Skip to content
GitLab
Projects
Groups
Snippets
/
Help
Help
Support
Community forum
Keyboard shortcuts
?
Submit feedback
Contribute to GitLab
Sign in
Toggle navigation
Menu
Open sidebar
csst-sims
csst_ifs_sim
Commits
b4201fbc
Commit
b4201fbc
authored
Apr 13, 2024
by
Yan Zhaojun
Browse files
more case test
parent
e985dd75
Pipeline
#4002
passed with stage
in 0 seconds
Changes
1
Pipelines
1
Hide whitespace changes
Inline
Side-by-side
csst_ifs_sim/csst_ifs_sim.py
View file @
b4201fbc
...
@@ -117,50 +117,50 @@ def transRaDec2D(ra, dec):
...
@@ -117,50 +117,50 @@ def transRaDec2D(ra, dec):
###############################################################################
###############################################################################
def
flux2ill
(
wave
,
flux
):
#
def flux2ill(wave, flux):
"""
#
"""
Parameters
#
Parameters
----------
#
----------
wave : TYPE
#
wave : TYPE
DESCRIPTION.
#
DESCRIPTION.
flux : TYPE
#
flux : TYPE
DESCRIPTION.
#
DESCRIPTION.
Returns
#
Returns
-------
#
-------
E : TYPE
#
E : TYPE
DESCRIPTION.
#
DESCRIPTION.
"""
#
"""
# erg/s/cm^2/A/arcsec^2 to W/m^2
#
# erg/s/cm^2/A/arcsec^2 to W/m^2
# 1 W/m^2/sr/μm = 0.10 erg/cm^2/s/sr/A
#
# 1 W/m^2/sr/μm = 0.10 erg/cm^2/s/sr/A
# 1 sr = 1 rad^2 = 4.25452e10 arcsec^2
#
# 1 sr = 1 rad^2 = 4.25452e10 arcsec^2
# 1 J/s = 1 W
#
# 1 J/s = 1 W
# 1 J = 10^7 erg
#
# 1 J = 10^7 erg
# convert erg/s/cm^2/A/arcsec^2 to erg/s/cm^2/A/sr
#
# convert erg/s/cm^2/A/arcsec^2 to erg/s/cm^2/A/sr
flux1
=
flux
/
(
1
/
4.25452e10
)
#
flux1 = flux / (1/4.25452e10)
# convert erg/s/cm^2/A/sr to W/m^2/sr/um
#
# convert erg/s/cm^2/A/sr to W/m^2/sr/um
flux2
=
flux1
*
10
#
flux2 = flux1 * 10
# 对接收面积积分,输出单位 W/m^2/nm
#
# 对接收面积积分,输出单位 W/m^2/nm
D
=
2
# meter
#
D = 2 # meter
f
=
28
# meter
#
f = 28 # meter
flux3
=
flux2
*
np
.
pi
*
D
**
2
/
4
/
f
**
2
/
10
**
3
#
flux3 = flux2 * np.pi * D**2 / 4 / f**2 / 10**3
# 对波长积分
#
# 对波长积分
f
=
interp1d
(
wave
,
flux3
)
#
f = interp1d(wave, flux3)
wave_interp
=
np
.
arange
(
3800
,
7800
)
#
wave_interp = np.arange(3800, 7800)
flux3_interp
=
f
(
wave_interp
)
#
flux3_interp = f(wave_interp)
# 输出单位 W/m^2
#
# 输出单位 W/m^2
delta_lamba
=
0.1
# nm
#
delta_lamba = 0.1 # nm
E
=
np
.
sum
(
flux3_interp
*
delta_lamba
)
#
E = np.sum(flux3_interp * delta_lamba)
return
E
#
return E
################################################################
################################################################
...
@@ -391,25 +391,25 @@ class StrayLight(object):
...
@@ -391,25 +391,25 @@ class StrayLight(object):
###############################################################################
###############################################################################
def
str2time
(
strTime
):
#
def str2time(strTime):
"""
#
"""
Parameters
#
Parameters
----------
#
----------
strTime : TYPE
#
strTime : TYPE
DESCRIPTION.
#
DESCRIPTION.
Returns
#
Returns
-------
#
-------
TYPE
#
TYPE
DESCRIPTION.
