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Commit d4b41c36 authored by Wei Chengliang's avatar Wei Chengliang
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update fits module

parent f5372672
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Catalog/C6_fits_Catalog.py
View file @ d4b41c36
...@@ -60,6 +60,9 @@ class Catalog(CatalogBase): ...@@ -60,6 +60,9 @@ class Catalog(CatalogBase):
with pkg_resources.path('Catalog.data', 'SLOAN_SDSS.g.fits') as filter_path: with pkg_resources.path('Catalog.data', 'SLOAN_SDSS.g.fits') as filter_path:
self.normF_star = Table.read(str(filter_path)) self.normF_star = Table.read(str(filter_path))
with pkg_resources.path('Catalog.data', 'lsst_throuput_g.fits') as filter_path:
self.normF_galaxy = Table.read(str(filter_path))
self.config = config self.config = config
self.chip = chip self.chip = chip
...@@ -138,8 +141,8 @@ class Catalog(CatalogBase): ...@@ -138,8 +141,8 @@ class Catalog(CatalogBase):
return None return None
###mock_stamp_START ###mock_stamp_START
elif obj.type == "stamp": elif obj.type == "stamp":
#return self.normF_galaxy ###normalize_filter for stamp return self.normF_galaxy ###normalize_filter for stamp
return None #return None
###mock_stamp_END ###mock_stamp_END
else: else:
return None return None
...@@ -197,8 +200,8 @@ class Catalog(CatalogBase): ...@@ -197,8 +200,8 @@ class Catalog(CatalogBase):
for igals in range(ngals): for igals in range(ngals):
# # (TEST) # # (TEST)
# if igals > 100: if igals > 2000:
# break break
param = self.initialize_param() param = self.initialize_param()
param['ra'] = ra_arr[igals] param['ra'] = ra_arr[igals]
...@@ -321,8 +324,8 @@ class Catalog(CatalogBase): ...@@ -321,8 +324,8 @@ class Catalog(CatalogBase):
) )
for istars in range(nstars): for istars in range(nstars):
# # (TEST) # # (TEST)
# if istars > 100: if istars > 100:
# break break
param = self.initialize_param() param = self.initialize_param()
param['ra'] = ra_arr[istars] param['ra'] = ra_arr[istars]
...@@ -389,6 +392,9 @@ class Catalog(CatalogBase): ...@@ -389,6 +392,9 @@ class Catalog(CatalogBase):
input_time_str=time_str input_time_str=time_str
) )
for iAGNs in range(nAGNs): for iAGNs in range(nAGNs):
if iAGNs > 100:
break
param = self.initialize_param() param = self.initialize_param()
param['ra'] = ra_arr[iAGNs] param['ra'] = ra_arr[iAGNs]
param['dec'] = dec_arr[iAGNs] param['dec'] = dec_arr[iAGNs]
...@@ -425,13 +431,15 @@ class Catalog(CatalogBase): ...@@ -425,13 +431,15 @@ class Catalog(CatalogBase):
self.ud = galsim.UniformDeviate(pix_id) self.ud = galsim.UniformDeviate(pix_id)
for istamp in range(nstamps): for istamp in range(nstamps):
print('DEBUG:::istamp=', istamp)
fitsfile = os.path.join(self.cat_dir, "stampCats/"+stamps['filename'][istamp].decode('utf-8')) fitsfile = os.path.join(self.cat_dir, "stampCats/"+stamps['filename'][istamp].decode('utf-8'))
hdu=fitsio.open(fitsfile) hdu=fitsio.open(fitsfile)
param = self.initialize_param() param = self.initialize_param()
param['id'] = hdu[0].header['index'] #istamp param['id'] = hdu[0].header['index'] #istamp
param['star'] = 3 # Stamp type in .cat file param['star'] = 3 # Stamp type in .cat file
param['lensGalaxyID'] = hdu[0].header['lensGID'] ###param['lensGalaxyID'] = hdu[0].header['lensGID']
param['ra'] = hdu[0].header['ra'] param['ra'] = hdu[0].header['ra']
param['dec']= hdu[0].header['dec'] param['dec']= hdu[0].header['dec']
param['pixScale']= hdu[0].header['pixScale'] param['pixScale']= hdu[0].header['pixScale']
...@@ -440,9 +448,9 @@ class Catalog(CatalogBase): ...@@ -440,9 +448,9 @@ class Catalog(CatalogBase):
#param['PA']= hdu[0].header['PA'] #param['PA']= hdu[0].header['PA']
#param['bfrac']= hdu[0].header['bfrac'] #param['bfrac']= hdu[0].header['bfrac']
#param['z']= hdu[0].header['z'] #param['z']= hdu[0].header['z']
param['mag_use_normal'] = 22 #hdu[0].header['m_normal'] #gals['mag_true_g_lsst'] param['mag_use_normal'] = 20 #hdu[0].header['m_normal'] #gals['mag_true_g_lsst']
assert(stamps['lensGID'][istamp] == param['lensGalaxyID']) ###assert(stamps['lensGID'][istamp] == param['lensGalaxyID'])
# Apply astrometric modeling # Apply astrometric modeling
# in C3 case only aberration # in C3 case only aberration
......
