_alpha (float): alpha of scale bar.
scale_bar_loc (str): Scale bar position, options are "left" and "right".
color_bar (bool): Whether show colorbar or not.
add_text (str): The text you want to add to the figure. Note that it is wrapped within ``$\mathrm{}$``.
text_fontsize (float): Fontsize of text.
text_y_offset (float): Offset of text on y-axis.
text_color (str): Color of text.
text_box (dict): dictionary for box. Such as `dict(boxstyle='round', facecolor='wheat', alpha=0.5)`.
Returns:
ax: If the input ``ax`` is not ``None``.
"""
from PIL import Image, ImageOps
if ax is None:
fig = plt.figure(figsize=(xsize, ysize))
ax1 = fig.add_subplot(111)
else:
ax1 = ax
if isinstance(img, Image.Image):
img = ImageOps.flip(img)
show = ax1.imshow(
img,
origin='lower',
cmap=cmap,
)
(img_size_x, img_size_y) = img.size
else:
(img_size_x, img_size_y) = img.shape
# Stretch option
if stretch.strip() == 'arcsinh':
img_scale = np.arcsinh(img)
elif stretch.strip() == 'log':
if no_negative:
img[img <= 0.0] = 1.0E-10
img_scale = np.log(img)
elif stretch.strip() == 'log10':
if no_negative:
img[img <= 0.0] = 1.0E-10
img_scale = np.log10(img)
elif stretch.strip() == 'linear':
img_scale = img
else:
raise Exception("# Wrong stretch option.")
# Scale option
if scale.strip() == 'zscale':
try:
zmin, zmax = ZScaleInterval(
contrast=contrast).get_limits(img_scale)
except IndexError:
# TODO: Deal with problematic image
zmin, zmax = -1.0, 1.0
elif scale.strip() == 'percentile':
try:
zmin, zmax = AsymmetricPercentileInterval(
lower_percentile=lower_percentile,
upper_percentile=upper_percentile).get_limits(img_scale)
except IndexError:
# TODO: Deal with problematic image
zmin, zmax = -1.0, 1.0
else:
zmin, zmax = np.nanmin(img_scale), np.nanmax(img_scale)
if scale_manual is not None:
assert len(
scale_manual) == 2, '# length of manual scale must be two!'
zmin, zmax = scale_manual
show = ax1.imshow(img_scale,
origin='lower',
cmap=cmap,
vmin=zmin,
vmax=zmax)
# Hide ticks and tick labels
ax1.tick_params(labelbottom=False,
labelleft=False,
axis=u'both',
which=u'both',
length=0)
#ax1.axis('off')
# Put scale bar on the image
if physical_scale is not None:
pixel_scale *= physical_scale
if scale_bar:
if scale_bar_loc == 'left':
scale_bar_x_0 = int(img_size_x * 0.04)
scale_bar_x_1 = int(img_size_x * 0.04 +
(scale_bar_length / pixel_scale))
else:
scale_bar_x_0 = int(img_size_x * 0.95 -
(scale_bar_length / pixel_scale))
scale_bar_x_1 = int(img_size_x * 0.95)
scale_bar_y = int(img_size_y * 0.10)
scale_bar_text_x = (scale_bar_x_0 + scale_bar_x_1) / 2
scale_bar_text_y = (scale_bar_y * scale_bar_y_offset)
if physical_scale is not None:
if scale_bar_length > 1000:
scale_bar_text = r'$%d\ \mathrm{Mpc}$' % int(
scale_bar_length / 1000)
else:
scale_bar_text = r'$%d\ \mathrm{kpc}$' % int(scale_bar_length)
