Newer
Older
import galsim
import os
import numpy as np
from astropy.table import Table
from numpy.random import Generator, PCG64
from astropy.io import fits
from datetime import datetime
from ObservationSim.Instrument.Chip import Effects as effects
from ObservationSim.Instrument.FocalPlane import FocalPlane
from ObservationSim.Config.Header import generatePrimaryHeader, generateExtensionHeader
try:
import importlib.resources as pkg_resources
except ImportError:
# Try backported to PY<37 'importlib_resources'
import importlib_resources as pkg_resources
Fang Yuedong
committed
def __init__(self, chipID, ccdEffCurve_dir=None, CRdata_dir=None, sls_dir=None, config=None, treering_func=None, logger=None):
# Get focal plane (instance of paraent class) info
# TODO: use chipID to config individual chip?
super().__init__()
self.npix_x = 9216
self.npix_y = 9232
self.read_noise = 5.0 # e/pix
self.dark_noise = 0.02 # e/pix/s
self.pix_scale = 0.074 # pixel scale
self.gain = float(config["ins_effects"]["gain"])
self.bias_level = float(config["ins_effects"]["bias_level"])
self.exptime = float(config["obs_setting"]["exp_time"]) # second
self.dark_exptime = float(config["ins_effects"]['dark_exptime'])
self.flat_exptime = float(config["ins_effects"]['flat_exptime'])
self.readout_time = float(config["ins_effects"]['readout_time'])
self.full_well = int(config["ins_effects"]["full_well"])
Fang Yuedong
committed
self.logger = logger
# A chip ID must be assigned
self.chipID = int(chipID)
self._getChipRowCol()
# Get corresponding filter info
self.filter_id, self.filter_type = self.getChipFilter()
self.survey_type = self._getSurveyType()
# Get boundary (in pix)
self.bound = self.getChipLim()
self.ccdEffCurve_dir = ccdEffCurve_dir
self.CRdata_dir = CRdata_dir
# self.sls_conf = os.path.join(self.sls_dir, self.getChipSLSConf())
slsconfs = self.getChipSLSConf()
if np.size(slsconfs) == 1:
# self.sls_conf = [os.path.join(self.sls_dir, slsconfs)]
with pkg_resources.path('ObservationSim.Instrument.data.sls_conf', slsconfs) as conf_path:
self.sls_conf = str(conf_path)
# self.sls_conf = [os.path.join(self.sls_dir, slsconfs[0]), os.path.join(self.sls_dir, slsconfs[1])]
self.sls_conf = []
with pkg_resources.path('ObservationSim.Instrument.data.sls_conf', slsconfs[0]) as conf_path:
self.sls_conf.append(str(conf_path))
with pkg_resources.path('ObservationSim.Instrument.data.sls_conf', slsconfs[1]) as conf_path:
self.sls_conf.append(str(conf_path))
self.effCurve = self._getChipEffCurve(self.filter_type)
self._getCRdata()
# Define the sensor
if config["ins_effects"]["bright_fatter"] == True and self.survey_type == "photometric":
self.sensor = galsim.SiliconSensor(strength=config["ins_effects"]["df_strength"], treering_func=treering_func)
else:
self.sensor = galsim.Sensor()
# def _getChipRowCol(self):
# self.rowID = (self.chipID - 1) // 5 + 1
# self.colID = (self.chipID - 1) % 5 + 1
def _getChipRowCol(self):
self.rowID, self.colID = self.getChipRowCol(self.chipID)
def getChipRowCol(self, chipID):
rowID = ((chipID - 1) % 5) + 1
colID = 6 - ((chipID - 1) // 5)
return rowID, colID
def _getSurveyType(self):
