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Liu Dezi
csst_msc_sim
Commits
88aea0d6
Commit
88aea0d6
authored
Apr 02, 2024
by
Fang Yuedong
Browse files
split sim steps into multiple files
parent
3d7404e7
Changes
11
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Inline
Side-by-side
ObservationSim/ObservationSim.py
View file @
88aea0d6
...
@@ -14,7 +14,7 @@ from ObservationSim.Instrument.Chip import Effects
...
@@ -14,7 +14,7 @@ from ObservationSim.Instrument.Chip import Effects
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
from
ObservationSim._util
import
makeSubDir_PointingList
from
ObservationSim._util
import
makeSubDir_PointingList
from
ObservationSim.Astrometry.Astrometry_util
import
on_orbit_obs_position
from
ObservationSim.Astrometry.Astrometry_util
import
on_orbit_obs_position
from
ObservationSim.
S
im
S
teps
import
SimSteps
,
SIM_STEP_TYPES
from
ObservationSim.
s
im
_s
teps
import
SimSteps
,
SIM_STEP_TYPES
class
Observation
(
object
):
class
Observation
(
object
):
def
__init__
(
self
,
config
,
Catalog
,
work_dir
=
None
,
data_dir
=
None
):
def
__init__
(
self
,
config
,
Catalog
,
work_dir
=
None
,
data_dir
=
None
):
...
...
ObservationSim/SimSteps.py
deleted
100644 → 0
View file @
3d7404e7
This diff is collapsed.
Click to expand it.
ObservationSim/sim_steps/__init__.py
0 → 100644
View file @
88aea0d6
import
os
class
SimSteps
:
def
__init__
(
self
,
overall_config
,
chip_output
,
all_filters
):
self
.
overall_config
=
overall_config
self
.
chip_output
=
chip_output
self
.
all_filters
=
all_filters
from
.prepare_headers
import
prepare_headers
from
.add_sky_background
import
add_sky_background_sci
,
add_sky_flat_calibration
,
add_sky_background
from
.add_objects
import
add_objects
from
.add_cosmic_rays
import
add_cosmic_rays
from
.add_pattern_noise
import
apply_PRNU
,
add_poisson_and_dark
,
add_detector_defects
,
add_nonlinearity
,
add_blooming
,
add_bias
from
.add_brighter_fatter_CTE
import
add_brighter_fatter
,
apply_CTE
from
.readout_output
import
add_prescan_overscan
,
add_readout_noise
,
apply_gain
,
quantization_and_output
SIM_STEP_TYPES
=
{
"scie_obs"
:
"add_objects"
,
"sky_background"
:
"add_sky_background"
,
"cosmic_rays"
:
"add_cosmic_rays"
,
"PRNU_effect"
:
"apply_PRNU"
,
"poisson_and_dark"
:
"add_poisson_and_dark"
,
"bright_fatter"
:
"add_brighter_fatter"
,
"detector_defects"
:
"add_detector_defects"
,
"nonlinearity"
:
"add_nonlinearity"
,
"blooming"
:
"add_blooming"
,
"CTE_effect"
:
"apply_CTE"
,
"prescan_overscan"
:
"add_prescan_overscan"
,
"bias"
:
"add_bias"
,
"readout_noise"
:
"add_readout_noise"
,
"gain"
:
"apply_gain"
,
"quantization_and_output"
:
"quantization_and_output"
,
"led_calib_model"
:
"add_LED_Flat"
,
"sky_flatField"
:
"add_sky_flat_calibration"
,
}
\ No newline at end of file
ObservationSim/sim_steps/add_LED_flat.py
0 → 100644
View file @
88aea0d6
import
numpy
as
np
from
ObservationSim.MockObject
import
FlatLED
def
add_LED_Flat
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
if
not
hasattr
(
self
,
'h_ext'
):
_
,
_
=
self
.
prepare_headers
(
chip
=
chip
,
pointing
=
pointing
)
chip_wcs
=
galsim
.
