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import os
import galsim
import ctypes
import numpy as np
from astropy.io import fits
from datetime import datetime
from ObservationSim.Instrument.Chip import Effects as effects
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
def log_info(msg, logger=None):
if logger:
logger.info(msg)
else:
print(msg, flush=True)
def getChipSLSGratingID(chipID):
gratingID = ['','']
if chipID == 1: gratingID = ['GI2', 'GI1']
if chipID == 2: gratingID = ['GV4', 'GV3']
if chipID == 3: gratingID = ['GU2', 'GU1']
if chipID == 4: gratingID = ['GU4', 'GU3']
if chipID == 5: gratingID = ['GV2', 'GV1']
if chipID == 10: gratingID = ['GI4', 'GI3']
if chipID == 21: gratingID = ['GI6', 'GI5']
if chipID == 26: gratingID = ['GV8', 'GV7']
if chipID == 27: gratingID = ['GU6', 'GU5']
if chipID == 28: gratingID = ['GU8', 'GU7']
if chipID == 29: gratingID = ['GV6', 'GV5']
if chipID == 30: gratingID = ['GI8', 'GI7']
return gratingID
def getChipSLSConf(chipID):
confFile = ''
if chipID == 1: confFile = ['CSST_GI2.conf', 'CSST_GI1.conf']
if chipID == 2: confFile = ['CSST_GV4.conf', 'CSST_GV3.conf']
if chipID == 3: confFile = ['CSST_GU2.conf', 'CSST_GU1.conf']
if chipID == 4: confFile = ['CSST_GU4.conf', 'CSST_GU3.conf']
if chipID == 5: confFile = ['CSST_GV2.conf', 'CSST_GV1.conf']
if chipID == 10: confFile = ['CSST_GI4.conf', 'CSST_GI3.conf']
if chipID == 21: confFile = ['CSST_GI6.conf', 'CSST_GI5.conf']
if chipID == 26: confFile = ['CSST_GV8.conf', 'CSST_GV7.conf']
if chipID == 27: confFile = ['CSST_GU6.conf', 'CSST_GU5.conf']
if chipID == 28: confFile = ['CSST_GU8.conf', 'CSST_GU7.conf']
if chipID == 29: confFile = ['CSST_GV6.conf', 'CSST_GV5.conf']
if chipID == 30: confFile = ['CSST_GI8.conf', 'CSST_GI7.conf']
return confFile
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def generateHeader(chip, ra_cen, dec_cen, img_rot, im_type, pointing_ID, exptime=150., project_cycle=6, run_counter=0, 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=chip.npix_x,
ylen=chip.npix_y,
pointNum = str(pointing_ID),
ra=ra_cen,
dec=dec_cen,
pixel_scale=chip.pix_scale,
date=date_obs,
time_obs=time_obs,
im_type = im_type,
exptime=exptime,
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project_cycle=project_cycle,
run_counter=run_counter,
chip_name=str(chip.chipID).rjust(2, '0')
)
h_ext = generateExtensionHeader(
chip=chip,
xlen=chip.npix_x,
ylen=chip.npix_y,
ra=ra_cen,
dec=dec_cen,
pa=img_rot.deg,
gain=chip.gain,
readout=chip.read_noise,
dark=chip.dark_noise,
saturation=90000,
pixel_scale=chip.pix_scale,
pixel_size=chip.pix_size,
xcen=chip.x_cen,
ycen=chip.y_cen,
timestamp = timestamp,
exptime = exptime,
readoutTime = chip.readout_time)
return h_prim, h_ext
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def outputCal(chip, img, ra_cen, dec_cen, img_rot, im_type, pointing_ID, output_dir, exptime=150., project_cycle=6, run_counter=0, timestamp = 1621915200):
h_prim, h_ext = generateHeader(
chip=chip,
ra_cen=ra_cen,
dec_cen=dec_cen,
img_rot=img_rot,
im_type=im_type,
pointing_ID=pointing_ID,
exptime=exptime,
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project_cycle=project_cycle,
run_counter=run_counter,
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timestamp=timestamp)
hdu1 = fits.PrimaryHDU(header=h_prim)
hdu1.add_checksum()
hdu1.header.comments['CHECKSUM'] = 'HDU checksum'
hdu1.header.comments['DATASUM'] = 'data unit checksum'
hdu2 = fits.ImageHDU(img.array, header=h_ext)
hdu2.add_checksum()
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)