if self.filter_type in ["GI", "GV", "GU"]:
return "spectroscopic"
else:
return "photometric"
def _getChipEffCurve(self, filter_type):
# CCD efficiency curves
if filter_type in ['nuv', 'u', 'GU']: filename = 'UV0.txt'
if filter_type in ['g', 'r', 'GV']: filename = 'Astro_MB.txt'
if filter_type in ['i', 'z', 'y', 'GI']: filename = 'Basic_NIR.txt'
# Mirror efficiency:
# if filter_type == 'nuv': mirror_eff = 0.54
# if filter_type == 'u': mirror_eff = 0.68
# if filter_type in ['g', 'r', 'i', 'z', 'y']: mirror_eff = 0.8
# if filter_type in ['GU', 'GV', 'GI']: mirror_eff = 1. # Not sure if this is right
# path = os.path.join(self.ccdEffCurve_dir, filename)
# table = Table.read(path, format='ascii')
with pkg_resources.path('ObservationSim.Instrument.data.ccd', filename) as ccd_path:
table = Table.read(ccd_path, format='ascii')
# throughput = galsim.LookupTable(x=table['col1'], f=table['col2']*mirror_eff, interpolant='linear')
throughput = galsim.LookupTable(x=table['col1'], f=table['col2'], interpolant='linear')
bandpass = galsim.Bandpass(throughput, wave_type='nm')
return bandpass
def _getCRdata(self):
# path = os.path.join(self.CRdata_dir, 'wfc-cr-attachpixel.dat')
# self.attachedSizes = np.loadtxt(path)
with pkg_resources.path('ObservationSim.Instrument.data', "wfc-cr-attachpixel.dat") as cr_path:
self.attachedSizes = np.loadtxt(cr_path)
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
def getChipFilter(self, chipID=None, filter_layout=None):
"""Return the filter index and type for a given chip #(chipID)
"""
filter_type_list = ["nuv","u", "g", "r", "i","z","y","GU", "GV", "GI"]
# TODO: maybe a more elegent way other than hard coded?
# e.g. use something like a nested dict:
if filter_layout is not None:
return filter_layout[chipID][0], filter_layout[chipID][1]
if chipID == None:
chipID = self.chipID
# updated configurations
# if chipID>30 or chipID<1: raise ValueError("!!! Chip ID: [1,30]")
# if chipID in [10, 15, 16, 21]: filter_type = 'y'
# if chipID in [11, 20]: filter_type = "z"
# if chipID in [9, 22]: filter_type = "i"
# if chipID in [12, 19]: filter_type = "u"
# if chipID in [7, 24]: filter_type = "r"
# if chipID in [14, 13, 18, 17]: filter_type = "nuv"
# if chipID in [8, 23]: filter_type = "g"
# if chipID in [6, 5, 25, 26]: filter_type = "GI"
# if chipID in [27, 30, 1, 4]: filter_type = "GV"
# if chipID in [28, 29, 2, 3]: filter_type = "GU"
if chipID in [6, 15, 16, 25]: filter_type = "y"
if chipID in [11, 20]: filter_type = "z"
if chipID in [7, 24]: filter_type = "i"
if chipID in [14, 17]: filter_type = "u"
if chipID in [9, 22]: filter_type = "r"
if chipID in [12, 13, 18, 19]: filter_type = "nuv"
if chipID in [8, 23]: filter_type = "g"
if chipID in [1, 10, 21, 30]: filter_type = "GI"
if chipID in [2, 5, 26, 29]: filter_type = "GV"
if chipID in [3, 4, 27, 28]: filter_type = "GU"
filter_id = filter_type_list.index(filter_type)
return filter_id, filter_type
def getChipLim(self, chipID=None):
"""Calculate the edges in pixel for a given CCD chip on the focal plane
NOTE: There are 5*4 CCD chips in the focus plane for photometric observation.
