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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
from ObservationSim.Instrument._util import rotate_conterclockwise
try:
import importlib.resources as pkg_resources
except ImportError:
# Try backported to PY<37 'importlib_resources'
import importlib_resources as pkg_resources
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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.pix_scale = 0.074 # pixel scale
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self.nsecy = 2
self.nsecx = 8
self.gain_channel = np.ones(self.nsecy* self.nsecx)
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self.logger = logger
# Get corresponding filter info
self.filter_id, self.filter_type = self.getChipFilter()
self.survey_type = self._getSurveyType()
# [TODO]
if self.filter_type != "FGS":
self._getChipRowCol()
# Set the relavent specs for FGS detectors
# [TODO]
try:
with pkg_resources.files('ObservationSim.Instrument.data.ccd').joinpath("chip_definition.json") as chip_definition:
with open(chip_definition, "r") as f:
chip_dict = json.load(f)[str(self.chipID)]
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data.ccd', "chip_definition.json") as chip_definition:
with open(chip_definition, "r") as f:
chip_dict = json.load(f)[str(self.chipID)]
for key in chip_dict:
setattr(self, key, chip_dict[key])
if self.filter_type == "FGS":
if ("field_dist" in config) and (config["ins_effects"]["field_dist"]) == False:
self.fdModel = None
else:
fgs_name = self.chip_name[0:4]
try:
with pkg_resources.files('ObservationSim.Instrument.data.field_distortion').joinpath("FieldDistModelGlobal_pr4_%s.pickle"%(fgs_name.lower())) as field_distortion:
with open(field_distortion, "rb") as f:
self.fdModel = pickle.load(f)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data.field_distortion', "FieldDistModelGlobal_pr4_%s.pickle"%(fgs_name.lower())) as field_distortion:
with open(field_distortion, "rb") as f:
self.fdModel = pickle.load(f)
else:
# Get the corresponding field distortion model
if ("field_dist" in config) and (config["ins_effects"]["field_dist"] == False):
# with pkg_resources.files('ObservationSim.Instrument.data.field_distortion').joinpath("FieldDistModelGlobal_mainFP_v1.0.pickle") as field_distortion:
with pkg_resources.files('ObservationSim.Instrument.data.field_distortion').joinpath("FieldDistModel_v2.0.pickle") as field_distortion:
with open(field_distortion, "rb") as f:
self.fdModel = pickle.load(f)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data.field_distortion', "FieldDistModelGlobal_mainFP_v1.0.pickle") as field_distortion:
with open(field_distortion, "rb") as f:
self.fdModel = pickle.load(f)
# Get boundary (in pix)
self.bound = self.getChipLim()
self.ccdEffCurve_dir = ccdEffCurve_dir
self.CRdata_dir = CRdata_dir
slsconfs = self.getChipSLSConf()
if np.size(slsconfs) == 1:
try:
with pkg_resources.files('ObservationSim.Instrument.data.sls_conf').joinpath(slsconfs) as conf_path:
self.sls_conf = str(conf_path)
except AttributeError:
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 = []
try:
with pkg_resources.files('ObservationSim.Instrument.data.sls_conf').joinpath(slsconfs[0]) as conf_path:
self.sls_conf.append(str(conf_path))
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data.sls_conf', slsconfs[0]) as conf_path:
self.sls_conf.append(str(conf_path))
try:
with pkg_resources.files('ObservationSim.Instrument.data.sls_conf').joinpath(slsconfs[1]) as conf_path:
self.sls_conf.append(str(conf_path))
except AttributeError:
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()
if "bright_fatter" in config["ins_effects"] and config["ins_effects"]["bright_fatter"] == True and self.survey_type == "photometric":
self.sensor = galsim.SiliconSensor(strength=self.df_strength, treering_func=treering_func)
self.flat_cube = None # for spectroscopic flat field cube simulation
def _set_attributes_from_config(self, config):
# Default setting
self.read_noise = 5.0 # e/pix
self.dark_noise = 0.02 # e/pix/s
self.rotate_angle = 0.
self.overscan = 1000
# Override default values
for key in ["gain", "bias_level, dark_exptime", "flat_exptime", "readout_time", "full_well", "read_noise", "dark_noise", "overscan"]:
if key in config["ins_effects"]:
setattr(self, key, config["ins_effects"][key])
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"
elif self.filter_type in ["nuv", "u", "g", 'r', 'i', 'z', 'y', 'FGS']:
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', 'FGS']: filename = 'Astro_MB.txt' # TODO, need to switch to the right efficiency curvey for FGS CMOS
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')
try:
with pkg_resources.files('ObservationSim.Instrument.data.ccd').joinpath(filename) as ccd_path:
table = Table.read(ccd_path, format='ascii')
except AttributeError:
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'], interpolant='linear')
bandpass = galsim.Bandpass(throughput, wave_type='nm')
return bandpass
def _getCRdata(self):
try:
with pkg_resources.files('ObservationSim.Instrument.data').joinpath("wfc-cr-attachpixel.dat") as cr_path:
self.attachedSizes = np.loadtxt(cr_path)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data', "wfc-cr-attachpixel.dat") as cr_path:
self.attachedSizes = np.loadtxt(cr_path)
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", "FGS"]
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>42 or chipID<1: raise ValueError("!!! Chip ID: [1,42]")
if chipID in [6, 15, 16, 25]: filter_type = "y"
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"
if chipID in range(31, 43): filter_type = 'FGS'
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 / spectroscopic observation.
