def source_morphology(in_image, ext_name, **kwargs):
fo = fits.open(in_image, "append")
hdu = fo[ext_name]
segm_obj = SegmentationImage(fo["DEBLEND"].data)
errmap = fo["WEIGHT_MAP"].data
seg_props = fo["DEBLEND_PROPS"].data
im = hdu.data
bkg_estimator = photutils.MedianBackground()
bkg = photutils.Background2D(hdu.data, (50, 50),
bkg_estimator=bkg_estimator)
im -= bkg.background
npix = im.shape[0]
center_slice = segm_obj.data[int(npix / 2) - 2:int(npix / 2) + 2,
int(npix / 2) - 2:int(npix / 2) + 2]
central_index = np.where(seg_props["id"] == center_slice[0, 0])[0][0]
fo.flush()
fo.close()
source_morph = statmorph.SourceMorphology(im,
segm_obj,
central_index,
weightmap=errmap,
**kwargs)
return source_morph
def threshold(self, nsig=1.5, box_size=(50, 50), filter_size=(3, 3)):
"""
Generate threshold image
self.thresh_img is set in place
Args:
nsig (float, optional):
Primary threshold parameter
box_size (tuple):
Primary Background2D parameter
filter_size (tuple):
Primary Background2D parameter
Returns:
"""
if self.hdu is None:
self.load_image()
# Background
bkg_estimator = photutils.MedianBackground()
self.bkg = photutils.Background2D(self.hdu.data,
box_size,
filter_size=filter_size,
bkg_estimator=bkg_estimator,
exclude_percentile=self.exc_per)
# Threshold
self.thresh_img = self.bkg.background + (nsig *
self.bkg.background_rms)
def subtract_background(self,
subtract_min_value=True,
plot_background=False,
ax=None):
"""
A function to subtract the background for the FRD tests
INPUT:
subtract_min_value - subtracts the .min value (no negative numbers)
plot_background - if True, plots the estimated background with the meshes it used.
"""
self.aper = photutils.CircularAperture(positions=(self.x, self.y),
r=self.r)
# get the mask from the aperture
# hack
mask = self.aper.to_mask()[0].to_image(self.data.shape)
# use sigma clipping
sigma_clip = SigmaClip(sigma=3., iters=10)
bkg_estimator = photutils.MedianBackground()
self.bkg = photutils.Background2D(self.data,
self.box_size,
filter_size=(3, 3),
sigma_clip=sigma_clip,
bkg_estimator=bkg_estimator,
mask=mask,
edge_method="crop")
self.data_background = self.data - self.bkg.background
if subtract_min_value:
self.subtracted_value = self.data_background.min()
print("Subtracted min value:", self.subtracted_value)
self.data_background -= self.subtracted_value
if plot_background:
if ax == None:
self.fig, self.ax = plt.subplots()
else:
self.ax = ax
im = self.ax.imshow(self.bkg.background,
origin='lower',
cmap='Greys_r')
self.ax.set_xlim(0, self.bkg.background.shape[1])
self.ax.set_ylim(0, self.bkg.background.shape[0])
self.ax.set_title("Estimated Background", y=1.02)
self.ax.set_xlabel("X pixels")
self.ax.set_ylabel("Y pixels")
if ax == None:
# Only do this if ax is not supplied
# Don't know how to deal with this without passing the figure explicitly
self.fig.colorbar(im)
self.bkg.plot_meshes(outlines=True, color='#1f77b4', ax=self.ax)
return self.data_background
def sub_background(image: CCDData, filter_size: int = 27, box_size: int = 150):
"""
Perform background subtraction using photutils' median background estimator over a 2D mesh.
"""
binning = image.header['BINNING']
filter_size = int(filter_size / binning)
box_size = int(box_size / binning)
bkg_estimator = photutils.MedianBackground()
bkg = photutils.Background2D(image, (box_size, box_size),
filter_size=(filter_size, filter_size),
bkg_estimator=bkg_estimator)
sub = image.data - bkg.background
return sub
def detect_sources(in_image, ext_name, filt_wheel, **kwargs):
fo = fits.open(in_image, "append")
hdu = fo[ext_name]