Parameters:
chipID: int
the index of the chip
Returns:
A galsim BoundsD object
"""
# if chipID == None:
# chipID = self.chipID
# gx = self.npix_gap_x
# gy1, gy2 = self.npix_gap_y
# # xlim of a given ccd chip
# xrem = (chipID-1)%self.nchip_x - self.nchip_x // 2
# xcen = (self.npix_x + gx) * xrem
# nx0 = xcen - self.npix_x//2 + 1
# nx1 = xcen + self.npix_x//2
# # ylim of a given ccd chip
# yrem = 2*((chipID-1)//self.nchip_x) - (self.nchip_y-1)
# ycen = (self.npix_y//2 + gy1//2) * yrem
# if chipID <= 6: ycen = (self.npix_y//2 + gy1//2) * yrem - (gy2-gy1)
# if chipID >= 25: ycen = (self.npix_y//2 + gy1//2) * yrem + (gy2-gy1)
# ny0 = ycen - self.npix_y//2 + 1
# ny1 = ycen + self.npix_y//2
if chipID == None:
chipID = self.chipID
rowID, colID = self.rowID, self.colID
else:
rowID, colID = self.getChipRowCol(chipID)
gx1, gx2 = self.npix_gap_x
gy = self.npix_gap_y
# xlim of a given CCD chip
xrem = 2*(colID - 1) - (self.nchip_x - 1)
xcen = (self.npix_x//2 + gx1//2) * xrem
if chipID >= 26 or chipID == 21:
xcen = (self.npix_x//2 + gx1//2) * xrem - (gx2-gx1)
if chipID <= 5 or chipID == 10:
xcen = (self.npix_x//2 + gx1//2) * xrem + (gx2-gx1)
nx0 = xcen - self.npix_x//2 + 1
nx1 = xcen + self.npix_x//2
# ylim of a given CCD chip
yrem = (rowID - 1) - self.nchip_y // 2
ycen = (self.npix_y + gy) * yrem
ny0 = ycen - self.npix_y//2 + 1
ny1 = ycen + self.npix_y//2
return galsim.BoundsD(nx0-1, nx1-1, ny0-1, ny1-1)
def getSkyCoverage(self, wcs):
return super().getSkyCoverage(wcs, self.bound.xmin, self.bound.xmax, self.bound.ymin, self.bound.ymax)
def getSkyCoverageEnlarged(self, wcs, margin=0.5):
"""The enlarged sky coverage of the chip
"""
margin /= 60.0
bound = self.getSkyCoverage(wcs)
return galsim.BoundsD(bound.xmin - margin, bound.xmax + margin, bound.ymin - margin, bound.ymax + margin)
def isContainObj(self, ra_obj, dec_obj, wcs=None, margin=1):
# magin in number of pix
if wcs is None:
wcs = self.img.wcs
pos_obj = wcs.toImage(galsim.CelestialCoord(ra=ra_obj*galsim.degrees, dec=dec_obj*galsim.degrees))
xmin, xmax = self.bound.xmin - margin, self.bound.xmax + margin
ymin, ymax = self.bound.ymin - margin, self.bound.ymax + margin
if (pos_obj.x - xmin) * (pos_obj.x - xmax) > 0.0 or (pos_obj.y - ymin) * (pos_obj.y - ymax) > 0.0:
return False
return True
def getChipNoise(self, exptime=150.0):
noise = self.dark_noise * exptime + self.read_noise**2
return noise
def getChipSLSConf(self):
confFile = ''
if self.chipID == 1: confFile = ['CSST_GI2.conf', 'CSST_GI1.conf']
if self.chipID == 2: confFile = ['CSST_GV4.conf', 'CSST_GV3.conf']
if self.chipID == 3: confFile = ['CSST_GU2.conf', 'CSST_GU1.conf']
if self.chipID == 4: confFile = ['CSST_GU4.conf', 'CSST_GU3.conf']
if self.chipID == 5: confFile = ['CSST_GV2.conf', 'CSST_GV1.conf']
if self.chipID == 10: confFile = ['CSST_GI4.conf', 'CSST_GI3.conf']
if self.chipID == 21: confFile = ['CSST_GI6.conf', 'CSST_GI5.conf']
if self.chipID == 26: confFile = ['CSST_GV8.conf', 'CSST_GV7.conf']
if self.chipID == 27: confFile = ['CSST_GU6.conf', 'CSST_GU5.conf']
if self.chipID == 28: confFile = ['CSST_GU8.conf', 'CSST_GU7.conf']
if self.chipID == 29: confFile = ['CSST_GV6.conf', 'CSST_GV5.conf']
if self.chipID == 30: confFile = ['CSST_GI8.conf', 'CSST_GI7.conf']
return confFile
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