else:
if scale_bar_length < 60:
scale_bar_text = r'$%d^{\prime\prime}$' % int(scale_bar_length)
elif 60 < scale_bar_length < 3600:
scale_bar_text = r"%d arcmin" % int(
scale_bar_length / 60) # r'$%d^{\prime}$'
else:
scale_bar_text = r'$%d^{\circ}$' % int(scale_bar_length / 3600)
scale_bar_text_size = scale_bar_fontsize
ax1.plot([scale_bar_x_0, scale_bar_x_1], [scale_bar_y, scale_bar_y],
linewidth=5,
c=scale_bar_color,
alpha=scale_bar_alpha)
ax1.text(scale_bar_text_x,
scale_bar_text_y,
scale_bar_text,
fontsize=scale_bar_text_size,
fontweight=text_fontweight,
horizontalalignment='center',
color=scale_bar_color,
alpha=scale_bar_alpha)
if add_text is not None:
text_x_0 = int(img_size_x * text_x_offset)
text_y_0 = int(img_size_y * text_y_offset)
ax1.text(text_x_0,
text_y_0,
add_text,
horizontalalignment='left',
verticalalignment='top',
fontsize=text_fontsize,
color=text_color,
bbox=text_box,
fontweight=text_fontweight)
# Put a color bar on the image
if color_bar:
ax_cbar = inset_axes(ax1,
width=color_bar_width,
height=color_bar_height,
loc=color_bar_loc)
if ax is None:
cbar = plt.colorbar(show,
ax=ax1,
cax=ax_cbar,
orientation='horizontal')
else:
cbar = plt.colorbar(show,
ax=ax,
cax=ax_cbar,
orientation='horizontal')
cbar.ax.xaxis.set_tick_params(color=color_bar_color)
cbar.ax.yaxis.set_tick_params(color=color_bar_color)
cbar.outline.set_edgecolor(color_bar_color)
plt.setp(plt.getp(cbar.ax.axes, 'xticklabels'),
color=color_bar_color,
fontsize=color_bar_fontsize)
plt.setp(plt.getp(cbar.ax.axes, 'yticklabels'),
color=color_bar_color,
fontsize=color_bar_fontsize)
if ax is None:
return fig
return ax1
#pl.subplots_adjust(left=panel_rect[0], bottom=panel_rect[1], right=panel_rect[0]+panel_rect[2], top=panel_rect[1]+panel_rect[3])
pl.imshow(FitsImage, cmap='gray', origin='lower', aspect='equal', norm=LogNorm())
#cb = pl.colorbar()
#
# Save eps
#
fig.savefig('%s.scale.log.jpg'%(FitsFile), format='jpg')
print('Output to %s'%('%s.scale.log.jpg'%(FitsFile)))
#
# Plot the fits image in 99.5 percentile
#
if [[ 1 == 0 ]]; then
pl.cla()
#fig.delaxes(fig.axes[-1]) # remove previous colorbar
#pl.subplots_adjust(left=panel_rect[0], bottom=panel_rect[1], right=panel_rect[0]+panel_rect[2], top=panel_rect[1]+panel_rect[3])
normfun = ImageNormalize(FitsImage, interval=AsymmetricPercentileInterval(19.5,99.5))
pl.imshow(FitsImage, cmap='gray', origin='lower', aspect='equal', norm=normfun)
#cb = pl.colorbar()
#
# Save eps
#
fig.savefig('%s.scale.995.jpg'%(FitsFile), format='jpg')
print('Output to %s'%('%s.scale.995.jpg'%(FitsFile)))
print('Done!')
def plot_rgb(self,
filters,
ax=None,
ra=None,
dec=None,
radius=None,
north=True,
rscale=2,
upper_scale=99.7,
lower_scale=1,
asinh_factor=0.7):
""" Given a filter, makes a normalized, asinh-stretched plot of a galaxy.