#
DESCRIPTION.
"""
#
"""
if
len
(
strTime
)
>
20
:
# 暂时未用到
#
if len(strTime) > 20: # 暂时未用到
msec
=
int
(
float
(
'0.'
+
strTime
[
20
:])
*
1000000
)
# 微秒
#
msec = int(float('0.'+strTime[20:])*1000000) # 微秒
str2
=
strTime
[
0
:
19
]
+
' '
+
str
(
msec
)
#
str2 = strTime[0:19]+' '+str(msec)
return
datetime
.
strptime
(
str2
,
'%Y %m %d %H %M %S %f'
)
#
return datetime.strptime(str2, '%Y %m %d %H %M %S %f')
# datetime类转mjd
# datetime类转mjd
##########################################################################
##########################################################################
...
@@ -822,40 +822,40 @@ def centroid(data):
...
@@ -822,40 +822,40 @@ def centroid(data):
return
float
(
cx
),
float
(
cy
)
return
float
(
cx
),
float
(
cy
)
###############################################################################
###############################################################################
def
centroidN
(
data
):
#
def centroidN(data):
"""
#
"""
Parameters
#
Parameters
----------
#
----------
data : TYPE
#
data : TYPE
DESCRIPTION.
#
DESCRIPTION.
Returns
#
Returns
-------
#
-------
cx : TYPE
#
cx : TYPE
DESCRIPTION.
#
DESCRIPTION.
cy : TYPE
#
cy : TYPE
DESCRIPTION.
#
DESCRIPTION.
"""
#
"""
'''
#
'''
calculate the centroid of the input two-dimentional image data
#
calculate the centroid of the input two-dimentional image data
Parameters
#
Parameters
----------
#
----------
data : input image.
#
data : input image.
Returns
#
Returns
-------
#
-------
cx: the centroid column number, in horizontal direction definet in python image show
#
cx: the centroid column number, in horizontal direction definet in python image show
cy: the centroid row number , in vertical direction
#
cy: the centroid row number , in vertical direction
'''
#
'''
###
#
###
from
scipy
import
ndimage
#
from scipy import ndimage
cy
,
cx
=
ndimage
.
center_of_mass
(
data
)
#
cy, cx = ndimage.center_of_mass(data)
return
cx
,
cy
#
return cx, cy
####################################################################
####################################################################
...
@@ -1494,42 +1494,42 @@ class IFSsimulator():
...
@@ -1494,42 +1494,42 @@ class IFSsimulator():
return
wave_A
,
spec_erg2
return
wave_A
,
spec_erg2
##########################################################################
##########################################################################
def
smoothingWithChargeDiffusion
(
self
,
image
,
sigma
=
(
0.32
,
0.32
)):
#
def smoothingWithChargeDiffusion(self, image, sigma=(0.32, 0.32)):
"""
#
"""
Parameters
#
Parameters
----------
#
----------
image : TYPE
#
image : TYPE
DESCRIPTION.
#
DESCRIPTION.
sigma : TYPE, optional
#
sigma : TYPE, optional
DESCRIPTION. The default is (0.32, 0.32).
#
DESCRIPTION. The default is (0.32, 0.32).
Returns
#
Returns
-------
#
-------
TYPE
#
TYPE
DESCRIPTION.
#
DESCRIPTION.
"""
#
"""
"""
#
"""
Smooths a given image with a gaussian kernel with widths given as sigmas.
#
Smooths a given image with a gaussian kernel with widths given as sigmas.
This smoothing can be used to mimic charge diffusion within the CCD.
#
This smoothing can be used to mimic charge diffusion within the CCD.
The default values are from Table 8-2 of CCD_273_Euclid_secification_1.0.130812.pdf converted
#
The default values are from Table 8-2 of CCD_273_Euclid_secification_1.0.130812.pdf converted
to sigmas (FWHM / (2sqrt(2ln2)) and rounded up to the second decimal.
#
to sigmas (FWHM / (2sqrt(2ln2)) and rounded up to the second decimal.
.. Note:: This method should not be called for the full image if the charge spreading
#
.. Note:: This method should not be called for the full image if the charge spreading
has already been taken into account in the system PSF to avoid double counting.