def generateHeader(self, ra_cen, dec_cen, img_rot, im_type, pointing_ID, date_obs, time_obs, exptime=150.):
h_prim = generatePrimaryHeader(
xlen=self.npix_x,
ylen=self.npix_y,
pointNum = str(pointing_ID),
ra=ra_cen,
dec=dec_cen,
psize=self.pix_scale,
row_num=self.rowID,
col_num=self.colID,
date=date_obs,
time_obs=time_obs,
im_type = im_type,
exptime=exptime
)
h_ext = generateExtensionHeader(
xlen=self.npix_x,
ylen=self.npix_y,
ra=ra_cen,
dec=dec_cen,
pa=img_rot.deg,
gain=self.gain,
readout=self.read_noise,
dark=self.dark_noise,
saturation=90000,
psize=self.pix_scale,
row_num=self.rowID,
col_num=self.colID,
extName='raw')
return h_prim, h_ext
def outputCal(self, img, ra_cen, dec_cen, img_rot, im_type, pointing_ID, date_obs, time_obs, output_dir, exptime=150.):
h_prim, h_ext = self.generateHeader(
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
im_type=im_type,
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
exptime=exptime)
hdu1 = fits.PrimaryHDU(header=h_prim)
hdu2 = fits.ImageHDU(img.array, header=h_ext)
hdu1 = fits.HDUList([hdu1, hdu2])
fname = os.path.join(output_dir, h_prim['FILENAME']+'.fits')
hdu1.writeto(fname, output_verify='ignore', overwrite=True)
Fang Yuedong
committed
def addEffects(self, config, img, chip_output, filt, ra_cen, dec_cen, img_rot, exptime=150., pointing_ID=0, timestamp_obs=1621915200, pointing_type='MS', sky_map=None, tel=None, logger=None):
SeedGainNonuni=int(config["random_seeds"]["seed_gainNonUniform"])
SeedBiasNonuni=int(config["random_seeds"]["seed_biasNonUniform"])
SeedRnNonuni = int(config["random_seeds"]["seed_rnNonUniform"])
SeedBadColumns = int(config["random_seeds"]["seed_badcolumns"])
SeedDefective = int(config["random_seeds"]["seed_defective"])
SeedCosmicRay = int(config["random_seeds"]["seed_CR"])
fullwell = int(config["ins_effects"]["full_well"])
if config["ins_effects"]["add_hotpixels"] == True:
Fang Yuedong
committed
self.logger = logger
# Add sky background
sky_map = filt.getSkyNoise(exptime=self.exptime)
elif img.array.shape != sky_map.shape:
raise ValueError("The shape img and sky_map must be equal.")
elif tel is not None: # If sky_map is given in flux
sky_map = sky_map * tel.pupil_area * self.exptime
img += sky_map
del sky_map
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Creating and applying Flat-Fielding")
msg = str(img.bounds)
self.logger.info(msg)
else:
print(" Creating and applying Flat-Fielding", flush=True)
print(img.bounds, flush=True)
if self.survey_type == "photometric":
img *= flat_normal
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Apply shutter effect")
else:
print(" Apply shutter effect", flush=True)
shuttimg = effects.ShutterEffectArr(img, t_shutter=1.3, dist_bearing=735, dt=1E-3) # shutter effect normalized image for this chip
if self.survey_type == "photometric":
img *= shuttimg
if config["output_setting"]["shutter_output"] == True: # output 16-bit shutter effect image with pixel value <=65535
shutt_gsimg = galsim.ImageUS(shuttimg*6E4)
shutt_gsimg.write("%s/ShutterEffect_%s_1.fits" % (chip_output.subdir, self.chipID))
del shutt_gsimg
del shuttimg
# Add Poisson noise
seed = int(config["random_seeds"]["seed_poisson"]) + pointing_ID*30 + self.chipID
rng_poisson = galsim.BaseDeviate(seed)
poisson_noise = galsim.PoissonNoise(rng_poisson, sky_level=0.)