INPUTS:
filters: list of filter names [red, green, blue] e.g. ["i", "r", "g"]
ax: axis to plot on. If None, create a new plot
north: align the data North? Default: True
rpet: radius of the galaxy. If None, use "size" from the Galaxy object
xc, yc: pixel coordinates of image center. If None, use ra, dec of Galaxy
rpet_scale: image scale in terms of galaxy radii
upper_scale, lower_scale: scales used in normalization. By default, upper_scale
is given in metadata or 99.7; lower_scale is 1
"""
# Load the images for each filter
data = {"r": {}, "g": {}, "b": {}}
for filt, key in zip(filters, data):
node = self.data[filt]
data[key]["img"] = node["img"][()]
data[key]["wcs"] = attr_to_wcs(node.attrs)
data[key]["pxscale"] = node.attrs["pxscale"]
# If ra, dec and rpet are not passed, populate them using galaxy properties
if ra is None or dec is None or radius is None:
ra, dec, radius = self.ra, self.dec, self.size
# Resize all images
for k, v in data.items():
v["img"], v["wcs"] = _resize(v["img"],
v["wcs"],
ra,
dec,
v["pxscale"],
radius,
scale=rscale)
# Create a WCS to reproject the images to using blue WCS (north-aligned?)
rgb_wcs = data["b"]["wcs"].deepcopy()
if north:
rgb_pxscale = data["b"]["pxscale"]
rgb_wcs = _rotate_wcs(rgb_wcs, ra, dec, rgb_pxscale)
# Define stretch and norm
try:
upper_scale = self.data.attrs["uscale"]
except:
pass
stretch = AsinhStretch(asinh_factor)
norm = AsymmetricPercentileInterval(lower_scale, upper_scale)
norm_r = AsymmetricPercentileInterval(lower_scale, upper_scale - 0.1)
# Reproject all data onto this new WCS, apply norm and stretch
for k, v in data.items():
img = reproject_interp((v["img"], v["wcs"]),
rgb_wcs,
shape_out=data["b"]["img"].shape)[
0] #data["b"]["img"].shape)[0]
img = stretch(norm_r(img)) if k == "r" else stretch(norm(img))
v["plot_img"] = img
# Make a data cube
rgb = np.dstack([val["plot_img"] for key, val in data.items()])
# If ax=None, create figure
if ax is None:
fig = plt.figure(figsize=(6, 6))
ax = plt.axes()
ax.axis('off')
ax.imshow(rgb, origin="lower")
def normalize_img(img_arr, stretch='asinh', minmax_percent=None, minmax_value=None, invert=False):
"""
Apply given stretch and scaling to an image array.
Parameters
----------
img_arr : array
The input image array.
stretch : str
Optional, default 'asinh'. The stretch to apply to the image array.
Valid values are: asinh, sinh, sqrt, log, linear
minmax_percent : array
Optional. Interval based on a keeping a specified fraction of pixels (can be asymmetric)
when scaling the image. The format is [lower percentile, upper percentile], where pixel
values below the lower percentile and above the upper percentile are clipped.
Only one of minmax_percent and minmax_value shoul be specified.
minmax_value : array
Optional. Interval based on user-specified pixel values when scaling the image.
The format is [min value, max value], where pixel values below the min value and above
the max value are clipped.
Only one of minmax_percent and minmax_value should be specified.
invert : bool
Optional, default False. If True the image is inverted (light pixels become dark and vice versa).
Returns
-------
response : array
The normalized image array, in the form in an integer arrays with values in the range 0-255.