#
has already been taken into account in the system PSF to avoid double counting.
:param image: image array which is smoothed with the kernel
#
:param image: image array which is smoothed with the kernel
:type image: ndarray
#
:type image: ndarray
:param sigma: widths of the gaussian kernel that approximates the charge diffusion [0.32, 0.32].
#
:param sigma: widths of the gaussian kernel that approximates the charge diffusion [0.32, 0.32].
:param sigma: tuple
#
:param sigma: tuple
:return: smoothed image array
#
:return: smoothed image array
:rtype: ndarray
#
:rtype: ndarray
"""
#
"""
return
ndimage
.
filters
.
gaussian_filter
(
image
,
sigma
)
#
return ndimage.filters.gaussian_filter(image, sigma)
###############################################################################
###############################################################################
def
readCosmicRayInformation
(
self
):
def
readCosmicRayInformation
(
self
):
...
@@ -1835,88 +1835,88 @@ class IFSsimulator():
...
@@ -1835,88 +1835,88 @@ class IFSsimulator():
######################################################################
######################################################################
##############################################################################
##############################################################################
def
generateflat
(
self
,
ave
=
1.0
,
sigma
=
0.01
):
#
def generateflat(self, ave=1.0, sigma=0.01):
"""
#
"""
Parameters
#
Parameters
----------
#
----------
ave : TYPE, optional
#
ave : TYPE, optional
DESCRIPTION. The default is 1.0.
#
DESCRIPTION. The default is 1.0.
sigma : TYPE, optional
#
sigma : TYPE, optional
DESCRIPTION. The default is 0.01.
#
DESCRIPTION. The default is 0.01.
Returns
#
Returns
-------
#
-------
TYPE
#
TYPE
DESCRIPTION.
#
DESCRIPTION.
TYPE
#
TYPE
DESCRIPTION.
#
DESCRIPTION.
"""
#
"""
"""
#
"""
Creates a flat field image with given properties.
#
Creates a flat field image with given properties.
:return: flat field image
#
:return: flat field image
:rtype: ndarray
#
:rtype: ndarray
"""
#
"""
self
.
log
.
info
(
'Generating a flat field...'
)
#
self.log.info('Generating a flat field...')
self
.
log
.
info
(
'The flat field has mean value of 1 and a given fluctuations, usually either 1 or 2 percent defined by sigma= %d...'
%
sigma
)
#
self.log.info('The flat field has mean value of 1 and a given fluctuations, usually either 1 or 2 percent defined by sigma= %d...' % sigma)
np
.
random
.
seed
(
5
*
self
.
simnumber
)
#
np.random.seed(5*self.simnumber)
self
.
flat_b
=
np
.
random
.
normal
(
loc
=
ave
,
scale
=
sigma
,
size
=
(
2048
,
4096
))
#
self.flat_b = np.random.normal(loc=ave, scale=sigma, size=(2048, 4096))
np
.
random
.
seed
(
55
*
self
.
simnumber
)
#
np.random.seed(55*self.simnumber)
self
.
flat_r
=
np
.
random
.
normal
(
loc
=
ave
,
scale
=
sigma
,
size
=
(
3072
,
6144
))
#
self.flat_r = np.random.normal(loc=ave, scale=sigma, size=(3072, 6144))
s1
=
self
.
flat_b
#
s1 = self.flat_b
hdu1
=
fits
.
PrimaryHDU
(
s1
)
#
hdu1 = fits.PrimaryHDU(s1)
hdu1
.
header
.
set
(
'sigma'
,
sigma
)
#
hdu1.header.set('sigma', sigma)
dtime
=
datetime
.
utcnow
().
strftime
(
'%Y -%m -%d %H: %M: %S'
)
#
dtime = datetime.utcnow().strftime('%Y -%m -%d %H: %M: %S')
hdu1
.
header
.
add_history
(
#
hdu1.header.add_history(
'flat image of blue channel is generated on :'
+
dtime
)
#
'flat image of blue channel is generated on :'+dtime)
f1
=
'../flat_Blue_'
+
str
(
sigma
)
+
'.fits'
#
f1 = '../flat_Blue_'+str(sigma)+'.fits'
fits
.
writeto
(
f1
,
s1
,
header
=
hdu1
.
header
,
overwrite
=
True
)
#
fits.writeto(f1, s1, header=hdu1.header, overwrite=True)
s2
=
self
.
flat_r
#
s2 = self.flat_r
hdu1
=
fits
.