img.addNoise(poisson_noise)
if config["ins_effects"]["cosmic_ray"] == True and pointing_type=='MS':
Fang Yuedong
committed
if self.logger is not None:
self.logger.info((" Adding Cosmic-Ray"))
else:
print(" Adding Cosmic-Ray", flush=True)
exTime=self.exptime+0.5*self.readout_time,
cr_pixelRatio=0.003*(self.exptime+0.5*self.readout_time)/600.,
seed=SeedCosmicRay+pointing_ID*30+self.chipID) # seed: obj-imaging:+0; bias:+1; dark:+2; flat:+3;
img += cr_map
cr_map[cr_map > 65535] = 65535
cr_map[cr_map < 0] = 0
crmap_gsimg = galsim.Image(cr_map, dtype=np.uint16)
# crmap_gsimg.write("%s/CosmicRay_%s_1.fits" % (chip_output.subdir, self.chipID))
# crmap_gsimg.write("%s/CosmicRay_%s.fits" % (chip_output.subdir, self.chipID))
datetime_obs = datetime.fromtimestamp(timestamp_obs)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
self.outputCal(
img=crmap_gsimg,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
im_type='CRS',
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
output_dir=chip_output.subdir,
# Apply PRNU effect and output PRNU flat file:
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying PRNU effect")
else:
print(" Applying PRNU effect", flush=True)
prnu_img = effects.PRNU_Img(
xsize=self.npix_x,
ysize=self.npix_y,
sigma=0.01,
seed=int(config["random_seeds"]["seed_prnu"]+self.chipID))
img *= prnu_img
prnu_img.write("%s/FlatImg_PRNU_%s.fits" % (chip_output.subdir,self.chipID))
del prnu_img
# Add dark current
dark_noise = galsim.DeviateNoise(galsim.PoissonDeviate(rng_poisson, self.dark_noise*(self.exptime+0.5*self.readout_time)))
img.addNoise(dark_noise)
# Add Hot Pixels or/and Dead Pixels
rgbadpix = Generator(PCG64(int(SeedDefective+self.chipID)))
badfraction = 5E-5*(rgbadpix.random()*0.5+0.7)
img = effects.DefectivePixels(img, IfHotPix=BoolHotPix, IfDeadPix=BoolDeadPix, fraction=badfraction, seed=SeedDefective+self.chipID, biaslevel=0)
# Apply Bad lines
Fang Yuedong
committed
img = effects.BadColumns(img, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Adding Bias level and 16-channel non-uniformity")
else:
print(" Adding Bias level and 16-channel non-uniformity")
Fang Yuedong
committed
seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
# Apply Nonlinearity on the chip image
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying Non-Linearity on the chip image")
else:
print(" Applying Non-Linearity on the chip image", flush=True)
img = effects.NonLinearity(GSImage=img, beta1=5.e-7, beta2=0)
# Apply CCD Saturation & Blooming
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying CCD Saturation & Blooming")
else:
print(" Applying CCD Saturation & Blooming")
img = effects.SaturBloom(GSImage=img, nsect_x=1, nsect_y=1, fullwell=fullwell)
# Apply CTE Effect
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Apply CTE Effect")
else:
print(" Apply CTE Effect")
img = effects.CTE_Effect(GSImage=img, threshold=27)
# Add Read-out Noise
if config["ins_effects"]["add_readout"] == True:
seed = int(config["random_seeds"]["seed_readout"]) + pointing_ID*30 + self.chipID
rng_readout = galsim.BaseDeviate(seed)
readout_noise = galsim.GaussianNoise(rng=rng_readout, sigma=self.read_noise)
img.addNoise(readout_noise)
# Apply Gain & Quantization
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying Gain (and 16 channel non-uniformity) & Quantization")
else:
print(" Applying Gain (and 16 channel non-uniformity) & Quantization", flush=True)