"""
# Setting up the transform with the stretch
if stretch == 'asinh':
transform = AsinhStretch()
elif stretch == 'sinh':
transform = SinhStretch()
elif stretch == 'sqrt':
transform = SqrtStretch()
elif stretch == 'log':
transform = LogStretch()
elif stretch == 'linear':
transform = LinearStretch()
else:
raise InvalidInputError("Stretch {} is not supported!".format(stretch))
# Adding the scaling to the transform
if minmax_percent is not None:
transform += AsymmetricPercentileInterval(*minmax_percent)
if minmax_value is not None:
warnings.warn("Both minmax_percent and minmax_value are set, minmax_value will be ignored.",
InputWarning)
elif minmax_value is not None:
transform += ManualInterval(*minmax_value)
else: # Default, scale the entire image range to [0,1]
transform += MinMaxInterval()
# Performing the transform and then putting it into the integer range 0-255
norm_img = transform(img_arr)
norm_img = np.multiply(255, norm_img, out=norm_img)
norm_img = norm_img.astype(np.uint8)
# Applying invert if requested
if invert:
norm_img = 255 - norm_img
return norm_img
imdss = sax.imshow(dssdata, transform=sax.get_transform(dssw), cmap='bone', vmin=vmin+dmad)
textent = None
talpha = .66
else:
sax = plt.subplot()
textent = [column, column+args.size, row, row+args.size]
talpha = 1
lcmap = cmap_map(lambda x: 0.6*x, cm.get_cmap(args.cmap))
#stamp = sax.imshow(np.log10(np.nanmedian(flux[::10], axis=0)),
# cmap=lcmap, origin='lower', aspect='equal', alpha=talpha,
# extent=textent)
mstamp = np.nanmedian(flux[::10], axis=0)
norm = ImageNormalize(mstamp, interval=AsymmetricPercentileInterval(0,100), stretch=LogStretch(a=250))
stamp = sax.imshow(mstamp,
cmap=lcmap, origin='lower', aspect='equal', alpha=talpha,
extent=textent, norm=norm)
xm, ym = pixel_border(dap[bidx])
for xi,yi in zip(xm, ym):
if args.pngdss:
sax.plot(xi, yi, color='#FF0043', lw=1.5, transform=sax.get_transform('pixel'))
else:
sax.plot(column+xi, row+yi, color='#FF0043', lw=1.5)
#sax.grid(which='minor', zorder=99)
#sax.grid(color='white')
def get_regstat(fixed_image, moving_image, out_stats, out_tm, out_qc, tm):
x = [[]]
time1 = time.time()
# loading images
target = plt.imread(fixed_image)
#tar=cv2.imread(fixed_image)
target_name = os.path.split(fixed_image)[1]
# print(target_name)
# target=cv2.resize(target,(5705,5705))
# tar=cv2.resize(tar,(5705,5705))
moving = plt.imread(moving_image)
#mov=cv2.imread(moving_image)
# moving=cv2.resize(moving,(5705,5705))
# mov=cv2.resize(mov,(5705,5705))
moving_name = os.path.split(moving_image)[-1]
# print(moving_name)
# registration
#a=target.shape[0]
b=target.shape[1]
#moving=cv2.resize(moving,(b,b))
mov_avg=np.mean(moving.astype("float"))
print(target.shape)
print(moving.shape)
res=ird.similarity(target,moving)
def_moving=res['timg']
scale=res['scale']
angle=res['angle']
(t0,t1)=res['tvec']
#def_moving, scale, angle, (t0, t1) = imreg.similarity(target, moving)
def_mov_array=imreg.similarity_matrix(scale,angle,(t0,t1))
np.save(out_tm, def_mov_array)
def_avg=np.mean(def_moving.astype("float"))
# def_moving=cv2.resize(def_moving,(5705,5705))
time2 = time.time()
ti = time2-time1
# statistical results
cc = np.corrcoef(moving.flat, target.flat)
r1 = cc[0, 1]
score1, diff = compare_ssim(target, moving, full=True, multichannel=True)
loss_before = 0.5*(1-r1) + 0.5*(1-score1)
cc = np.corrcoef(def_moving.flat, target.flat)