FitsWCS
(
header
=
self
.
h_ext
)
pf_map
=
np
.
zeros_like
(
chip
.
img
.
array
)
if
obs_param
[
"LED_TYPE"
]
is
not
None
:
if
len
(
obs_param
[
"LED_TYPE"
])
!=
0
:
print
(
"LED OPEN--------"
)
led_obj
=
FlatLED
(
chip
,
filt
)
led_flat
=
led_obj
.
drawObj_LEDFlat
(
led_type_list
=
obs_param
[
"LED_TYPE"
],
exp_t_list
=
obs_param
[
"LED_TIME"
])
pf_map
=
led_flat
chip
.
img
=
chip
.
img
+
led_flat
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/add_brighter_fatter_CTE.py
0 → 100644
View file @
88aea0d6
import
numpy
as
np
import
galsim
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
from
ObservationSim.Instrument.Chip.libCTI.CTI_modeling
import
CTI_sim
def
add_brighter_fatter
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
chip
.
img
=
chip_utils
.
add_brighter_fatter
(
img
=
chip
.
img
)
return
chip
,
filt
,
tel
,
pointing
def
apply_CTE
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Apply CTE Effect"
)
### 2*8 -> 1*16 img-layout
img
=
chip_utils
.
formatOutput
(
GSImage
=
chip
.
img
)
chip
.
nsecy
=
1
chip
.
nsecx
=
16
img_arr
=
img
.
array
ny
,
nx
=
img_arr
.
shape
dx
=
int
(
nx
/
chip
.
nsecx
)
dy
=
int
(
ny
/
chip
.
nsecy
)
newimg
=
galsim
.
Image
(
nx
,
int
(
ny
+
chip
.
overscan_y
),
init_value
=
0
)
for
ichannel
in
range
(
16
):
print
(
'
\n
***add CTI effects: pointing-{:} chip-{:} channel-{:}***'
.
format
(
pointing
.
id
,
chip
.
chipID
,
ichannel
+
1
))
noverscan
,
nsp
,
nmax
=
chip
.
overscan_y
,
3
,
10
beta
,
w
,
c
=
0.478
,
84700
,
0
t
=
np
.
array
([
0.74
,
7.7
,
37
],
dtype
=
np
.
float32
)
rho_trap
=
np
.
array
([
0.6
,
1.6
,
1.4
],
dtype
=
np
.
float32
)
trap_seeds
=
np
.
array
([
0
,
1000
,
10000
],
dtype
=
np
.
int32
)
+
ichannel
+
chip
.
chipID
*
16
release_seed
=
50
+
ichannel
+
pointing
.
id
*
30
+
chip
.
chipID
*
16
newimg
.
array
[:,
0
+
ichannel
*
dx
:
dx
+
ichannel
*
dx
]
=
CTI_sim
(
img_arr
[:,
0
+
ichannel
*
dx
:
dx
+
ichannel
*
dx
],
dx
,
dy
,
noverscan
,
nsp
,
nmax
,
beta
,
w
,
c
,
t
,
rho_trap
,
trap_seeds
,
release_seed
)
newimg
.
wcs
=
img
.
wcs
del
img
img
=
newimg
### 1*16 -> 2*8 img-layout
chip
.
img
=
chip_utils
.
formatRevert
(
GSImage
=
img
)
chip
.
nsecy
=
2
chip
.
nsecx
=
8
# [TODO] make overscan_y == 0
chip
.
overscan_y
=
0
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/add_cosmic_rays.py
0 → 100644
View file @
88aea0d6
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
def
add_cosmic_rays
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Adding Cosmic-Ray"
)
chip
.
img
,
crmap_gsimg
,
cr_event_num
=
chip_utils
.
add_cosmic_rays
(
img
=
chip
.
img
,
chip
=
chip
,
exptime
=
pointing
.
exp_time
,
seed
=
self
.
overall_config
[
"random_seeds"
][
"seed_CR"
]
+
pointing
.
id
*
30
+
chip
.
chipID
)
# [TODO] output cosmic ray image
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/add_objects.py
0 → 100644
View file @
88aea0d6
import
os
import
gc
import
psutil
import
numpy
as
np
import
galsim
from
ObservationSim._util
import
get_shear_field
from
ObservationSim.PSF
import
PSFGauss
,
FieldDistortion
,
PSFInterp
,
PSFInterpSLS
def
add_objects
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
# Prepare output file(s) for this chip
self
.