ObservationSim/MockObject/Stamp.py
View file @ d4b41c36
import os, sys import os, sys
import random
import numpy as np import numpy as np
import galsim
import astropy.constants as cons import astropy.constants as cons
from astropy.table import Table from astropy.table import Table
from scipy import interpolate from scipy import interpolate
import astropy.io.fits as fitsio
import galsim
import gc
from ObservationSim.MockObject.MockObject import MockObject from ObservationSim.MockObject.MockObject import MockObject
from ObservationSim.MockObject.SpecDisperser import SpecDisperser
from ObservationSim.MockObject._util import magToFlux,VC_A
from ObservationSim.MockObject._util import eObs, integrate_sed_bandpass, getNormFactorForSpecWithABMAG, getObservedSED, getABMAG,convolveGaussXorders from ObservationSim.MockObject._util import eObs, integrate_sed_bandpass, getNormFactorForSpecWithABMAG, getObservedSED, getABMAG,convolveGaussXorders
class Stamp(MockObject): class Stamp(MockObject):
def __init__(self, param): def __init__(self, param, logger=None):
super().__init__(param) super().__init__(param, logger=logger)
def unload_SED(self): def unload_SED(self):
"""(Test) free up SED memory """(Test) free up SED memory
...@@ -35,9 +30,9 @@ class Stamp(MockObject): ...@@ -35,9 +30,9 @@ class Stamp(MockObject):
self.logger.error(e) self.logger.error(e)
return False return False
nphotons_sum = 0 #nphotons_sum = 0
photons_list = [] #photons_list = []
xmax, ymax = 0, 0 #xmax, ymax = 0, 0
if self.getMagFilter(filt) <= 15: if self.getMagFilter(filt) <= 15:
folding_threshold = 5.e-4 folding_threshold = 5.e-4
...@@ -46,7 +41,7 @@ class Stamp(MockObject): ...@@ -46,7 +41,7 @@ class Stamp(MockObject):
gsp = galsim.GSParams(folding_threshold=folding_threshold) gsp = galsim.GSParams(folding_threshold=folding_threshold)
self.real_pos = self.getRealPos(chip.img, global_x=self.posImg.x, global_y=self.posImg.y, self.real_pos = self.getRealPos(chip.img, global_x=self.posImg.x, global_y=self.posImg.y,
img_real_wcs=self.real_wcs) img_real_wcs=self.chip_wcs)
x, y = self.real_pos.x + 0.5, self.real_pos.y + 0.5 x, y = self.real_pos.x + 0.5, self.real_pos.y + 0.5
x_nominal = int(np.floor(x + 0.5)) x_nominal = int(np.floor(x + 0.5))
...@@ -55,72 +50,237 @@ class Stamp(MockObject): ...@@ -55,72 +50,237 @@ class Stamp(MockObject):
dy = y - y_nominal dy = y - y_nominal
offset = galsim.PositionD(dx, dy) offset = galsim.PositionD(dx, dy)
real_wcs_local = self.real_wcs.local(self.real_pos) chip_wcs_local = self.chip_wcs.local(self.real_pos)
is_updated = 0
if fd_shear:
g1 += fd_shear.g1
g2 += fd_shear.g2
gal_shear = galsim.Shear(g1=g1, g2=g2)
for i in range(len(bandpass_list)): for i in range(len(bandpass_list)):
bandpass = bandpass_list[i] bandpass = bandpass_list[i]
try: try:
sub = integrate_sed_bandpass(sed=self.sed, bandpass=bandpass) sub = integrate_sed_bandpass(sed=self.sed, bandpass=bandpass)
except Exception as e: except Exception as e:
print(e) print(e)
self.logger.error(e) if self.logger:
# return False self.logger.error(e)
continue continue