r2 = cc[0, 1]
score2, diff = compare_ssim(def_moving, target, full=True)
loss_after = 0.5*(1-r2) + 0.5*(1-score2)
mi_bef = mutual_info_score(moving.ravel(), target.ravel())
mi_aft = mutual_info_score(target.ravel(), def_moving.ravel())
mae = np.sum(np.absolute(target.astype("float") - moving.astype("float")))
u1 = np.sum(target.astype("float") + moving.astype("float"))
mean_before = np.divide(mae, u1)
u2 = np.sum(target.astype("float") + def_moving.astype("float"))
mae = np.sum(np.absolute(target.astype(
"float") - def_moving.astype("float")))
mean_after = np.divide(mae, u2)
t = Texttable()
#print(def_moving.shape)
if mi_aft > mi_bef:
plt.imsave(tm, def_moving,cmap='gray')
else:
plt.imsave(tm, moving,cmap='gray')
# plt.imsave(tm,def_moving,cmap='gray')
x.append([target_name, moving_name, r1, r2, score1, score2, loss_before,
loss_after, mi_bef, mi_aft, mean_before, mean_after,mov_avg,def_avg, ti])
t.add_rows(x)
t.set_cols_align(['r', 'r', 'r', 'r', 'r', 'r',
'r', 'r', 'r', 'r', 'r', 'r', 'r','r', 'r'])
t.header(['TARGET', 'MOVING', 'PCC_BEFORE', 'PCC_AFTER', 'SSIM_BEFORE', 'SSIM_AFTER',
'loss_BEFORE', 'loss_AFTER', 'MI_BEFORE', 'MI_AFTER', 'MEAN_BEFORE', 'MEAN_AFTER', 'AVERAGE_INTENSITY_BEFORE', 'AVERAGE_INTENSITY_AFTER','TIME'])
def_mov1 = cv2.imread(tm,0)
# plotting the results
transform = AsinhStretch() + AsymmetricPercentileInterval(0.1, 99.99)
targ= transform(target)
#targ=cv2.cvtColor(targ.astype(np.uint8),cv2.COLOR_GRAY2RGB)
#targ_im=Image.fromarray(targ)
plt.imsave('target.tiff', targ, cmap='gray')
#plt.imsave(r'/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/target.tiff', targ, cmap='gray')
movi = transform(moving)
#movi=cv2.cvtColor(movi.astype(np.uint8),cv2.COLOR_GRAY2BGR)
plt.imsave('moving.tiff', movi, cmap='gray')
#movi_im=Image.fromarray(movi)
#plt.imsave(r'/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/moving.tiff', movi, cmap='gray')
targ = cv2.imread('target.tiff')
#targ=Image.open(targ_im)
movi= cv2.imread('moving.tiff')
#movi=Image.open(movi_im)
#targ = cv2.imread( r'/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/target.tiff')
#movi = cv2.imread(r'/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/moving.tiff')
# def_mov1=cv2.resize(def_mov1,(5705,5705))
def_mov1 = transform(def_mov1)
#print(def_mov2.shape)
#def_mov1=cv2.cvtColor(def_mov1.astype(np.uint8),cv2.COLOR_GRAY2BGR)
plt.imsave('def_moving.tiff', def_mov1, cmap='gray')
#def_mov1=Image.fromarray(def_mov1)
#plt.imsave('/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/def_moving.tiff', def_mov1, cmap='gray')
def_mov1 = cv2.imread('def_moving.tiff')
#def_mov1=Image.open(def_mov1)
#def_mov1 = cv2.imread(r'/media/u0132399/L-drive/GBW-0075_MILAN_Multiplex/u0140317/registration_comparison/imreg/output_images/def_moving.tiff')
#targ = targ.astype(np.uint8)
#movi = movi.astype(np.uint8)
#def_mov1 = def_mov1.astype(np.uint8)
tar1 = np.zeros(targ.shape)
mov1 = np.zeros(movi.shape)
def_mov = np.zeros(def_mov1.shape)
tar1[:, :, 0] = targ[:, :, 0]
mov1[:, :, 2] = movi[:, :, 2]
def_mov[:, :, 2] = def_mov1[:, :, 2]
tar1 = tar1.astype(np.uint8)
mov1 = mov1.astype(np.uint8)
def_mov = def_mov.astype(np.uint8)
# mov[np.where((mov>[15]).all(axis=2))]=[255,0,0]
# def_mov1[np.where((def_mov1>[15]).all(axis=2))]=[255,0,0]
alpha = 1
beta = 1
gamma = 0
t1 = cv2.addWeighted(tar1, alpha, mov1, beta, gamma)