PrimaryHDU
(
s2
)
#
hdu1 = fits.PrimaryHDU(s2)
hdu1
.
header
.
set
(
'sigma'
,
sigma
)
#
hdu1.header.set('sigma', sigma)
dtime
=
datetime
.
utcnow
().
strftime
(
'%Y -%m -%d %H: %M: %S'
)
#
dtime = datetime.utcnow().strftime('%Y -%m -%d %H: %M: %S')
hdu1
.
header
.
add_history
(
#
hdu1.header.add_history(
'flat image of red channel is generated on :'
+
dtime
)
#
'flat image of red channel is generated on :'+dtime)
f2
=
'../flat_Red_'
+
str
(
sigma
)
+
'.fits'
#
f2 = '../flat_Red_'+str(sigma)+'.fits'
fits
.
writeto
(
f2
,
s2
,
header
=
hdu1
.
header
,
overwrite
=
True
)
#
fits.writeto(f2, s2, header=hdu1.header, overwrite=True)
return
self
.
flat_b
,
self
.
flat_r
#
return self.flat_b, self.flat_r
##########################################################################
##########################################################################
def
addLampFlux
(
self
):
#
def addLampFlux(self):
"""
#
"""
Returns
#
Returns
-------
#
-------
None.
#
None.
"""
#
"""
"""
#
"""
Include flux from the calibration source.
#
Include flux from the calibration source.
"""
#
"""
self
.
image_b
+=
fits
.
getdata
(
self
.
information
[
'flatflux'
])
#
self.image_b += fits.getdata(self.information['flatflux'])
self
.
image_r
+=
fits
.
getdata
(
self
.
information
[
'flatflux'
])
#
self.image_r += fits.getdata(self.information['flatflux'])
self
.
log
.
info
(
'Flux from the calibration unit included (%s)'
%
#
self.log.info('Flux from the calibration unit included (%s)' %
self
.
information
[
'flatflux'
])
#
self.information['flatflux'])
#############################################################################
#############################################################################
def
MakeFlatMatrix
(
self
,
img
,
seed
):
def
MakeFlatMatrix
(
self
,
img
,
seed
):
...
@@ -2111,69 +2111,69 @@ class IFSsimulator():
...
@@ -2111,69 +2111,69 @@ class IFSsimulator():
##########################################################
##########################################################
#########################################################################
#########################################################################
def
addReadoutTrails
(
self
):
#
def addReadoutTrails(self):
"""
#
"""
Returns
#
Returns
-------
#
-------
None.
#
None.
"""
#
"""
"""
#
"""
Add readout trails resulting from reading out the shutter open.
#
Add readout trails resulting from reading out the shutter open.
Quadrants assumed to be numbered:
#
Quadrants assumed to be numbered:
2 3
#
2 3
0 1
#
0 1
"""
#
"""
flux_ratio
=
self
.
information
[
'readouttime'
]
/
float
(
#
flux_ratio = self.information['readouttime'] / float(
self
.
information
[
'bluesize'
])
/
self
.
information
[
'exptime'
]
#
self.information['bluesize']) / self.information['exptime']
# make a copy, this will be updated
#
# make a copy, this will be updated
data
=
self
.
image_b
.
copy
()
#
data = self.image_b.copy()
# Amplifier at different positions depending on the quadrant number !
#
# Amplifier at different positions depending on the quadrant number !
# left side is 0, 2 and right side is 1, 3 starting from bottom i.e.
#
# left side is 0, 2 and right side is 1, 3 starting from bottom i.e.
# going clock wise from lower left we have 0, 2, 3, and 1 quadrants.
#
# going clock wise from lower left we have 0, 2, 3, and 1 quadrants.
if
self
.
information
[
'quadrant'
]
in
(
2
,
3
):
#
if self.information['quadrant'] in (2, 3):
data
=
data
[::
-
1
,
:]
#
data = data[::-1, :]
data_shift
=
data
.