def add_sky_background(img, filt, exptime, sky_map=None, tel=None):
# Add sky background
if sky_map is None:
sky_map = filt.getSkyNoise(exptime=exptime)
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 if it utilizes 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
sky_map = sky_map * tel.pupil_area * exptime
img += sky_map
return img, sky_map
def get_flat(img, seed):
flat_img = effects.MakeFlatSmooth(
GSBounds=img.bounds,
seed=seed)
flat_normal = flat_img / np.mean(flat_img.array)
return flat_img, flat_normal
def add_cosmic_rays(img, chip, exptime=150, seed=0):
cr_map, cr_event_num = effects.produceCR_Map(
xLen=chip.npix_x, yLen=chip.npix_y,
exTime=exptime+0.5*chip.readout_time,
cr_pixelRatio=0.003*(exptime+0.5*chip.readout_time)/600.,
gain=chip.gain,
attachedSizes=chip.attachedSizes,
seed=seed) # 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)
del cr_map
return img, crmap_gsimg, cr_event_num
def add_PRNU(img, chip, seed=0):
prnu_img = effects.PRNU_Img(
xsize=chip.npix_x,
ysize=chip.npix_y,
sigma=0.01,
seed=seed)
img *= prnu_img
return img, prnu_img
def get_poisson(seed=0, sky_level=0.):
rng_poisson = galsim.BaseDeviate(seed)
poisson_noise = galsim.PoissonNoise(rng_poisson, sky_level=sky_level)
return rng_poisson, poisson_noise
def get_base_img(img, chip, read_noise, readout_time, dark_noise, exptime=150., InputDark=None):
if InputDark == None:
# base_level = read_noise**2 + dark_noise*(exptime+0.5*readout_time)
## base_level = dark_noise*(exptime+0.5*readout_time)
base_level = dark_noise*(exptime)
base_img1 = base_level * np.ones_like(img.array)
else:
base_img1 = np.zeros_like(img.array)
ny = int(chip.npix_y/2)
nx = chip.npix_x
arr = np.arange(ny).reshape(ny, 1)
arr = np.broadcast_to(arr, (ny, nx))
base_img2 = np.zeros_like(img.array)
base_img2[:ny, :] = arr
base_img2[ny:, :] = arr[::-1,:]
base_img2[:,:] = base_img2[:,:]*(readout_time/ny)*dark_noise
return base_img1+base_img2
def add_poisson(img, chip, exptime=150., seed=0, sky_level=0., poisson_noise=None, dark_noise=None, InputDark=None):
if poisson_noise is None:
_, poisson_noise = get_poisson(seed=seed, sky_level=sky_level)
read_noise = chip.read_noise
if dark_noise is None:
dark_noise = chip.dark_noise
base_img = get_base_img(img=img, chip, read_noise=read_noise, readout_time=chip.readout_time, dark_noise=dark_noise, exptime=exptime, InputDark=None)
img += base_img
img.addNoise(poisson_noise)
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# img -= read_noise**2
if InputDark != None:
hdu = fits.open(InputDark) ##"Instrument/data/dark/dark_1000s_example_0.fits"
img += hdu[0].data/hdu[0].header['exptime']*exptime
hdu.close()
return img, base_img
def add_brighter_fatter(img):
#Inital dynamic lib
try:
with pkg_resources.files('ObservationSim.Instrument.Chip.libBF').joinpath("libmoduleBF.so") as lib_path:
lib_bf = ctypes.CDLL(lib_path)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.Chip.libBF', "libmoduleBF.so") as lib_path:
lib_bf = ctypes.CDLL(lib_path)
lib_bf.addEffects.argtypes = [ctypes.c_int, ctypes.c_int, ctypes.POINTER(ctypes.c_float), ctypes.POINTER(ctypes.c_float), ctypes.c_int]
# Set bit flag
bit_flag = 1
bit_flag = bit_flag | (1 << 2)
nx, ny = img.array.shape
nn = nx * ny
arr_ima= (ctypes.c_float*nn)()
arr_imc= (ctypes.c_float*nn)()
arr_ima[:]= img.array.reshape(nn)
arr_imc[:]= np.zeros(nn)
lib_bf.addEffects(nx, ny, arr_ima, arr_imc, bit_flag)
img.array[:, :] = np.reshape(arr_imc, [nx, ny])
del arr_ima, arr_imc
def add_inputdark(img, chip, exptime):
fname = "/share/home/weichengliang/CSST_git/test_new_sim/csst-simulation/ObservationSim/Instrument/data/dark/dark_1000s_example_0.fits"
