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Commit f6a0c574 authored by Yan Zhaojun's avatar Yan Zhaojun
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csst_mci_sim/mci_data/mci_all_9K.config deleted 100755 → 0
View file @ bd72dad4
[TEST]
dir_path=mci_sim/MCI_inputData/
result_path=mci_sim/mci_sim_result/
ver=C10
#size of the output image array, xsize is column, ysize is row, xsize = 9216,ysize = 9232
xsize =9216
ysize =9232
##overscanx = column, overscany =row
prescan = 27
overscan = 320
#charge trap information file
parallelTrapfile=MCI_inputData/data/cdm_euclid_parallel.dat
serialTrapfile=MCI_inputData/data/cdm_euclid_serial.dat
#cosmetic defects input file
cosmeticsFile_g =MCI_inputData/data/Cosmetics_g.txt
cosmeticsFile_r =MCI_inputData/data/Cosmetics_r.txt
cosmeticsFile_i =MCI_inputData/data/Cosmetics_i.txt
###comicray information file
cosmicraylengths=MCI_inputData/data/cdf_cr_length.dat
cosmicraydistance=MCI_inputData/data/cdf_cr_total.dat
##################################################
#### ####
####Control flags (can be yes/no, true/false) ####
##################################################
cosmicRays = yes
darknoise = yes
cosmetics = yes
radiationDamage= yes
bleeding = yes
overscans = yes
nonlinearity = yes
readoutNoise = yes
skyback = yes
TianceEffect = yes
intscale = yes
ghosts = yes
shutterEffect = yes
flatfieldM = yes
PRNUeffect = yes
appFatt = no
sky_shift_rot = yes
distortion = yes
sim_star = no
sim_galaxy = yes
save_starpsf = no
save_cosmicrays = no
lensing = yes
##############################################
##############################################
#CCD properties
fullwellcapacity = 90000
#dark noise in electrons per second
dark = 0.001
#exposure to simulate, exposure time
exptime = 300.0
###PNRU matrix sigma
flatsigma=0.001
### cosmicray coveringFraction
coveringFraction=0.1
#offset from the object, note that at the moment this is fixed, but in reality a focal plane position dependent.
ghostOffsetX = 100
ghostOffsetY = 100
ghostRatio = 1e-04
####treering effect,bright fatter effect and difusion effect
treering=0.1
fatter=1.0
difusion=0.1
### the choosen Filters in three CCDs
filter_g=u
filter_r=F555W
filter_i=F814W
##['G_filters']=["F275W", "F280N","NUV", "WU", "CBU", "F343N", "u", "F373N", "F395N"," F336W"]
##['R_filters']=["F487N", "F502N", "CBV", "r", "F656N", "F658N", "F467M", "F555W", "F606W", "F673N"]
##['I_filters']=["z", "y", "F815N", "CBI", "F925N", "F960M", "F968N", "F845M" ,"F850LP" ,"F814W"]
####################
g_gain1=1.53
g_gain2=1.54
g_gain3=1.55
g_gain4=1.53
g_gain5=1.51
g_gain6=1.56
g_gain7=1.58
g_gain8=1.53
g_gain9=1.54
g_gain10=1.57
g_gain11=1.51
g_gain12=1.53
g_gain13=1.55
g_gain14=1.57
g_gain15=1.53
g_gain16=1.52
#######################
g_rdnois1=4.53
g_rdnois2=4.54
g_rdnois3=4.55
g_rdnois4=4.53
g_rdnois5=4.51
g_rdnois6=4.56
g_rdnois7=4.58
g_rdnois8=4.53
g_rdnois9=4.54
g_rdnois10=4.57
g_rdnois11=4.51
g_rdnois12=4.53
g_rdnois13=4.55
g_rdnois14=4.57
g_rdnois15=4.53
g_rdnois16=4.52
############################
g_detbia1=500
g_detbia2=510
g_detbia3=514
g_detbia4=520
g_detbia5=524
g_detbia6=540
g_detbia7=530
g_detbia8=532
g_detbia9=534
g_detbia10=526
g_detbia11=532
g_detbia12=516
g_detbia13=540
g_detbia14=560
g_detbia15=536
g_detbia16=528