# filename=target_name+moving_name+'unreg_imreg.tif'
# cv2.imwrite(,t1)
t2 = cv2.addWeighted(tar1, alpha, def_mov, beta, gamma)
# filename=target_name+moving_name+'reg_imreg.tif'
# cv2.imwrite(filename,t2)
if mi_aft > mi_bef:
cv2.imwrite(out_qc, t2)
else:
cv2.imwrite(out_qc, t1)
# plt.figure(figsize=(10,10))
# plt.axis('off')
# plt.imshow(t1,cmap='gray')
# plt.show(block=False)
# plt.pause(5)
# plt.close()
# plt.figure(figsize=(10,10))
# plt.axis('off')
# plt.imshow(t2,cmap='gray')
# plt.show(block=False)
# plt.pause(5)
# plt.close()
df = pd.DataFrame(x, columns=['TARGET', 'MOVING', 'PCC_BEFORE', 'PCC_AFTER', 'SSIM_BEFORE', 'SSIM_AFTER',
'loss_BEFORE', 'loss_AFTER', 'MI_BEFORE', 'MI_AFTER', 'MEAN_BEFORE', 'MEAN_AFTER','AVERAGE_INTENSITY_BEFORE', 'AVERAGE_INTENSITY_AFTER', 'TIME'])
#df[columns]= ['PCC_BEFORE','PCC_AFTER','SSIM_BEFORE' ,'SSIM_AFTER','loss_BEFORE','loss_AFTER','MI_BEFORE','MI_AFTER','MEAN_BEFORE','MEAN_AFTER']
#writer = pd.ExcelWriter(out_stats)
df.to_csv(out_stats, index=None, header=True)
# writer.save()
#print(t.draw())
return t
def as_array(self,
interval_r=AsymmetricPercentileInterval(2.5, 99.0),
interval_g=AsymmetricPercentileInterval(5., 99.2),
interval_b=AsymmetricPercentileInterval(10., 99.2)):
"""Returns the colour image as a MxNx3 (RGB) array."""
# First we determine the shifts
cx, cy = 2050, 1024 # central coordinates of the image
maxshiftx, maxshifty = 0, 0
aligned_imgs = {}
for idx, band in enumerate(self.filenames.keys()):
fn = self.filenames[band]
hdu = fits.open(os.path.join(VPHAS_DATA_PATH, fn))[self.ccd]
wcs = WCS(hdu.header)
img = hdu.data
if idx == 0: # The first image acts as reference
cra, cdec = wcs.wcs_pix2world(cx, cy, 1)
else: # For all subsequent images, compute the shift using the WCS
refx, refy = wcs.wcs_world2pix(cra, cdec, 1)
shiftx = int(refx - cx)
shifty = int(refy - cy)
# Now apply the required shift to the image
if shiftx > 0:
img = np.pad(img, ((0, 0), (0, shiftx)),
mode=str('constant'))[:, shiftx:]
elif shiftx < 0:
img = np.pad(img, ((0, 0), (-shiftx, 0)),
mode=str('constant'))[:, :shiftx]
if shifty > 0:
img = np.pad(img, ((0, shifty), (0, 0)),
mode=str('constant'))[shifty:, :]
elif shifty < 0:
img = np.pad(img, ((-shifty, 0), (0, 0)),
mode=str('constant'))[:shifty, :]
# The maximum shift applied will determine the final img shape
maxshiftx = max(abs(shiftx), maxshiftx)
maxshifty = max(abs(shifty), maxshifty)
aligned_imgs[band] = img
if maxshiftx > cx or maxshifty > cy:
raise VphasDataException('{0}-{1}: bands do not overlap'.format(
self.offset, self.ccd))
# New stretch, scale, and stack the data into an MxNx3 array
r = aligned_imgs['i'] + aligned_imgs['ha']
g = aligned_imgs['g'] + aligned_imgs['r'] + aligned_imgs['r2']
b = aligned_imgs['u'] + 2 * aligned_imgs['g']
r, g, b = 1.5 * r, 0.8 * g, 2.2 * b
vmin_r, vmax_r = np.percentile(r, [1., 99.5])
vmin_g, vmax_g = np.percentile(g, [5., 99.5])
vmin_b, vmax_b = np.percentile(b, [10., 99.5])
#log.info((vmin_r, vmin_g, vmin_b))
#log.info((vmax_r, vmax_g, vmax_b))
#if vmin_b < 100:
# vmin_b = 100
minrange = np.max(
(1250., vmax_g - vmin_g, vmax_g - vmin_g, vmax_b - vmin_b))
if (vmax_r - vmin_r) < minrange:
vmax_r = vmin_r + minrange
if (vmax_g - vmin_g) < minrange:
vmax_g = vmin_g + minrange
if (vmax_b - vmin_b) < minrange:
vmax_b = vmin_b + minrange
interval_r = ManualInterval(vmin_r, vmax_r)