hdu = fits.open(fname)
#ny, nx = img.array.shape
#inputdark = np.zeros([ny, nx])
img.array[:, :] += hdu[0].data/hdu[0].header['exptime']*exptime
hdu.close()
del inputdark
return img
def AddPreScan(GSImage, pre1=27, pre2=4, over1=71, over2=80, nsecy = 2, nsecx=8):
img= GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
imgt=np.zeros([int(nsecy*nsecx), int(ny/nsecy+pre2+over2), int(nx/nsecx+pre1+over1)])
for iy in range(nsecy):
for ix in range(nsecx):
if iy % 2 == 0:
tx = ix
else:
tx = (nsecx-1)-ix
ty = iy
chunkidx = int(tx+ty*nsecx) #chunk1-[1,2,3,4], chunk2-[5,6,7,8], chunk3-[9,10,11,12], chunk4-[13,14,15,16]
imgtemp = np.zeros([int(ny/nsecy+pre2+over2), int(nx/nsecx+pre1+over1)])
if int(chunkidx/4) == 0:
imgtemp[pre2:pre2+dy, pre1:pre1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp
if int(chunkidx/4) == 1:
imgtemp[pre2:pre2+dy, over1:over1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[:, ::-1]
if int(chunkidx/4) == 2:
imgtemp[over2:over2+dy, over1:over1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[::-1, ::-1]
if int(chunkidx/4) == 3:
imgtemp[over2:over2+dy, pre1:pre1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[::-1, :]
imgtx1 = np.hstack(imgt[:nsecx:, :, :]) #hstack chunk(1,2)-[1,2,3,4,5,6,7,8]
imgtx2 = np.hstack(imgt[:(nsecx-1):-1, :, :]) #hstack chunk(4,3)-[16,15,14,13,12,11,,10,9]
newimg = galsim.Image(int(nx+(pre1+over1)*nsecx), int(ny+(pre2+over2)*nsecy), init_value=0)
newimg.array[:, :] = np.concatenate([imgtx1, imgtx2]) #vstack chunk(1,2) & chunk(4,3)
newimg.wcs = GSImage.wcs
return newimg
def AddPreScanFO(GSImage, pre1=27, pre2=4, over1=71, over2=80, nsecy = 1, nsecx=16):
img= GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
newimg = galsim.Image(int(nx+(pre1+over1)*nsecx), int(ny+(pre2+over2)*nsecy), init_value=0)
for ix in range(nsecx):
newimg.array[pre2:pre2+dy, pre1+ix*(dx+pre1+over1):pre1+dx+ix*(dx+pre1+over1)] = img[0:dy, 0+ix*dx:dx+ix*dx]
newimg.wcs = GSImage.wcs
return newimg
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def formatOutput(GSImage, nsecy = 2, nsecx=8):
img = GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
imgt = np.zeros([int(nsecx*nsecy), dy, dx])
for iy in range(nsecy):
for ix in range(nsecx):
if iy % 2 == 0:
tx = ix
else:
tx = (nsecx-1)-ix
ty = iy
chunkidx = int(tx+ty*nsecx)
if int(chunkidx/4) == 0:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 1:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 2:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 3:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgttx0 = np.hstack(imgt[ 0:4:, :, :])
imgttx1 = np.hstack(imgt[ 4:8:, :, ::-1])
imgttx2 = np.hstack(imgt[8:12:, ::-1, ::-1])
imgttx3 = np.hstack(imgt[12:16:,::-1, :])
newimg = galsim.Image(int(dx*nsecx*nsecy), dy, init_value=0)
newimg.array[:, :] = np.hstack([imgttx0, imgttx1, imgttx2, imgttx3])
return newimg
def formatRevert(GSImage, nsecy = 1, nsecx=16):
img = GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
newimg = galsim.Image(int(dx*8), int(dy*2), init_value=0)
for ix in range(0,4):
tx = ix
newimg.array[0:dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx]
for ix in range(4,8):
tx = ix
newimg.array[0:dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][:, ::-1]
for ix in range(8,12):
tx = 7-(ix-8)
newimg.array[0+dy:dy+dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][::-1, ::-1]
for ix in range(12,16):
tx = 7-(ix-8)
newimg.array[0+dy:dy+dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][::-1, :]
return newimg