img = effects.ApplyGainNonUniform16(
img, gain=self.gain,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedGainNonuni+self.chipID,
logger=self.logger)
img.array[img.array > 65535] = 65535
img.replaceNegative(replace_value=0)
img.quantize()
######################################################################################
# Output images for calibration pointing
######################################################################################
if config["ins_effects"]["add_bias"] == True and config["output_setting"]["bias_output"] == True and pointing_type=='CAL':
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Output N frame Bias files")
else:
print(" Output N frame Bias files", flush=True)
for i in range(NBias):
BiasCombImg, BiasTag = effects.MakeBiasNcomb(
self.npix_x, self.npix_y,
Fang Yuedong
committed
seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
if config["ins_effects"]["cosmic_ray"] == True:
if config["ins_effects"]["cray_differ"] == True:
cr_map, cr_event_num = effects.produceCR_Map(
xLen=self.npix_x, yLen=self.npix_y,
exTime=0.01,
gain=self.gain,
attachedSizes=self.attachedSizes,
seed=SeedCosmicRay+pointing_ID*30+self.chipID+1)
# seed: obj-imaging:+0; bias:+1; dark:+2; flat:+3;
BiasCombImg += cr_map
del cr_map
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying Non-Linearity on the Bias image")
else:
print(" Applying Non-Linearity on the Bias image", flush=True)
BiasCombImg = effects.NonLinearity(GSImage=BiasCombImg, beta1=5.e-7, beta2=0)
# Apply Bad lines
Fang Yuedong
committed
BiasCombImg = effects.BadColumns(BiasCombImg-float(config["ins_effects"]["bias_level"])+5, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger) + float(config["ins_effects"]["bias_level"])-5
BiasCombImg = effects.ApplyGainNonUniform16(BiasCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedGainNonuni+self.chipID,
logger=self.logger)
# overscan=float(config["ins_effects"]["bias_level"])-2, gain=self.gain,
# widthl=27, widthr=27, widtht=8, widthb=8)
BiasCombImg.replaceNegative(replace_value=0)
BiasCombImg.quantize()
BiasCombImg = galsim.ImageUS(BiasCombImg)
# BiasCombImg.write("%s/BiasImg_%s_%s_%s.fits" % (chip_output.subdir, BiasTag, self.chipID, i+1))
datetime_obs = datetime.fromtimestamp(timestamp_obs)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
timestamp_obs += 10 * 60
self.outputCal(
img=BiasCombImg,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
output_dir=chip_output.subdir,
exptime=0.0)
del BiasCombImg
# Export combined (ncombine, Vignetting + PRNU) & single vignetting flat-field file
if config["ins_effects"]["flat_fielding"] == True and config["output_setting"]["flat_output"] == True and pointing_type=='CAL':
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Output N frame Flat-Field files")
else:
print(" Output N frame Flat-Field files", flush=True)
NFlat = int(config["ins_effects"]["NFlat"])
if config["ins_effects"]["add_bias"] == True:
darklevel = self.dark_noise*(self.flat_exptime+0.5*self.readout_time)
for i in range(NFlat):
FlatSingle = flat_img * prnu_img + darklevel
FlatCombImg, FlatTag = effects.MakeFlatNcomb(
flat_single_image=FlatSingle,
ncombine=1,
read_noise=self.read_noise,
gain=1,
overscan=overscan,
biaslevel=0,
Fang Yuedong
committed
seed_bias=SeedDefective+self.chipID,
logger=self.logger
if config["ins_effects"]["cosmic_ray"] == True:
if config["ins_effects"]["cray_differ"] == True:
cr_map, cr_event_num = effects.produceCR_Map(