############################
r_gain1=1.52
r_gain2=1.54
r_gain3=1.52
r_gain4=1.55
r_gain5=1.56
r_gain6=1.52
r_gain7=1.54
r_gain8=1.6
r_gain9=1.54
r_gain10=1.52
r_gain11=1.54
r_gain12=1.57
r_gain13=1.52
r_gain14=1.55
r_gain15=1.52
r_gain16=1.55
################################
r_rdnois1=4.23
r_rdnois2=4.24
r_rdnois3=4.25
r_rdnois4=4.23
r_rdnois5=4.21
r_rdnois6=4.26
r_rdnois7=4.28
r_rdnois8=4.23
r_rdnois9=4.24
r_rdnois10=4.27
r_rdnois11=4.21
r_rdnois12=4.23
r_rdnois13=4.25
r_rdnois14=4.27
r_rdnois15=4.23
r_rdnois16=4.22
###################################
r_detbia1=600
r_detbia2=610
r_detbia3=614
r_detbia4=620
r_detbia5=624
r_detbia6=640
r_detbia7=630
r_detbia8=632
r_detbia9=634
r_detbia10=626
r_detbia11=632
r_detbia12=616
r_detbia13=640
r_detbia14=660
r_detbia15=636
r_detbia16=628
###################################
i_gain1=1.62
i_gain2=1.64
i_gain3=1.62
i_gain4=1.65
i_gain5=1.66
i_gain6=1.62
i_gain7=1.64
i_gain8=1.6
i_gain9=1.64
i_gain10=1.62
i_gain11=1.64
i_gain12=1.67
i_gain13=1.62
i_gain14=1.65
i_gain15=1.62
i_gain16=1.65
###################################
i_rdnois1=4.63
i_rdnois2=4.64
i_rdnois3=4.65
i_rdnois4=4.63
i_rdnois5=4.61
i_rdnois6=4.66
i_rdnois7=4.68
i_rdnois8=4.63
i_rdnois9=4.64
i_rdnois10=4.67
i_rdnois11=4.61
i_rdnois12=4.63
i_rdnois13=4.65
i_rdnois14=4.67
i_rdnois15=4.63
i_rdnois16=4.62
#######################################
i_detbia1=400
i_detbia2=410
i_detbia3=414
i_detbia4=420
i_detbia5=424
i_detbia6=440
i_detbia7=430
i_detbia8=432
i_detbia9=434
i_detbia10=426
i_detbia11=432
i_detbia12=416
i_detbia13=440
i_detbia14=460
i_detbia15=436
i_detbia16=428
####### end #######################
csst_mci_sim/support/sed.py
View file @ f6a0c574
...@@ -121,103 +121,103 @@ def calibrate(wave, flux, mag, path, band='GAIA_bp'): ...@@ -121,103 +121,103 @@ def calibrate(wave, flux, mag, path, band='GAIA_bp'):
# SED Template # SED Template
class Gal_Temp(): # class Gal_Temp():
""" # """
Template of Galaxy SED # Template of Galaxy SED
""" # """
def __init__(self, log, path): # def __init__(self, log, path):
# # #
# parent = os.path.dirname(os.path.realpath(__file__)) # # parent = os.path.dirname(os.path.realpath(__file__))
self.path = path # self.path = path
hdulist = fits.open( # hdulist = fits.open(
self.path+'MCI_inputData/SED_Code/seddata/galaxy_temp.fits') # self.path+'MCI_inputData/SED_Code/seddata/galaxy_temp.fits')
if len(hdulist) < 4: # if len(hdulist) < 4:
log.error( # log.error(
'Data error in galaxy_temp.fits file, please check!!!') # 'Data error in galaxy_temp.fits file, please check!!!')
raise ValueError( # raise ValueError(
'Data error in galaxy_temp.fits file, please check!!!') # 'Data error in galaxy_temp.fits file, please check!!!')
self.wave = hdulist[1].data['wave'] # self.wave = hdulist[1].data['wave']
self.flux = hdulist[2].data # self.flux = hdulist[2].data
self.age_grid = hdulist[3].data['logAge'] # self.age_grid = hdulist[3].data['logAge']
self.feh_grid = hdulist[3].data['FeH'] # self.feh_grid = hdulist[3].data['FeH']
def toMag(self, redshift=0): # def toMag(self, redshift=0):
"""Calculating magnitude # """Calculating magnitude
Args: # Args:
redshift (float, optional): redshift of spectra. Defaults to 0. # redshift (float, optional): redshift of spectra. Defaults to 0.