# build kernel for pre-filtering. How big?
# don't assume redshift knowledge here
typical_kpc_per_arcsec = 8.0
kernel_kpc_fwhm = 5.0
kernel_arcsec_fwhm = kernel_kpc_fwhm / typical_kpc_per_arcsec
kernel_pixel_fwhm = kernel_arcsec_fwhm / hdu.header["PIXSIZE"]
sigma = kernel_pixel_fwhm * gaussian_fwhm_to_sigma
nsize = int(5 * kernel_pixel_fwhm)
kernel = Gaussian2DKernel(sigma, x_size=nsize, y_size=nsize)
bkg_estimator = photutils.MedianBackground()
bkg = photutils.Background2D(hdu.data, (50, 50),
bkg_estimator=bkg_estimator)
thresh = bkg.background + (5.0 * bkg.background_rms)
segmap_obj = photutils.detect_sources(hdu.data,
thresh,
npixels=5,
filter_kernel=kernel,
**kwargs)
if segmap_obj is None:
nhdu = fits.ImageHDU()
nhdu.header["EXTNAME"] = "SEGMAP"
fo.append(nhdu)
thdu = fits.BinTableHDU()
thdu.header["EXTNAME"] = "SEGMAP_PROPS"
fo.append(thdu)
fo.flush()
fo.close()
return None, None, None
else:
# Error image can be computed with photutils plus a GAIN keyword -- ratio of flux units to counts
gain = filt_wheel[hdu.header["FILTER"]][2]
errmap = calc_total_error(hdu.data,
bkg.background_rms,
effective_gain=gain)
segmap = segmap_obj.data
props = photutils.source_properties(hdu.data, segmap, errmap)
props_table = astropy.table.Table(props.to_table())
# these give problems given their format/NoneType objects
props_table.remove_columns([
"sky_centroid",
"sky_centroid_icrs",
"source_sum_err",
"background_sum",
"background_mean",
"background_at_centroid",
])
nhdu = fits.ImageHDU(segmap)
# save segmap and info
nhdu.header["EXTNAME"] = "SEGMAP"
fo.append(nhdu)
thdu = fits.BinTableHDU(props_table)
thdu.header["EXTNAME"] = "SEGMAP_PROPS"
fo.append(thdu)
fo.flush()
nhdu = fits.ImageHDU(errmap)
# save errmap
nhdu.header["EXTNAME"] = "WEIGHT_MAP"
fo.append(nhdu)
fo.flush()
fo.close()
return segmap_obj, kernel, errmap
def forced_phot(image,
wcs,
zp,
catalog_alt,
catalog_az,
catalog_mag,
catalog_id,
nside=8,
phot_params=None,
do_background=False,
return_table=False,
mjd=0.):
"""
Generate a map of the extinction on the sky
Parameters
----------
image : array
The image to find the extinction map from
wcs : wcs-like object
WCS describing the image. Note WCS RA,Dec will be interpreted as Az,Alt.
zp : float
The zeropoint of the image
catalog_alt : array
Altitude of stars expected to be in the image (degrees)
catalog_az : array
Azimuth of stars expected in the image (degrees)
catalog_mag : array
Magnitudes of stars expected in the image
nside : int
Healpixel nside to set resoltion of output map
phot_params : dict (None)
Dictionary holding common photometry kwargs. Loads defaults from default_phot_params
if None.
do_background : bool (False)
Do a 2D background model subtraction. Skipped by default because astropy is really slow.
return_table : bool (False)
If True, return the astropy table with the photometry, otherwise, return the extinction map.
Output
------
extinction : array
A healpixel array (where latitude and longitude are altitude and azimuth). Pixels
with no stars are filled with the healpixel mask value. Non-masked pixels have the
measured extinction in magnitudes.
