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import galsim
import os
import numpy as np
import Instrument.Chip.Effects as effects
from Instrument.FocalPlane import FocalPlane
from astropy.table import Table
from numpy.random import Generator, PCG64
class Chip(FocalPlane):
def __init__(self, chipID, ccdEffCurve_dir, CRdata_dir, normalize_dir=None, sls_dir=None, config=None, treering_func=None):
# Get focal plane (instance of paraent class) info
# TODO: use chipID to config individual chip?
super().__init__()
# if config is not None:
# self.npix_x = config["npix_x"]
# self.npix_y = config["npix_y"]
# self.read_noise = config["read_noise"]
# self.dark_noise = config["dark_noise"]
# self.pix_scale = config["pix_scale"]
# self.gain = config["gain"]
# self.bias_level = config["bias_level"]
# self.overscan = config["overscan"]
# else:
# Default setting
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 = 1.0
# self.bias_level = 1000 # e-/pix
self.gain = float(config["gain"])
self.bias_level = float(config["bias_level"])
self.overscan = 1000
self.exptime = 150 # second
# 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.normalize_dir = normalize_dir
self.sls_dir=sls_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)]
else:
self.sls_conf = [os.path.join(self.sls_dir, slsconfs[0]), os.path.join(self.sls_dir, slsconfs[1])]
if self.normalize_dir is not None:
self._getNormF()
self.effCurve = self._getChipEffCurve(self.filter_type)
self._getCRdata()
# Define the sensor
if config["bright_fatter"].lower() == "y":
self.sensor = galsim.SiliconSensor(strength=config["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 _getNormF(self):
self.normF_star = Table.read(os.path.join(self.normalize_dir, 'SLOAN_SDSS.g.fits'))
self.normF_galaxy = Table.read(os.path.join(self.normalize_dir, 'lsst_throuput_g.fits'))
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')
throughput = galsim.LookupTable(x=table['col1'], f=table['col2']*mirror_eff, 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)
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 addNoise_phot(self, img, exptime=150.0, sky_noise=0., seed=31415):
rng = galsim.BaseDeviate(seed)
dark_noise = galsim.DeviateNoise(galsim.PoissonDeviate(rng, self.dark_noise*exptime))
img.addNoise(dark_noise)
ccd_noise = galsim.CCDNoise(rng, sky_level=sky_noise, gain=self.gain, read_noise=self.read_noise)
img.addNoise(ccd_noise)
return img
def addNoise_spec(self, config, tel, img, sky_map, exptime=150.0, seed=31415):
if img.array.shape != sky_map.shape:
raise ValueError("The shape img and sky_map must be equal.")
# n_img_arrar = (img.array + sky_map) * tel.pupil_area * exptime
# Should be the following?
rng = galsim.BaseDeviate(seed)
noise_img = galsim.Image(img, copy=True)
dark_noise = galsim.DeviateNoise(galsim.PoissonDeviate(rng, self.dark_noise*exptime))
img.addNoise(dark_noise)
if config["abs_back"].lower() == "y":
img += (sky_map * tel.pupil_area * exptime)
ccd_noise = galsim.CCDNoise(rng, gain=self.gain, read_noise=self.read_noise)
img.addNoise(ccd_noise)
return img
# pNoise = self.dark_noise * exptime
# noise_img = galsim.Image(n_img_arrar, copy=True)
# dNose = galsim.PoissonNoise(rng=rng, sky_level=pNoise)
# noise_img.addNoise(dNose)
# rdNoise = galsim.GaussianNoise(rng=rng, sigma=self.read_noise)
# noise_img.addNoise(rdNoise)
# return noise_img
def addNoise(self, config, tel, filt, img, sky_map=None, exptime=150.0):
if self.survey_type == "photometric":
sky_level = filt.getSkyNoise(exptime=exptime, gain=self.gain)
img = self.addNoise_phot(
img=img,
exptime=exptime,
sky_noise=filt.getSkyNoise(exptime=exptime, gain=self.gain),
seed=int(config["seed_skynoise"]))
if config["abs_back"].lower() == "y":
img += sky_level