ratio = sub/full ratio = sub/full
if not (ratio == -1 or (ratio != ratio)): if not (ratio == -1 or (ratio != ratio)):
nphotons = ratio * nphotons_tot nphotons = ratio * nphotons_tot
else: else:
# return False
continue continue
nphotons_sum += nphotons #nphotons_sum += nphotons
psf, pos_shear = psf_model.get_PSF(chip=chip, pos_img=pos_img, bandpass=bandpass, folding_threshold=folding_threshold) psf, pos_shear = psf_model.get_PSF(chip=chip, pos_img=pos_img, bandpass=bandpass, folding_threshold=folding_threshold)
_gal = self.param['image'] _gal = self.param['image']
galIm = galsim.ImageF(_gal, scale=self.param['pixScale']) galImg= galsim.ImageF(_gal, scale=self.param['pixScale'])
gal = galsim.InterpolatedImage(galIm) gal_temp= galsim.InterpolatedImage(galImg)
gal = gal.withFlux(nphotons) gal_temp= gal_temp.shear(gal_shear)
#gal_shear = galsim.Shear(g1=g1, g2=g2) gal_temp= gal_temp.withFlux(nphotons)
#gal = gal.shear(gal_shear)
gal = galsim.Convolve(psf, gal) gal_temp= galsim.Convolve(psf, gal_temp)
if fd_shear is not None:
gal = gal.shear(fd_shear)
stamp = gal.drawImage(wcs=real_wcs_local, method='phot', offset=self.offset, save_photons=True) if i == 0:
gal = gal_temp
xmax = max(xmax, stamp.xmax - stamp.xmin) else:
ymax = max(ymax, stamp.ymax - stamp.ymin) gal = gal + gal_temp
photons = stamp.photons
photons.x += x_nominal
photons.y += y_nominal
photons_list.append(photons)
del gal
# print('xmax = %d, ymax = %d '%(xmax, ymax)) stamp = gal.drawImage(wcs=chip_wcs_local, offset=offset)
if np.sum(np.isnan(stamp.array)) > 0:
# ERROR happens
return 2, pos_shear
stamp = galsim.ImageF(int(xmax*1.1), int(ymax*1.1))
stamp.wcs = real_wcs_local
stamp.setCenter(x_nominal, y_nominal) stamp.setCenter(x_nominal, y_nominal)
bounds = stamp.bounds & galsim.BoundsI(0, chip.npix_x - 1, 0, chip.npix_y - 1) bounds = stamp.bounds & galsim.BoundsI(0, chip.npix_x - 1, 0, chip.npix_y - 1)
if bounds.area() > 0: if bounds.area() > 0:
chip.img.setOrigin(0, 0) chip.img.setOrigin(0, 0)
stamp[bounds] = chip.img[bounds] chip.img[bounds] += stamp[bounds]
for i in range(len(photons_list)): is_updated = 1
if i == 0: chip.img.setOrigin(chip.bound.xmin, chip.bound.ymin)
chip.sensor.accumulate(photons_list[i], stamp) del stamp
else:
chip.sensor.accumulate(photons_list[i], stamp, resume=True)
chip.img[bounds] = stamp[bounds] if is_updated == 0:
print("fits obj %s missed"%(self.id))
if self.logger:
self.logger.info("fits obj %s missed"%(self.id))
return 0, pos_shear
chip.img.setOrigin(chip.bound.xmin, chip.bound.ymin) return 1, pos_shear
def drawObj_slitless(self, tel, pos_img, psf_model, bandpass_list, filt, chip, nphotons_tot=None, g1=0, g2=0,
exptime=150., normFilter=None, grating_split_pos=3685, fd_shear=None):
if normFilter is not None:
norm_thr_rang_ids = normFilter['SENSITIVITY'] > 0.001
sedNormFactor = getNormFactorForSpecWithABMAG(ABMag=self.param['mag_use_normal'], spectrum=self.sed,
norm_thr=normFilter,
sWave=np.floor(normFilter[norm_thr_rang_ids][0][0]),
eWave=np.ceil(normFilter[norm_thr_rang_ids][-1][0]))
if sedNormFactor == 0:
return 2, None
else:
sedNormFactor = 1.