"""
if phot_params is None:
phot_params = default_phot_params()
# Find the healpixel for each catalog star
lat = np.radians(90. - catalog_alt)
catalog_hp = hp.ang2pix(nside, lat, np.radians(catalog_az))
order = np.argsort(catalog_hp)
catalog_alt = catalog_alt[order]
catalog_az = catalog_az[order]
catalog_mag = catalog_mag[order]
catalog_id = catalog_id[order]
catalog_hp = catalog_hp[order]
catalog_x, catalog_y = wcs.all_world2pix(catalog_az, catalog_alt, 0)
good_transform = ~np.isnan(catalog_x)
# Find the x,y positions of helpix centers
lat, lon = hp.pix2ang(nside, np.arange(hp.nside2npix(nside)))
hp_alt = np.degrees(np.pi / 2. - lat)
hp_az = np.degrees(lon)
hp_x, hp_y = wcs.all_world2pix(hp_az, hp_alt, 0)
# Run the photometry at the expected catalog positions
if do_background:
sigma_clip = phu.SigmaClip(sigma=phot_params['bk_clip_sigma'],
iters=phot_params['bk_iter'])
bkg_estimator = phu.MedianBackground()
bkg = phu.Background2D(
image,
(phot_params['background_size'], phot_params['background_size']),
filter_size=(phot_params['bk_filter_size'],
phot_params['bk_filter_size']),
sigma_clip=sigma_clip,
bkg_estimator=bkg_estimator)
bk_img = image - bkg.background
else:
bk_img = image
positions = list(zip(catalog_x[good_transform], catalog_y[good_transform]))
apertures = phu.CircularAperture(positions, r=phot_params['apper_r'])
annulus_apertures = phu.CircularAnnulus(positions,
r_in=phot_params['ann_r_in'],
r_out=phot_params['ann_r_out'])
apers = [apertures, annulus_apertures]
phot_table = phu.aperture_photometry(bk_img, apers)
bkg_mean = phot_table['aperture_sum_1'] / annulus_apertures.area()
bkg_sum = bkg_mean * apertures.area()
final_sum = phot_table['aperture_sum_0'] - bkg_sum
phot_table['residual_aperture_sum'] = final_sum
phot_table['catalog_id'] = catalog_id[good_transform]
phot_table['residual_aperture_mag'] = -2.5 * np.log10(final_sum) + zp
detected = np.where(final_sum > 0)
mag_difference = phot_table['residual_aperture_mag'][
detected] - catalog_mag[good_transform][detected]
phot_table['mag_difference'] = np.zeros(
phot_table['residual_aperture_mag'].data.size, dtype=float)
phot_table['mjd'] = np.zeros(phot_table['residual_aperture_mag'].data.size,
dtype=float)
phot_table['mag_difference'][detected] = mag_difference
phot_table['mjd'] = mjd
bins = np.arange(hp.nside2npix(nside) + 1) - 0.5
result, be, bn = binned_statistic(catalog_hp[good_transform][detected],
mag_difference,
bins=bins)
if return_table:
return phot_table, result
else:
return result
def getBackground(data,
fitsfilename,
bkg_method='2d',
box_size=128,
params=None,
locs=None):
if bkg_method == '2d':
bkg_estimator = pt.MedianBackground()
data_mask = (data < 1.1 * np.median(data))
bkg_maskarr = np.ma.array(data, mask=~data_mask)
bkg = pt.Background2D(bkg_maskarr, (box_size, box_size),
filter_size=(3, 3),
sigma_clip=None,
bkg_estimator=bkg_estimator)
bkg_median = bkg.background_median
plt.imshow(bkg.background,
origin='lower',
vmin=bkg_median - 100,
vmax=bkg_median + 100,
cmap='Greys')
plt.colorbar(orientation='horizontal')
if not os.path.exists(
os.path.join(os.path.dirname(fitsfilename), 'background')):
os.makedirs(
os.path.join(os.path.dirname(fitsfilename), 'background'))
savepath = os.path.join(
os.path.join(os.path.dirname(fitsfilename), 'background'),
'bkg_' + os.path.split(fitsfilename[:-5])[-1] + '.png')
plt.savefig(savepath)
plt.clf()
plt.close()
elif bkg_method == 'aperture':
bkg_arr = data.copy()
bkg = []
for loc in locs:
bkg_arr[loc[0] - params['sky_rad_in']:loc[0] +
params['sky_rad_in'],
loc[1] - params['sky_rad_in']:loc[1] +
params['sky_rad_in']] = np.nan
bkg.append(
np.nanmedian(bkg_arr[loc[0] - params['sky_rad_out']:loc[0] +
params['sky_rad_out'],
loc[1] - params['sky_rad_out']:loc[1] +
params['sky_rad_out']].flatten()))
plt.imshow(bkg_arr,
origin='lower',
vmin=np.nanmedian(bkg_arr) - 100,
vmax=np.nanmedian(bkg_arr) + 100)
plt.colorbar()
for loc in locs:
plt.gca().add_patch(
patch.Rectangle((loc[1] - params['sky_rad_out'],
loc[0] - params['sky_rad_out']),
2 * params['sky_rad_out'],
2 * params['sky_rad_out'],
color='k',
alpha=0.5))
if not os.path.exists(
os.path.join(os.path.dirname(fitsfilename), 'background')):
os.makedirs(
os.path.join(os.path.dirname(fitsfilename), 'background'))
savepath = os.path.join(
os.path.join(os.path.dirname(fitsfilename), 'background'),
'bkg_' + os.path.split(fitsfilename[:-5])[-1] + '.png')
plt.savefig(savepath)
plt.clf()
plt.close()
bkg = np.array(bkg)
bkg = BkgWrapper(bkg)
elif bkg_method == 'median':
return BkgWrapper(np.median(data.flatten()))
elif bkg_method == 'None':
return None
else:
raise ValueError('Method %s not supported.' % bkg_method)
return bkg