interval_g = ManualInterval(vmin_g, vmax_g)
interval_b = ManualInterval(vmin_b, vmax_b)
r = interval_r(r)
g = interval_g(g)
b = interval_b(b)
stacked = np.dstack((r[maxshifty:-maxshifty, maxshiftx:-maxshiftx],
g[maxshifty:-maxshifty,
maxshiftx:-maxshiftx], b[maxshifty:-maxshifty,
maxshiftx:-maxshiftx]))
return LuptonColorStretch()(stacked)
def data_to_pitch(data_array,
pitch_range=[100, 10000],
center_pitch=440,
zero_point="median",
stretch='linear',
minmax_percent=None,
minmax_value=None):
"""
Map data array to audible pitches in the given range, and apply stretch and scaling
as required.
Parameters
----------
data_array : array-like
Data to map to pitch values. Individual data values should be floats.
pitch_range : array
Optional, default [100,10000]. Range of acceptable pitches in Hz.
center_pitch : float
Optional, default 440. The pitch in Hz where that the the zero point of the
data will be mapped to.
zero_point : str or float
Optional, default "median". The data value that will be mapped to the center
pitch. Options are mean, median, or a specifical data value (float).
stretch : str
Optional, default 'linear'. The stretch to apply to the data array.
Valid values are: asinh, sinh, sqrt, log, linear
minmax_percent : array
Optional. Interval based on a keeping a specified fraction of data values (can be asymmetric)
when scaling the data. The format is [lower percentile, upper percentile], where data
values below the lower percentile and above the upper percentile are clipped.
Only one of minmax_percent and minmax_value should be specified.
minmax_value : array
Optional. Interval based on user-specified data values when scaling the data array.
The format is [min value, max value], where data values below the min value and above
the max value are clipped.
Only one of minmax_percent and minmax_value should be specified.
Returns
-------
response : array
The normalized data array, with values in given pitch range.
"""
# Parsing the zero point
if zero_point in ("med", "median"):
zero_point = np.median(data_array)
if zero_point in ("ave", "mean", "average"):
zero_point = np.mean(data_array)
# Normalizing the data_array and adding the zero point (so it can go through the same transform)
data_array = np.append(np.array(data_array), zero_point)
# Setting up the transform with the stretch
if stretch == 'asinh':
transform = AsinhStretch()
elif stretch == 'sinh':
transform = SinhStretch()
elif stretch == 'sqrt':
transform = SqrtStretch()
elif stretch == 'log':
transform = LogStretch()
elif stretch == 'linear':
transform = LinearStretch()
else:
raise InvalidInputError("Stretch {} is not supported!".format(stretch))
# Adding the scaling to the transform
if minmax_percent is not None:
transform += AsymmetricPercentileInterval(*minmax_percent)
if minmax_value is not None:
warnings.warn(
"Both minmax_percent and minmax_value are set, minmax_value will be ignored.",
InputWarning)
elif minmax_value is not None:
transform += ManualInterval(*minmax_value)
else: # Default, scale the entire image range to [0,1]
transform += MinMaxInterval()
# Performing the transform and then putting it into the pich range
pitch_array = transform(data_array)
zero_point = pitch_array[-1]
pitch_array = pitch_array[:-1]
pitch_array = np.multiply((center_pitch - pitch_range[0]) / zero_point,
pitch_array,
out=pitch_array) + pitch_range[0]
return pitch_array