copy
()
*
flux_ratio
#
data_shift = data.copy() * flux_ratio
size1
,
size2
=
data
.
shape
#
size1, size2 = data.shape
for
i
in
range
(
1
,
size2
,
1
):
#
for i in range(1, size2, 1):
data_shift2
=
np
.
roll
(
data_shift
,
i
,
axis
=
0
)
#
data_shift2 = np.roll(data_shift, i, axis=0)
data_shift2
[:
i
,
:]
=
0.0
#
data_shift2[:i, :] = 0.0
data
+=
data_shift2
#
data += data_shift2
if
self
.
information
[
'quadrant'
]
in
(
2
,
3
):
#
if self.information['quadrant'] in (2, 3):
self
.
image_b
=
data
[::
-
1
,
:]
#
self.image_b = data[::-1, :]
else
:
#
else:
self
.
image_b
=
data
#
self.image_b = data
flux_ratio
=
self
.
information
[
'readouttime'
]
/
float
(
#
flux_ratio = self.information['readouttime'] / float(
self
.
information
[
'redsize'
])
/
self
.
information
[
'exptime'
]
#
self.information['redsize']) / self.information['exptime']
# make a copy, this will be updated
#
# make a copy, this will be updated
data
=
self
.
image_r
.
copy
()
#
data = self.image_r.copy()
# Amplifier at different positions depending on the quadrant number !
#
# Amplifier at different positions depending on the quadrant number !
# left side is 0, 2 and right side is 1, 3 starting from bottom i.e.
#
# left side is 0, 2 and right side is 1, 3 starting from bottom i.e.
# going clock wise from lower left we have 0, 2, 3, and 1 quadrants.
#
# going clock wise from lower left we have 0, 2, 3, and 1 quadrants.
if
self
.
information
[
'quadrant'
]
in
(
2
,
3
):
#
if self.information['quadrant'] in (2, 3):
data
=
data
[::
-
1
,
:]
#
data = data[::-1, :]
data_shift
=
data
.
copy
()
*
flux_ratio
#
data_shift = data.copy() * flux_ratio
size1
,
size2
=
data
.
shape
#
size1, size2 = data.shape
for
i
in
range
(
1
,
size2
,
1
):
#
for i in range(1, size2, 1):
data_shift2
=
np
.
roll
(
data_shift
,
i
,
axis
=
0
)
#
data_shift2 = np.roll(data_shift, i, axis=0)
data_shift2
[:
i
,
:]
=
0.0
#
data_shift2[:i, :] = 0.0
data
+=
data_shift2
#
data += data_shift2
if
self
.
information
[
'quadrant'
]
in
(
2
,
3
):
#
if self.information['quadrant'] in (2, 3):
self
.
image_r
=
data
[::
-
1
,
:]
#
self.image_r = data[::-1, :]
else
:
#
else:
self
.
image_r
=
data
#
self.image_r = data
##############################################################################
##############################################################################
...
@@ -2259,24 +2259,24 @@ class IFSsimulator():
...
@@ -2259,24 +2259,24 @@ class IFSsimulator():
##########################################################################
##########################################################################
def
applyScatteredLight
(
self
):
#
def applyScatteredLight(self):
"""
#
"""
Returns
#
Returns
-------
#
-------
None.
#
None.
"""
#
"""
"""
#
"""
Adds spatially uniform scattered light to the image.
#
Adds spatially uniform scattered light to the image.
"""
#
"""
sl
=
self
.
information
[
'exptime'
]
*
self
.
information
[
'scattered_light'
]
#
sl = self.information['exptime'] * self.information['scattered_light']
self
.
image_b
+=
sl
#
self.image_b += sl
self
.
image_r
+=
sl
#
self.image_r += sl
self
.
log
.
info
(
'Added scattered light = %f'
%
sl
)
#
self.log.info('Added scattered light = %f' % sl)
##############################################################################
##############################################################################
def
applyPoissonNoise
(
self
):
def
applyPoissonNoise
(
self
):
...
...
Write
Preview
Supports
Markdown
0%
Try again
or
attach a new file
.
Cancel
You are about to add
0
people
to the discussion. Proceed with caution.
Finish editing this message first!
Cancel
Please
register
or
sign in
to comment