normalSED = Table(np.array([self.sed['WAVELENGTH'], self.sed['FLUX'] * sedNormFactor]).T,
names=('WAVELENGTH', 'FLUX'))
self.real_pos = self.getRealPos(chip.img, global_x=self.posImg.x, global_y=self.posImg.y,
img_real_wcs=self.chip_wcs)
x, y = self.real_pos.x + 0.5, self.real_pos.y + 0.5
x_nominal = int(np.floor(x + 0.5))
y_nominal = int(np.floor(y + 0.5))
dx = x - x_nominal
dy = y - y_nominal
offset = galsim.PositionD(dx, dy)
chip_wcs_local = self.chip_wcs.local(self.real_pos)
if self.getMagFilter(filt) <= 15:
folding_threshold = 5.e-4
else:
folding_threshold = 5.e-3
gsp = galsim.GSParams(folding_threshold=folding_threshold)
# nphotons_sum = 0
flat_cube = chip.flat_cube
xOrderSigPlus = {'A':1.3909419820029296,'B':1.4760376591236062,'C':4.035447379743442,'D':5.5684364343742825,'E':16.260021029735388}
grating_split_pos_chip = 0 + grating_split_pos
branges = np.zeros([len(bandpass_list), 2])
# print(hasattr(psf_model, 'bandranges'))
if hasattr(psf_model, 'bandranges'):
if psf_model.bandranges is None:
return 2, None
if len(psf_model.bandranges) != len(bandpass_list):
return 2, None
branges = psf_model.bandranges
else:
for i in range(len(bandpass_list)):
branges[i, 0] = bandpass_list[i].blue_limit * 10
branges[i, 1] = bandpass_list[i].red_limit * 10
for i in range(len(bandpass_list)):
# bandpass = bandpass_list[i]
brange = branges[i]
# psf, pos_shear = psf_model.get_PSF(chip=chip, pos_img=pos_img, bandpass=bandpass, folding_threshold=folding_threshold)
_gal = self.param['image']
galImg= galsim.ImageF(_gal, scale=self.param['pixScale'])
gal = galsim.InterpolatedImage(galImg)
# (TEST) Random knots
# knots = galsim.RandomKnots(npoints=100, profile=disk)
# kfrac = np.random.random()*(1.0 - self.bfrac)
# gal = self.bfrac * bulge + (1.0 - self.bfrac - kfrac) * disk + kfrac * knots
gal = gal.withFlux(tel.pupil_area * exptime)
if fd_shear:
g1 += fd_shear.g1
g2 += fd_shear.g2
gal_shear = galsim.Shear(g1=g1, g2=g2)
gal = gal.shear(gal_shear)
# gal = galsim.Convolve(psf, gal)
# if not big_galaxy: # Not apply PSF for very big galaxy
# gal = galsim.Convolve(psf, gal)
# # if fd_shear is not None:
# # gal = gal.shear(fd_shear)
starImg = gal.drawImage(wcs=chip_wcs_local, offset=offset,method = 'real_space')
origin_star = [y_nominal - (starImg.center.y - starImg.ymin),
x_nominal - (starImg.center.x - starImg.xmin)]
starImg.setOrigin(0, 0)
gal_origin = [origin_star[0], origin_star[1]]
gal_end = [origin_star[0] + starImg.array.shape[0] - 1, origin_star[1] + starImg.array.shape[1] - 1]
if gal_origin[1] < grating_split_pos_chip < gal_end[1]:
subSlitPos = int(grating_split_pos_chip - gal_origin[1] + 1)
## part img disperse
subImg_p1 = starImg.array[:, 0:subSlitPos]
star_p1 = galsim.Image(subImg_p1)
star_p1.setOrigin(0, 0)
origin_p1 = origin_star
xcenter_p1 = min(x_nominal,grating_split_pos_chip-1) - 0
ycenter_p1 = y_nominal-0
sdp_p1 = SpecDisperser(orig_img=star_p1, xcenter=xcenter_p1,
ycenter=ycenter_p1, origin=origin_p1,
tar_spec=normalSED,
band_start=brange[0], band_end=brange[1],
conf=chip.sls_conf[0],
isAlongY=0,
flat_cube=flat_cube)
# self.addSLStoChipImage(sdp=sdp_p1, chip=chip, xOrderSigPlus = xOrderSigPlus, local_wcs=chip_wcs_local)
pos_shear = self.addSLStoChipImageWithPSF(sdp=sdp_p1, chip=chip, pos_img_local=[xcenter_p1, ycenter_p1],