Parameters:
chipID: int
the index of the chip
Returns:
A galsim BoundsD object
"""
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if ((chipID is not None) and (int(chipID) <= 30)) or (self.chipID <= 30):
# [TODO]
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)
xmin, xmax, ymin, ymax = 1e10, -1e10, 1e10, -1e10
xcen = self.x_cen / self.pix_size
ycen = self.y_cen / self.pix_size
sign_x = [-1., 1., -1., 1.]
sign_y = [-1., -1., 1., 1.]
for i in range(4):
x = xcen + sign_x[i] * self.npix_x / 2.
y = ycen + sign_y[i] * self.npix_y / 2.
x, y = rotate_conterclockwise(x0=xcen, y0=ycen, x=x, y=y, angle=self.rotate_angle)
xmin, xmax = min(xmin, x), max(xmax, x)
ymin, ymax = min(ymin, y), max(ymax, y)
return galsim.BoundsD(xmin, xmax, ymin, ymax)
# print("In getSkyCoverage: xmin = %.3f, xmax = %.3f, ymin = %.3f, ymax = %.3f"%(self.bound.xmin, self.bound.xmax, self.bound.ymin, self.bound.ymax))
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=None, dec_obj=None, x_image=None, y_image=None, wcs=None, margin=1):
if (ra_obj is not None) and (dec_obj is not None):
if wcs is None:
wcs = self.img.wcs
pos_obj = wcs.toImage(galsim.CelestialCoord(ra=ra_obj*galsim.degrees, dec=dec_obj*galsim.degrees))
x_image, y_image = pos_obj.x, pos_obj.y
elif (x_image is None) or (y_image is None):
raise ValueError("Either (ra_obj, dec_obj) or (x_image, y_image) should be given")
xmin, xmax = self.bound.xmin - margin, self.bound.xmax + margin
ymin, ymax = self.bound.ymin - margin, self.bound.ymax + margin
if (x_image - xmin) * (x_image - xmax) > 0.0 or (y_image - ymin) * (y_image - 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
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def generateHeader(self, ra_cen, dec_cen, img_rot, im_type, pointing_ID, exptime=150., timestamp = 1621915200):
datetime_obs = datetime.utcfromtimestamp(timestamp)
date_obs = datetime_obs.strftime("%y%m%d")
time_obs = datetime_obs.strftime("%H%M%S")
h_prim = generatePrimaryHeader(
xlen=self.npix_x,
ylen=self.npix_y,
pointNum = str(pointing_ID),
ra=ra_cen,
dec=dec_cen,
date=date_obs,
time_obs=time_obs,
im_type = im_type,
exptime=exptime,
chip_name=str(self.chipID).rjust(2, '0')
xlen=self.npix_x,
ylen=self.npix_y,
ra=ra_cen,
pa=img_rot.deg,
gain=self.gain,
readout=self.read_noise,
dark=self.dark_noise,
saturation=90000,
pixel_scale=self.pix_scale,
pixel_size=self.pix_size,
xcen=self.x_cen,
ycen=self.y_cen,
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extName='SCI',
timestamp = timestamp,
exptime = exptime,
readoutTime = 40.)
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def outputCal(self, img, ra_cen, dec_cen, img_rot, im_type, pointing_ID, output_dir, exptime=150., timestamp = 1621915200):
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,
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exptime=exptime,
timestamp = timestamp)
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hdu1.header.comments['CHECKSUM'] = 'HDU checksum'
hdu1.header.comments['DATASUM'] = 'data unit checksum'
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hdu2.header.comments['XTENSION'] = 'extension type'
hdu2.header.comments['CHECKSUM'] = 'HDU checksum'
hdu2.header.comments['DATASUM'] = 'data unit checksum'
hdu1 = fits.HDUList([hdu1, hdu2])
fname = os.path.join(output_dir, h_prim['FILENAME']+'.fits')
hdu1.writeto(fname, output_verify='ignore', overwrite=True)
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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"])
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self.logger = logger
# Get Poisson noise generator
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.)
