def dqm_check_single(n):
prev_time = start_time
is_dqm_zero = np.ones(ni, dtype=bool)
hdu_r = fits.open(work_dir + 'fits/best_single/' + single_dqm_fn[k][2])
for ii in range(0, ni):
# read the celestial coordinate
cel_coord = [[sex_cat_r[galaxy_r]['ALPHA_J2000'][ii+n*ni],
sex_cat_r[galaxy_r]['DELTA_J2000'][ii+n*ni]], [0, 0]]
# sky_coord = SkyCoord(arr_for_coord['ALPHA_J2000'][i],
# arr_for_coord['DELTA_J2000'][i], unit='deg')
# for every CCD
# lock.acquire()
# try:
for jj in range(1, len(hdu_r)):
# read WCS
w = wcs.WCS(hdu_r[jj].header)
pixcrd = w.wcs_world2pix(cel_coord, 1)
# if w.footprint_contains(sky_coord):
if (pixcrd[0][0] > 0) & (pixcrd[0][0] < hdu_r[jj].shape[1]) & \
(pixcrd[0][1] > 0) & (pixcrd[0][1] < hdu_r[jj].shape[0]):
dqm_fits = hdu_r[jj].data
# check the value of DQM
if dqm_fits[int(pixcrd[0][1])][int(pixcrd[0][0])] % 128:
# toggle on saturated bool array
is_dqm_zero[ii] = False
# finally:
# lock.release()
if ii % 1000 == 0:
print("--- %06.2f minutes ---" % ((time.time() - prev_time) / 60.0))
print("--- %d / %d - %d (single r)---" % (ii, n*ni, (n+1)*ni))
my_module.print_time()
prev_time = time.time()
hdu_r.close()
return is_dqm_zero
def dqm_check_single(n):
prev_time = start_time
is_dqm_zero = np.ones(ni, dtype=bool)
hdu_r = fits.open(work_dir + 'fits/best_single/' + single_dqm_fn[k][2])
for ii in range(0, ni):
# read the celestial coordinate
cel_coord = [[sex_cat_r[criteria_r]['ALPHA_J2000'][ii+n*ni],
sex_cat_r[criteria_r]['DELTA_J2000'][ii+n*ni]], [0, 0]]
for jj in range(1, len(hdu_r)):
# read WCS
w = wcs.WCS(hdu_r[jj].header)
pixcrd = w.wcs_world2pix(cel_coord, 1)
# if w.footprint_contains(sky_coord):
if (pixcrd[0][0] > 0) & (pixcrd[0][0] < hdu_r[jj].shape[1]) & \
(pixcrd[0][1] > 0) & (pixcrd[0][1] < hdu_r[jj].shape[0]):
dqm_fits = hdu_r[jj].data
# check the value of DQM
if k == 0: # Somehow A754 has value 7 (cosmic ray) in galaxies
if dqm_fits[int(pixcrd[0][1])][int(pixcrd[0][0])] % 7:
# toggle on saturated bool array
is_dqm_zero[ii] = False
else: # somehow other clusters have value 128 (?) in galaxies
if dqm_fits[int(pixcrd[0][1])][int(pixcrd[0][0])] % 128:
# toggle on saturated bool array
is_dqm_zero[ii] = False
if ii % 1000 == 0:
print("--- %06.2f minutes ---" % ((time.time() - prev_time) / 60.0))
print("--- %d / %d - %d (single r)---" % (ii, n*ni, (n+1)*ni))
my_module.print_time()
prev_time = time.time()
hdu_r.close()
return is_dqm_zero
ref_r['FROM_WHERE']
[i]) else 'green' # red for stack green for short
# color = 'darkorange'
# regFile.writelines("j2000; ellipse({:12.7f}, {:12.7f}, {:7.3f}\", {:7.3f}\", {:7.3f}) # "
# "color={} \n".format(
# coords_r[i].ra.value,
# coords_r[i].dec.value,
# ref_r['A_WORLD'][i] * 3600 * ref_r['KRON_RADIUS'][i],
# ref_r['B_WORLD'][i] * 3600 * ref_r['KRON_RADIUS'][i],
# 180 - ref_r['THETA_WORLD'][i],
# color))
regFile.writelines(
"j2000; ellipse({:12.7f}, {:12.7f}, {:7.3f}\", {:7.3f}\", {:7.3f}) # text=\'{}\' "
"color={} \n".format(
coords_r[i].ra.value, coords_r[i].dec.value,
ref_r['A_WORLD'][i] * 3600 * ref_r['KRON_RADIUS'][i],
ref_r['B_WORLD'][i] * 3600 * ref_r['KRON_RADIUS'][i],
180 - ref_r['THETA_WORLD'][i], i, color))
if i % 10000 == 0:
print("--- %06.2f minutes ---" %
(((time.time() - prev_time)) / 60.0))
print("--- %d / %d (write cat) ---" % (i, num_all))
my_module.print_time()
prev_time = time.time()
print(f"--- {ab.clusters[k]} Done ---")
my_module.print_time()
#from os import getcwd
#def print_path():
# print('The execution location: {0}'.format(getcwd()))
## VERSION 4 (Create my_script.py, my_module.py, my_module2.py)
## This is my_script.py
from my_module import print_time
from my_module2 import print_path
#help(print_time)
#print(print_time.__doc__)
print_time(print_path())
## This is my_module.py
#import datetime
#
#def print_time(my_path):
# a=datetime.datetime.now()
# print('Execution time: {0}'.format(a))
# print(my_path)
# return
## This is my_module2.py
#from os import getcwd