psf_model=psf_model, bandNo=i + 1,
grating_split_pos=grating_split_pos,
local_wcs=chip_wcs_local, pos_img = pos_img)
subImg_p2 = starImg.array[:, subSlitPos+1:starImg.array.shape[1]]
star_p2 = galsim.Image(subImg_p2)
star_p2.setOrigin(0, 0)
origin_p2 = [origin_star[0], grating_split_pos_chip]
xcenter_p2 = max(x_nominal, grating_split_pos_chip - 1) - 0
ycenter_p2 = y_nominal - 0
sdp_p2 = SpecDisperser(orig_img=star_p2, xcenter=xcenter_p2,
ycenter=ycenter_p2, origin=origin_p2,
tar_spec=normalSED,
band_start=brange[0], band_end=brange[1],
conf=chip.sls_conf[1],
isAlongY=0,
flat_cube=flat_cube)
# self.addSLStoChipImage(sdp=sdp_p2, chip=chip, xOrderSigPlus = xOrderSigPlus, local_wcs=chip_wcs_local)
pos_shear = self.addSLStoChipImageWithPSF(sdp=sdp_p2, chip=chip, pos_img_local=[xcenter_p2, ycenter_p2],
psf_model=psf_model, bandNo=i + 1,
grating_split_pos=grating_split_pos,
local_wcs=chip_wcs_local, pos_img = pos_img)
del sdp_p1
del sdp_p2
elif grating_split_pos_chip<=gal_origin[1]:
sdp = SpecDisperser(orig_img=starImg, xcenter=x_nominal - 0,
ycenter=y_nominal - 0, origin=origin_star,
tar_spec=normalSED,
band_start=brange[0], band_end=brange[1],
conf=chip.sls_conf[1],
isAlongY=0,
flat_cube=flat_cube)
# self.addSLStoChipImage(sdp=sdp, chip=chip, xOrderSigPlus = xOrderSigPlus, local_wcs=chip_wcs_local)
pos_shear = self.addSLStoChipImageWithPSF(sdp=sdp, chip=chip, pos_img_local=[x_nominal, y_nominal],
psf_model=psf_model, bandNo=i + 1,
grating_split_pos=grating_split_pos,
local_wcs=chip_wcs_local, pos_img = pos_img)
del sdp
elif grating_split_pos_chip>=gal_end[1]:
sdp = SpecDisperser(orig_img=starImg, xcenter=x_nominal - 0,
ycenter=y_nominal - 0, origin=origin_star,
tar_spec=normalSED,
band_start=brange[0], band_end=brange[1],
conf=chip.sls_conf[0],
isAlongY=0,
flat_cube=flat_cube)
# self.addSLStoChipImage(sdp=sdp, chip=chip, xOrderSigPlus = xOrderSigPlus, local_wcs=chip_wcs_local)
pos_shear = self.addSLStoChipImageWithPSF(sdp=sdp, chip=chip, pos_img_local=[x_nominal, y_nominal],
psf_model=psf_model, bandNo=i + 1,
grating_split_pos=grating_split_pos,
local_wcs=chip_wcs_local, pos_img = pos_img)
del sdp
del photons_list # print(self.y_nominal, starImg.center.y, starImg.ymin)
del stamp # del psf
gc.collect() return 1, pos_shear
return True, pos_shear
config/config_C6_fits.yaml
View file @ d4b41c36
...@@ -9,9 +9,11 @@ ...@@ -9,9 +9,11 @@
# Base diretories and naming setup # Base diretories and naming setup
# Can add some of the command-line arguments here as well; # Can add some of the command-line arguments here as well;
# OK to pass either way or both, as long as they are consistent # OK to pass either way or both, as long as they are consistent
work_dir: "/share/simudata/CSSOSDataProductsSims/data/CSSTSimImage_C6/" work_dir: "/share/simudata/CSSOSDataProductsSims/data/CSSTSimImage_C8/"
data_dir: "/share/simudata/CSSOSDataProductsSims/data/" data_dir: "/share/simudata/CSSOSDataProductsSims/data/"
run_name: "C6_fits_testRun" run_name: "testRun_fits"
project_cycle: 6
run_counter: 1
# Whether to use MPI # Whether to use MPI
run_option: run_option:
...@@ -46,7 +48,7 @@ catalog_options: ...@@ -46,7 +48,7 @@ catalog_options:
#stamp_SED: #stamp_SED:
# Only simulate stars? # Only simulate stars?
star_only: NO star_only: YES
# Only simulate galaxies? # Only simulate galaxies?
galaxy_only: NO galaxy_only: NO
...@@ -63,13 +65,23 @@ catalog_options: ...@@ -63,13 +65,23 @@ catalog_options:
# Observation setting # Observation setting
############################################### ###############################################
obs_setting: obs_setting:
# Options for survey types: # Options for survey types:
# "Photometric": simulate photometric chips only # "Photometric": simulate photometric chips only
# "Spectroscopic": simulate slitless spectroscopic chips only # "Spectroscopic": simulate slitless spectroscopic chips only
# "FGS": simulate FGS chips only (31-42) # "FGS": simulate FGS chips only (31-42)
# "All": simulate full focal plane # "All": simulate full focal plane
survey_type: "Photometric" # "CALIBRATION": falt, bias, dark with or without postflash
survey_type: "All"
# "LED": ['LED1','LED2','LED3','LED4','LED5','LED6','LED7','LED8','LED9','LED10','LED11','LED12','LED13','LED14'] or null
# 'LED1': '275', 'LED2': '310', 'LED3': '430', 'LED4': '505', 'LED5': '545', 'LED6': '590', 'LED7': '670',
# 'LED8': '760', 'LED9': '940', 'LED10': '940', 'LED11': '1050', 'LED12': '1050','LED13': '340', 'LED14': '365'
# LED_TYPE: ['LED5']
# LED_TIME: [1.]
# # unit e- ,flat level
# FLAT_LEVEL: 20000
# FLAT_LEVEL_FIL: 'g'
# Exposure time [seconds] # Exposure time [seconds]
exp_time: 150. exp_time: 150.
...@@ -79,19 +91,17 @@ obs_setting: ...@@ -79,19 +91,17 @@ obs_setting:
# Default Pointing [degrees] # Default Pointing [degrees]
# Note: NOT valid when a pointing list file is specified # Note: NOT valid when a pointing list file is specified
ra_center: 244.972773 ra_center: 192.8595
dec_center: 39.895901 dec_center: 27.1283
# Image rotation [degree] # Image rotation [degree]
image_rot: 109.59 image_rot: -113.4333
# (Optional) a file of point list # (Optional) a file of point list
# if you just want to run default pointing: # if you just want to run default pointing:
# - pointing_dir: null # - pointing_dir: null
# - pointing_file: null # - pointing_file: null
pointing_dir: "/share/simudata/CSSOSDataProductsSims/data/" pointing_dir: "/share/simudata/CSSOSDataProductsSims/data/"
pointing_file: "pointing_radec_246.5_40.dat" pointing_file: "pointing_radec_246.5_40.dat"
# pointing_dir: null
# pointing_file: null
# Number of calibration pointings # Number of calibration pointings
np_cal: 0 np_cal: 0
...@@ -101,21 +111,25 @@ obs_setting: ...@@ -101,21 +111,25 @@ obs_setting:
# - run all pointings: null # - run all pointings: null
# Note: only valid when a pointing list is specified # Note: only valid when a pointing list is specified
run_pointings: [0] run_pointings: [0]
# Run specific chip(s): # Run specific chip(s):
# - give a list of indexes of chips: [ip_1, ip_2...] # - give a list of indexes of chips: [ip_1, ip_2...]
# - run all chips: null # - run all chips: null
# Note: for all pointings # Note: for all pointings
run_chips: [7] run_chips: [1, 2, 3, 7, 8, 9]
# Whether to enable astrometric modeling # Whether to enable astrometric modeling
enable_astrometric_model: False enable_astrometric_model: True
# Whether to enable straylight model
enable_straylight_model: True
# Cut by saturation magnitude in which band? # Cut by saturation magnitude in which band?
cut_in_band: "z" cut_in_band: "z"
# saturation magnitude margin # saturation magnitude margin
mag_sat_margin: -2.5 # mag_sat_margin: -2.5
mag_sat_margin: -15.