# Add sky background
sky_map = sky_map * np.ones_like(img.array)
sky_map = galsim.Image(array=sky_map)
# Apply Poisson noise to the sky map
# (NOTE): only for photometric chips
# since it utilize the photon shooting
# to draw stamps
if self.survey_type == "photometric":
sky_map.addNoise(poisson_noise)
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
img += sky_map
del sky_map
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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
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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 to the resulting images
# (NOTE): this can only applied to the slitless image
# since it dose not use photon shooting to draw stamps
if self.survey_type == "spectroscopic":
img.addNoise(poisson_noise)
if config["ins_effects"]["cosmic_ray"] == True and pointing_type=='MS':
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if self.logger is not None:
self.logger.info((" Adding Cosmic-Ray"))
else:
print(" Adding Cosmic-Ray", flush=True)
exTime=exptime+0.5*self.readout_time,
cr_pixelRatio=0.003*(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))
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# datetime_obs = datetime.utcfromtimestamp(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,
output_dir=chip_output.subdir,
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exptime=exptime,
timestamp=timestamp_obs)
# Apply PRNU effect and output PRNU flat file:
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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*(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
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img = effects.BadColumns(img, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
# Apply Nonlinearity on the chip image
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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
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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
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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 Bias level
if config["ins_effects"]["add_bias"] == True:
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")
if config["ins_effects"]["bias_16channel"] == True:
img = effects.AddBiasNonUniform16(img,
bias_level=float(self.bias_level),
nsecy = 2, nsecx=8,
seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
elif config["ins_effects"]["bias_16channel"] == False:
img += self.bias_level
# 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
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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)
if config["ins_effects"]["gain_16channel"] == True:
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img, self.gain_channel = effects.ApplyGainNonUniform16(
img, gain=self.gain,
nsecy = 2, nsecx=8,
seed=SeedGainNonuni+self.chipID,
logger=self.logger)
elif config["ins_effects"]["gain_16channel"] == False:
img /= self.gain
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':
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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,
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seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
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# Readout noise for Biases is not generated with random seeds. So readout noise for bias images can't be reproduced.
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
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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
BiasCombImg = effects.BadColumns(BiasCombImg-float(self.bias_level)+5, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger) + float(self.bias_level)-5
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BiasCombImg, self.gain_channel = effects.ApplyGainNonUniform16(BiasCombImg, gain=self.gain,
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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))
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# datetime_obs = datetime.utcfromtimestamp(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,
output_dir=chip_output.subdir,
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exptime=0.0,
timestamp=timestamp_obs)
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':
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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)
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elif config["ins_effects"]["add_bias"] == False:
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,
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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;
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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)
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FlatCombImg = effects.BadColumns(FlatCombImg, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
# Add Bias level
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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,
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seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
# Add Read-out Noise
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seed = int(config["random_seeds"]["seed_readout"]) + pointing_ID*30 + self.chipID + 3
rng_readout = galsim.BaseDeviate(seed)
readout_noise = galsim.GaussianNoise(rng=rng_readout, sigma=self.read_noise)
FlatCombImg.addNoise(readout_noise)
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FlatCombImg, self.gain_channel = effects.ApplyGainNonUniform16(FlatCombImg, gain=self.gain,
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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))
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# datetime_obs = datetime.utcfromtimestamp(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,
output_dir=chip_output.subdir,
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exptime=self.flat_exptime,
timestamp=timestamp_obs)
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':
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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)
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elif config["ins_effects"]["add_bias"] == False:
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,
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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
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# datetime_obs = datetime.utcfromtimestamp(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,
output_dir=chip_output.subdir,
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exptime=self.dark_exptime,
timestamp=timestamp_obs)
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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)
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DarkCombImg = effects.BadColumns(DarkCombImg, seed=SeedBadColumns, chipid=self.chipID, logger=self.logger)
# Add Bias level
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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,
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seed=SeedBiasNonuni+self.chipID,
logger=self.logger)
# Add Read-out Noise
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seed = int(config["random_seeds"]["seed_readout"]) + pointing_ID*30 + self.chipID + 2
rng_readout = galsim.BaseDeviate(seed)
readout_noise = galsim.GaussianNoise(rng=rng_readout, sigma=self.read_noise)
DarkCombImg.addNoise(readout_noise)
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DarkCombImg, self.gain_channel = effects.ApplyGainNonUniform16(
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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))
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# datetime_obs = datetime.utcfromtimestamp(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,
output_dir=chip_output.subdir,
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exptime=self.dark_exptime,
timestamp = timestamp_obs)
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
def loadSLSFLATCUBE(self, flat_fn='flat_cube.fits'):
from astropy.io import fits
try:
with pkg_resources.files('ObservationSim.Instrument.data').joinpath(flat_fn) as data_path:
flat_fits = fits.open(data_path, ignore_missing_simple=True)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.data', flat_fn) as data_path:
flat_fits = fits.open(data_path, ignore_missing_simple=True)
fl = len(flat_fits)
fl_sh = flat_fits[0].data.shape
assert fl == 4, 'FLAT Field Cube is Not 4 layess!!!!!!!'
self.flat_cube = np.zeros([fl, fl_sh[0], fl_sh[1]])
for i in np.arange(0, fl, 1):
self.flat_cube[i] = flat_fits[i].data