chip_output
.
create_output_file
()
# Prepare the PSF model
if
self
.
overall_config
[
"psf_setting"
][
"psf_model"
]
==
"Gauss"
:
psf_model
=
PSFGauss
(
chip
=
chip
,
psfRa
=
self
.
overall_config
[
"psf_setting"
][
"psf_rcont"
])
elif
self
.
overall_config
[
"psf_setting"
][
"psf_model"
]
==
"Interp"
:
if
chip
.
survey_type
==
"spectroscopic"
:
psf_model
=
PSFInterpSLS
(
chip
,
filt
,
PSF_data_prefix
=
self
.
overall_config
[
"psf_setting"
][
"psf_sls_dir"
])
else
:
psf_model
=
PSFInterp
(
chip
=
chip
,
npsf
=
chip
.
n_psf_samples
,
PSF_data_file
=
self
.
overall_config
[
"psf_setting"
][
"psf_pho_dir"
])
else
:
self
.
chip_output
.
Log_error
(
"unrecognized PSF model type!!"
,
flush
=
True
)
# Apply field distortion model
if
obs_param
[
"field_dist"
]
==
True
:
fd_model
=
FieldDistortion
(
chip
=
chip
,
img_rot
=
pointing
.
img_pa
.
deg
)
else
:
fd_model
=
None
# Update limiting magnitudes for all filters based on the exposure time
# Get the filter which will be used for magnitude cut
for
ifilt
in
range
(
len
(
self
.
all_filters
)):
temp_filter
=
self
.
all_filters
[
ifilt
]
temp_filter
.
update_limit_saturation_mags
(
exptime
=
pointing
.
get_full_depth_exptime
(
temp_filter
.
filter_type
),
chip
=
chip
)
if
temp_filter
.
filter_type
.
lower
()
==
self
.
overall_config
[
"obs_setting"
][
"cut_in_band"
].
lower
():
cut_filter
=
temp_filter
# Read in shear values from configuration file if the constant shear type is used
if
self
.
overall_config
[
"shear_setting"
][
"shear_type"
]
==
"constant"
:
g1_field
,
g2_field
,
_
=
get_shear_field
(
config
=
self
.
overall_config
)
self
.
chip_output
.
Log_info
(
"Use constant shear: g1=%.5f, g2=%.5f"
%
(
g1_field
,
g2_field
))
# Get chip WCS
if
not
hasattr
(
self
,
'h_ext'
):
_
,
_
=
self
.
prepare_headers
(
chip
=
chip
,
pointing
=
pointing
)
chip_wcs
=
galsim
.
FitsWCS
(
header
=
self
.
h_ext
)
# Loop over objects
nobj
=
len
(
catalog
.
objs
)
missed_obj
=
0
bright_obj
=
0
dim_obj
=
0
for
j
in
range
(
nobj
):
# # [DEBUG] [TODO]
# if j >= 10:
# break
obj
=
catalog
.
objs
[
j
]
# load and convert SED; also caculate object's magnitude in all CSST bands
try
:
sed_data
=
catalog
.
load_sed
(
obj
)
norm_filt
=
catalog
.
load_norm_filt
(
obj
)
obj
.
sed
,
obj
.
param
[
"mag_%s"
%
filt
.
filter_type
.
lower
()],
obj
.
param
[
"flux_%s"
%
filt
.
filter_type
.
lower
()]
=
catalog
.
convert_sed
(
mag
=
obj
.
param
[
"mag_use_normal"
],
sed
=
sed_data
,
target_filt
=
filt
,
norm_filt
=
norm_filt
,
)
_
,
obj
.
param
[
"mag_%s"
%
cut_filter
.
filter_type
.
lower
()],
obj
.
param
[
"flux_%s"
%
cut_filter
.
filter_type
.
lower
()]
=
catalog
.
convert_sed
(
mag
=
obj
.
param
[
"mag_use_normal"
],
sed
=
sed_data
,
target_filt
=
cut_filter
,
norm_filt
=
norm_filt
,
)
except
Exception
as
e
:
traceback
.
print_exc
()
self
.
chip_output
.