# limiting magnitude margin # limiting magnitude margin
mag_lim_margin: +1.0 mag_lim_margin: +1.0
...@@ -138,7 +152,7 @@ psf_setting: ...@@ -138,7 +152,7 @@ psf_setting:
# path to PSF data # path to PSF data
# NOTE: only valid for "Interp" PSF # NOTE: only valid for "Interp" PSF
psf_dir: "/share/simudata/CSSOSDataProductsSims/data/psfCube1" psf_dir: "/share/simudata/CSSOSDataProductsSims/data/psfCube1"
psf_sls_dir: "/share/simudata/CSSOSDataProductsSims/data/SLS_PSF_PCA_fp/"
############################################### ###############################################
# Shear setting # Shear setting
############################################### ###############################################
...@@ -160,25 +174,27 @@ ins_effects: ...@@ -160,25 +174,27 @@ ins_effects:
# switches # switches
# Note: bias_16channel, gain_16channel, and shutter_effect # Note: bias_16channel, gain_16channel, and shutter_effect
# is currently not applicable to "FGS" observations # is currently not applicable to "FGS" observations
field_dist: OFF # Whether to add field distortions field_dist: YES # Whether to add field distortions
add_back: OFF # Whether to add sky background add_back: YES # Whether to add sky background
add_dark: OFF # Whether to add dark noise add_dark: YES # Whether to add dark noise
add_readout: OFF # Whether to add read-out (Gaussian) noise add_readout: YES # Whether to add read-out (Gaussian) noise
add_bias: OFF # Whether to add bias-level to images add_bias: YES # Whether to add bias-level to images
bias_16channel: OFF # Whether to add different biases for 16 channels bias_16channel: YES # Whether to add different biases for 16 channels
gain_16channel: OFF # Whether to make different gains for 16 channels gain_16channel: YES # Whether to make different gains for 16 channels
shutter_effect: OFF # Whether to add shutter effect shutter_effect: YES # Whether to add shutter effect
flat_fielding: OFF # Whether to add flat-fielding effect flat_fielding: YES # Whether to add flat-fielding effect
prnu_effect: OFF # Whether to add PRNU effect prnu_effect: YES # Whether to add PRNU effect
non_linear: OFF # Whether to add non-linearity non_linear: YES # Whether to add non-linearity
cosmic_ray: OFF # Whether to add cosmic-ray cosmic_ray: YES # Whether to add cosmic-ray
cray_differ: OFF # Whether to generate different cosmic ray maps CAL and MS output cray_differ: YES # Whether to generate different cosmic ray maps CAL and MS output
cte_trail: OFF # Whether to simulate CTE trails cte_trail: NO # Whether to simulate CTE trails, CTI_lgl_v0.3.tar.gz
saturbloom: OFF # Whether to simulate Saturation & Blooming saturbloom: YES # Whether to simulate Saturation & Blooming
add_badcolumns: OFF # Whether to add bad columns add_badcolumns: YES # Whether to add bad columns
add_hotpixels: OFF # Whether to add hot pixels add_hotpixels: YES # Whether to add hot pixels
add_deadpixels: OFF # Whether to add dead(dark) pixels add_deadpixels: YES # Whether to add dead(dark) pixels
bright_fatter: OFF # Whether to simulate Brighter-Fatter (also diffusion) effect bright_fatter: YES # Whether to simulate Brighter-Fatter (also diffusion) effect
add_prescan: NO # Whether to add pre/over-scan
format_output: NO ##1*16 output
# Values: # Values:
# default values have been defined individually for each chip in: # default values have been defined individually for each chip in:
...@@ -220,4 +236,4 @@ random_seeds: ...@@ -220,4 +236,4 @@ random_seeds:
seed_badcolumns: 20240309 # Seed for bad columns seed_badcolumns: 20240309 # Seed for bad columns
seed_defective: 20210304 # Seed for defective (bad) pixels seed_defective: 20210304 # Seed for defective (bad) pixels
seed_readout: 20210601 # Seed for read-out gaussian noise seed_readout: 20210601 # Seed for read-out gaussian noise
... ...
\ No newline at end of file
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