""" # """
wave = self.wave * (1 + redshift) # wave = self.wave * (1 + redshift)
self.umag = flux_to_mag(wave, self.flux, self.path, band='SDSS_u') # self.umag = flux_to_mag(wave, self.flux, self.path, band='SDSS_u')
self.gmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_g') # self.gmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_g')
self.rmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_r') # self.rmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_r')
self.imag = flux_to_mag(wave, self.flux, self.path, band='SDSS_i') # self.imag = flux_to_mag(wave, self.flux, self.path, band='SDSS_i')
self.zmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_z') # self.zmag = flux_to_mag(wave, self.flux, self.path, band='SDSS_z')
class Star_Temp(): # class Star_Temp():
""" # """
Template of Stellar SED # Template of Stellar SED
""" # """
def __init__(self, path): # def __init__(self, path):
# # #
self.path = path # self.path = path
# parent = os.path.dirname(os.path.realpath(__file__)) # # parent = os.path.dirname(os.path.realpath(__file__))
# print("获取其父目录——" + parent) # 从当前文件路径中获取目录 # # print("获取其父目录——" + parent) # 从当前文件路径中获取目录
hdulist = fits.open( # hdulist = fits.open(
os.path.join(path, 'MCI_inputData/SED_Code/seddata/stellar_temp_wrong.fits')) # os.path.join(path, 'MCI_inputData/SED_Code/seddata/stellar_temp_wrong.fits'))
if len(hdulist) < 4: # if len(hdulist) < 4:
self.log.error( # self.log.error(
'Data error in galaxy_temp.fits file, please check!!!') # 'Data error in galaxy_temp.fits file, please check!!!')
raise ValueError( # raise ValueError(
'Data error in galaxy_temp.fits file, please check!!!') # 'Data error in galaxy_temp.fits file, please check!!!')
self.wave = hdulist[1].data['wave'] # self.wave = hdulist[1].data['wave']
self.flux = hdulist[2].data # self.flux = hdulist[2].data
self.Teff_grid = hdulist[3].data['Teff'] # self.Teff_grid = hdulist[3].data['Teff']
self.FeH_grid = hdulist[3].data['FeH'] # self.FeH_grid = hdulist[3].data['FeH']
self.bpmag = flux_to_mag(self.wave, self.flux, path, band='GAIA_bp') # self.bpmag = flux_to_mag(self.wave, self.flux, path, band='GAIA_bp')
self.rpmag = flux_to_mag(self.wave, self.flux, path, band='GAIA_rp') # self.rpmag = flux_to_mag(self.wave, self.flux, path, band='GAIA_rp')
def toMag(self): # def toMag(self):
wave = self.wave # wave = self.wave
self.bpmag = flux_to_mag(wave, self.flux, self.path, band='GAIA_bp') # self.bpmag = flux_to_mag(wave, self.flux, self.path, band='GAIA_bp')
self.rpmag = flux_to_mag(wave, self.flux, self.path, band='GAIA_rp') # self.rpmag = flux_to_mag(wave, self.flux, self.path, band='GAIA_rp')
# ------------- # -------------
# SED Modelling # SED Modelling
def Model_Stellar_SED(wave, bp, rp, temp): # def Model_Stellar_SED(wave, bp, rp, temp):
"""Modelling stellar SED based on bp, rp magnitude # """Modelling stellar SED based on bp, rp magnitude
Args: # Args:
wave (float): Wavelength # wave (float): Wavelength
bp (float): Magnitude of GAIA BP band # bp (float): Magnitude of GAIA BP band
rp (float): Magnitude of GAIA RP band # rp (float): Magnitude of GAIA RP band
temp (class): Class of stellar template # temp (class): Class of stellar template
Returns: # Returns:
float array: Spectral energy distribution of stellar SED, # float array: Spectral energy distribution of stellar SED,
which have the same length to the input wave # which have the same length to the input wave
""" # """
color0 = bp - rp # color0 = bp - rp
colors = temp.bpmag - temp.rpmag # colors = temp.bpmag - temp.rpmag
idx = np.argmin(np.abs(colors - color0)) # idx = np.argmin(np.abs(colors - color0))
flux0 = temp.flux[idx] # flux0 = temp.flux[idx]
flux1 = np.interp(wave, temp.wave, flux0) # flux1 = np.interp(wave, temp.wave, flux0)
flux = calibrate(wave, flux1, rp, band='GAIA_rp') # flux = calibrate(wave, flux1, rp, band='GAIA_rp')
return flux # return flux
def Model_Galaxy_SED(wave, ugriz, z, temp, path): def Model_Galaxy_SED(wave, ugriz, z, temp, path):
......
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