exTime=self.flat_exptime+0.5*self.readout_time,
cr_pixelRatio=0.003*(self.flat_exptime+0.5*self.readout_time)/150.,
gain=self.gain,
attachedSizes=self.attachedSizes,
seed=SeedCosmicRay+pointing_ID*30+self.chipID+3)
# seed: obj-imaging:+0; bias:+1; dark:+2; flat:+3;
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying Non-Linearity on the Flat image")
else:
print(" Applying Non-Linearity on the Flat image", flush=True)
FlatCombImg = effects.NonLinearity(GSImage=FlatCombImg, beta1=5.e-7, beta2=0)
FlatCombImg = effects.CTE_Effect(GSImage=FlatCombImg, threshold=3)
# Add Hot Pixels or/and Dead Pixels
rgbadpix = Generator(PCG64(int(SeedDefective+self.chipID)))
badfraction = 5E-5*(rgbadpix.random()*0.5+0.7)
FlatCombImg = effects.DefectivePixels(FlatCombImg, IfHotPix=BoolHotPix, IfDeadPix=BoolDeadPix, fraction=badfraction, seed=SeedDefective+self.chipID, biaslevel=0)
Fang Yuedong
committed
FlatCombImg = effects.BadColumns(FlatCombImg, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
# Add Bias level
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Adding Bias level and 16-channel non-uniformity")
else:
print(" Adding Bias level and 16-channel non-uniformity")
FlatCombImg = effects.AddBiasNonUniform16(FlatCombImg,
bias_level=biaslevel,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
# Add Read-out Noise
if config["ins_effects"]["add_readout"] == True:
seed = int(config["random_seeds"]["seed_readout"]) + pointing_ID*30 + self.chipID
rng_readout = galsim.BaseDeviate(seed)
readout_noise = galsim.GaussianNoise(rng=rng_readout, sigma=self.read_noise)
FlatCombImg.addNoise(readout_noise)
FlatCombImg = effects.ApplyGainNonUniform16(FlatCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedGainNonuni+self.chipID,
logger=self.logger)
# FlatCombImg = effects.AddOverscan(FlatCombImg, overscan=overscan, gain=self.gain, widthl=27, widthr=27, widtht=8, widthb=8)
FlatCombImg.replaceNegative(replace_value=0)
FlatCombImg.quantize()
FlatCombImg = galsim.ImageUS(FlatCombImg)
# FlatCombImg.write("%s/FlatImg_%s_%s_%s.fits" % (chip_output.subdir, FlatTag, self.chipID, i+1))
datetime_obs = datetime.fromtimestamp(timestamp_obs)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
timestamp_obs += 10 * 60
self.outputCal(
img=FlatCombImg,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
output_dir=chip_output.subdir,
exptime=self.flat_exptime)
del FlatCombImg, FlatSingle, prnu_img
# flat_img.replaceNegative(replace_value=0)
# flat_img.quantize()
# galsim.ImageUS(flat_img).write("%s/FlatImg_Vignette_%s.fits" % (chip_output.subdir, self.chipID))
del flat_img
# Export Dark current images
if config["ins_effects"]["add_dark"] == True and config["output_setting"]["dark_output"] == True and pointing_type=='CAL':
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Output N frame Dark Current files")
else:
print(" Output N frame Dark Current files", flush=True)
NDark = int(config["ins_effects"]["NDark"])
if config["ins_effects"]["add_bias"] == True:
biaslevel = 0
overscan = 0
for i in range(NDark):
DarkCombImg, DarkTag = effects.MakeDarkNcomb(
self.npix_x, self.npix_y,
overscan=overscan, bias_level=0, darkpsec=0.02, exptime=self.dark_exptime+0.5*self.readout_time,
Fang Yuedong
committed
gain=1, seed_bias=SeedBiasNonuni+self.chipID,
logger=self.logger)
if config["ins_effects"]["cosmic_ray"] == True:
if config["ins_effects"]["cray_differ"] == True:
cr_map, cr_event_num = effects.produceCR_Map(