elif self.survey_type == "spectroscopic":
if sky_map is None:
raise ValueError("Must provide sky_map for spectroscopic chip")
img = self.addNoise_spec(
config=config,
tel=tel,
img=img,
sky_map=sky_map,
exptime=exptime,
seed=int(config["seed_skynoise"]))
return img
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
def addEffects(self, config, img, chip_output, filt, exptime=150., pointing_ID=0):
SeedGainNonuni=int(config["seed_gainNonUniform"])
SeedBiasNonuni=int(config["seed_biasNonUniform"])
SeedRnNonuni = int(config["seed_rnNonUniform"])
SeedBadColumns = int(config["seed_badcolumns"])
SeedDefective = int(config["seed_defective"])
SeedCosmicRay = int(config["seed_CR"])
fullwell = int(config["full_well"])
if config["add_hotpixels"].lower() == "y":
BoolHotPix = True
else:
BoolHotPix = False
if config["add_deadpixels"].lower() == "y":
BoolDeadPix = True
else:
BoolDeadPix = False
# Apply flat-field large scale structure for one chip
if config["flat_fielding"].lower() == "y":
print(" Creating and applying Flat-Fielding", flush=True)
print(img.bounds, flush=True)
flat_img = effects.MakeFlatSmooth(
img.bounds,
int(config["seed_flat"]))
flat_normal = flat_img / np.mean(flat_img.array)
img *= flat_normal
del flat_normal
if config["flat_output"].lower() == "n":
del flat_img
# Apply Shutter-effect for one chip
if config["shutter_effect"].lower() == "y":
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
img *= shuttimg
if config["shutter_output"].lower() == "y": # 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
# Apply PRNU effect and output PRNU flat file:
if config["prnu_effect"].lower() == "y":
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["seed_prnu"]+self.chipID))
img *= prnu_img
if config["prnu_output"].lower() == "y":
prnu_img.write("%s/FlatImg_PRNU_%s.fits" % (chip_output.subdir,self.chipID))
if config["flat_output"].lower() == "n":
del prnu_img
# Add dark current
img += self.dark_noise*exptime
# Add cosmic-rays
if config["cosmic_ray"].lower() == "y":
print(" Adding Cosmic-Ray", flush=True)
cr_map = effects.produceCR_Map(
xLen=self.npix_x, yLen=self.npix_y,
exTime=exptime,
cr_pixelRatio=0.003,
gain=self.gain,
attachedSizes=self.attachedSizes,
seed=SeedCosmicRay+pointing_ID*30+self.chipID)
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))
del crmap_gsimg
# Add Bias level
if config["add_bias"].lower() == "y":
print(" Adding Bias level and 16-channel non-uniformity")
# img += float(config["bias_level"])
img = effects.AddBiasNonUniform16(img,
bias_level=float(config["bias_level"]),
nsecy = 2, nsecx=8,
seed=SeedBiasNonuni+self.chipID)
# Bias output
if config["bias_output"].lower() == "y":
print(" Output N frame Bias files", flush=True)
NBias = int(config["NBias"])
for i in range(NBias):
BiasCombImg, BiasTag = effects.MakeBiasNcomb(
self.npix_x, self.npix_y,
bias_level=float(config["bias_level"]),
ncombine=1, read_noise=self.read_noise, gain=1,
seed=SeedBiasNonuni+self.chipID)
# Non-Linearity for Bias
if config["non_linear"].lower() == "y":
print(" Applying Non-Linearity on the Bias image", flush=True)
BiasCombImg = effects.NonLinearity(GSImage=BiasCombImg, beta1=1.e-7, beta2=1.e-10)
BiasCombImg = effects.ApplyGainNonUniform16(BiasCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
seed=SeedGainNonuni+self.chipID)
# BiasCombImg = effects.AddOverscan(
# BiasCombImg,
# overscan=float(config["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))
del BiasCombImg
# Export combined (ncombine, Vignetting + PRNU) & single vignetting flat-field file
if config["flat_output"].lower() == "y":
print(" Output N frame Flat-Field files", flush=True)
NFlat = int(config["NFlat"])
if config["add_bias"].lower() == "y":
biaslevel = self.bias_level