exTime=self.dark_exptime+0.5*self.readout_time,
cr_pixelRatio=0.003*(self.dark_exptime+0.5*self.readout_time)/150.,
gain=self.gain,
attachedSizes=self.attachedSizes,
seed=SeedCosmicRay+pointing_ID*30+self.chipID+2)
# seed: obj-imaging:+0; bias:+1; dark:+2; flat:+3;
cr_map[cr_map > 65535] = 65535
cr_map[cr_map < 0] = 0
crmap_gsimg = galsim.Image(cr_map, dtype=np.uint16)
del cr_map
datetime_obs = datetime.fromtimestamp(timestamp_obs)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
self.outputCal(
img=crmap_gsimg,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
im_type='CRD',
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
output_dir=chip_output.subdir,
exptime=self.dark_exptime)
del crmap_gsimg
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Applying Non-Linearity on the Dark image")
else:
print(" Applying Non-Linearity on the Dark image", flush=True)
DarkCombImg = effects.NonLinearity(GSImage=DarkCombImg, beta1=5.e-7, beta2=0)
DarkCombImg = effects.CTE_Effect(GSImage=DarkCombImg, threshold=3)
# Add Hot Pixels or/and Dead Pixels
rgbadpix = Generator(PCG64(int(SeedDefective+self.chipID)))
badfraction = 5E-5*(rgbadpix.random()*0.5+0.7)
DarkCombImg = effects.DefectivePixels(DarkCombImg, IfHotPix=BoolHotPix, IfDeadPix=BoolDeadPix, fraction=badfraction, seed=SeedDefective+self.chipID, biaslevel=0)
Fang Yuedong
committed
DarkCombImg = effects.BadColumns(DarkCombImg, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
# Add Bias level
Fang Yuedong
committed
if self.logger is not None:
self.logger.info(" Adding Bias level and 16-channel non-uniformity")
else:
print(" Adding Bias level and 16-channel non-uniformity")
DarkCombImg = effects.AddBiasNonUniform16(DarkCombImg,
bias_level=biaslevel,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
# Add Read-out Noise
if config["ins_effects"]["add_readout"] == True:
seed = int(config["random_seeds"]["seed_readout"]) + pointing_ID*30 + self.chipID
rng_readout = galsim.BaseDeviate(seed)
readout_noise = galsim.GaussianNoise(rng=rng_readout, sigma=self.read_noise)
DarkCombImg.addNoise(readout_noise)
DarkCombImg = effects.ApplyGainNonUniform16(
DarkCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
Fang Yuedong
committed
seed=SeedGainNonuni+self.chipID,
logger=self.logger)
# DarkCombImg = effects.AddOverscan(
# DarkCombImg,
# overscan=overscan, gain=self.gain,
# widthl=27, widthr=27, widtht=8, widthb=8)
DarkCombImg.replaceNegative(replace_value=0)
DarkCombImg.quantize()
DarkCombImg = galsim.ImageUS(DarkCombImg)
# DarkCombImg.write("%s/DarkImg_%s_%s_%s.fits" % (chip_output.subdir, DarkTag, self.chipID, i+1))
datetime_obs = datetime.fromtimestamp(timestamp_obs)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
timestamp_obs += 10 * 60
self.outputCal(
img=DarkCombImg,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
pointing_ID=pointing_ID,
date_obs=date_obs,
time_obs=time_obs,
output_dir=chip_output.subdir,
exptime=self.dark_exptime)
del DarkCombImg
# img = galsim.ImageUS(img)
# # 16 output channel, with each a single image file
# print(" 16 Output Channel simulation")
# for coli in [0, 1]:
# for rowi in range(8):
# sub_img = effects.readout16(
# GSImage=img,
# rowi=rowi,
# coli=coli,
# overscan_value=self.overscan)
# rowcoltag = str(rowi) + str(coli)
# img_name_root = chip_output.img_name.split(".")[0]
# sub_img.write("%s/%s_%s.fits" % (chip_output.subdir, img_name_root, rowcoltag))
# del sub_img