overscan = biaslevel-2
elif config["add_bias"].lower() == "n":
biaslevel = 0
overscan = 0
darklevel = self.dark_noise*self.exptime
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=biaslevel,
seed_bias=SeedDefective+self.chipID
)
if config["cosmic_ray"].lower() == "y":
FlatCombImg += cr_map
if config["non_linear"].lower() == "y":
print(" Applying Non-Linearity on the Flat image", flush=True)
FlatCombImg = effects.NonLinearity(GSImage=FlatCombImg, beta1=1.e-7, beta2=1.e-10)
if config["cte_trail"].lower() == "y":
FlatCombImg = effects.CTE_Effect(GSImage=FlatCombImg, threshold=3)
# Apply Bad lines
if config["add_badcolumns"].lower() == "y":
FlatCombImg = effects.BadColumns(FlatCombImg, seed=SeedBadColumns, chipid=self.chipID)
# 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=self.bias_level)
FlatCombImg = effects.ApplyGainNonUniform16(FlatCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
seed=SeedGainNonuni+self.chipID)
# 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))
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["dark_output"].lower() == "y":
print(" Output N frame Dark Current files", flush=True)
NDark = int(config["NDark"])
if config["add_bias"].lower() == "y":
biaslevel = self.bias_level
overscan = biaslevel-2
elif config["add_bias"].lower() == "n":
biaslevel = 0
overscan = 0
for i in range(NDark):
DarkCombImg, DarkTag = effects.MakeDarkNcomb(
self.npix_x, self.npix_y,
overscan=overscan, bias_level=biaslevel, darkpsec=0.02, exptime=150,
ncombine=1, read_noise=self.read_noise,
gain=1, seed_bias=SeedBiasNonuni+self.chipID)
if config["cosmic_ray"].lower() == "y":
DarkCombImg += cr_map
# Non-Linearity for Dark
if config["non_linear"].lower() == "y":
print(" Applying Non-Linearity on the Dark image", flush=True)
DarkCombImg = effects.NonLinearity(GSImage=DarkCombImg, beta1=1.e-7, beta2=1.e-10)
if config["cte_trail"].lower() == "y":
DarkCombImg = effects.CTE_Effect(GSImage=DarkCombImg, threshold=3)
# Apply Bad lines
if config["add_badcolumns"].lower() == "y":
DarkCombImg = effects.BadColumns(DarkCombImg, seed=SeedBadColumns, chipid=self.chipID)
# 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=self.bias_level)
DarkCombImg = effects.ApplyGainNonUniform16(
DarkCombImg, gain=self.gain,
nsecy = 2, nsecx=8,
seed=SeedGainNonuni+self.chipID)
# 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))
del DarkCombImg
# garbage collection of cosmic-ray array
if config["cosmic_ray"].lower() == "y":
del cr_map
# Apply Nonlinearity on the chip image
if config["non_linear"].lower() == "y":
print(" Applying Non-Linearity on the chip image", flush=True)
img = effects.NonLinearity(GSImage=img, beta1=1.e-7, beta2=1.e-10)
# Apply CCD Saturation & Blooming
if config["saturbloom"].lower() == "y":
print(" Applying CCD Saturation & Blooming")
img = effects.SaturBloom(GSImage=img, nsect_x=1, nsect_y=1, fullwell=fullwell)
# Apply CTE Effect
if config["cte_trail"].lower() == "y":
print(" Apply CTE Effect")
img = effects.CTE_Effect(GSImage=img, threshold=27)
# Apply Bad lines
if config["add_badcolumns"].lower() == "y":
img = effects.BadColumns(img, seed=SeedBadColumns, chipid=self.chipID)
# 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=self.bias_level)
# Apply Gain & Quantization
print(" Applying Gain (and 16 channel non-uniformity) & Quantization", flush=True)
img = effects.ApplyGainNonUniform16(
img, gain=self.gain,
nsecy = 2, nsecx=8,
seed=SeedGainNonuni+self.chipID)
img.array[img.array > 65535] = 65535
img.replaceNegative(replace_value=0)
img.quantize()
# img = galsim.ImageUS(img)
# # 16 output channel, with each a single image file
# if config["readout16"].lower() == "y":
# 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
return img