Log_error
(
e
)
continue
# [TODO] Testing
# self.chip_output.Log_info("mag_%s = %.3f"%(filt.filter_type.lower(), obj.param["mag_%s"%filt.filter_type.lower()]))
# Exclude very bright/dim objects (for now)
if
cut_filter
.
is_too_bright
(
mag
=
obj
.
param
[
"mag_%s"
%
self
.
overall_config
[
"obs_setting"
][
"cut_in_band"
].
lower
()],
margin
=
self
.
overall_config
[
"obs_setting"
][
"mag_sat_margin"
]):
self
.
chip_output
.
Log_info
(
"obj %s too birght!! mag_%s = %.3f"
%
(
obj
.
id
,
cut_filter
.
filter_type
,
obj
.
param
[
"mag_%s"
%
self
.
overall_config
[
"obs_setting"
][
"cut_in_band"
].
lower
()]))
bright_obj
+=
1
obj
.
unload_SED
()
continue
if
filt
.
is_too_dim
(
mag
=
obj
.
getMagFilter
(
filt
),
margin
=
self
.
overall_config
[
"obs_setting"
][
"mag_lim_margin"
]):
self
.
chip_output
.
Log_info
(
"obj %s too dim!! mag_%s = %.3f"
%
(
obj
.
id
,
filt
.
filter_type
,
obj
.
getMagFilter
(
filt
)))
dim_obj
+=
1
obj
.
unload_SED
()
continue
# Get corresponding shear values
if
self
.
overall_config
[
"shear_setting"
][
"shear_type"
]
==
"constant"
:
if
obj
.
type
==
'star'
:
obj
.
g1
,
obj
.
g2
=
0.
,
0.
else
:
# Figure out shear fields from overall configuration shear setting
obj
.
g1
,
obj
.
g2
=
g1_field
,
g2_field
elif
self
.
overall_config
[
"shear_setting"
][
"shear_type"
]
==
"catalog"
:
pass
else
:
self
.
chip_output
.
Log_error
(
"Unknown shear input"
)
raise
ValueError
(
"Unknown shear input"
)
# Get position of object on the focal plane
pos_img
,
_
,
_
,
_
,
fd_shear
=
obj
.
getPosImg_Offset_WCS
(
img
=
chip
.
img
,
fdmodel
=
fd_model
,
chip
=
chip
,
verbose
=
False
,
chip_wcs
=
chip_wcs
,
img_header
=
self
.
h_ext
)
# [TODO] For now, only consider objects which their centers (after field distortion) are projected within the focal plane
# Otherwise they will be considered missed objects
# if pos_img.x == -1 or pos_img.y == -1 or (not chip.isContainObj(x_image=pos_img.x, y_image=pos_img.y, margin=0.)):
if
pos_img
.
x
==
-
1
or
pos_img
.
y
==
-
1
:
self
.
chip_output
.
Log_info
(
'obj_ra = %.6f, obj_dec = %.6f, obj_ra_orig = %.6f, obj_dec_orig = %.6f'
%
(
obj
.
ra
,
obj
.
dec
,
obj
.
ra_orig
,
obj
.
dec_orig
))
self
.
chip_output
.
Log_error
(
"Objected missed: %s"
%
(
obj
.
id
))
missed_obj
+=
1
obj
.
unload_SED
()
continue
# Draw object & update output catalog
try
:
if
self
.
overall_config
[
"run_option"
][
"out_cat_only"
]:
isUpdated
=
True
obj
.
real_pos
=
obj
.
getRealPos
(
chip
.
img
,
global_x
=
obj
.
posImg
.
x
,
global_y
=
obj
.
posImg
.
y
,
img_real_wcs
=
obj
.
chip_wcs
)
pos_shear
=
0.
elif
chip
.
survey_type
==
"photometric"
and
not
self
.
overall_config
[
"run_option"
][
"out_cat_only"
]:
isUpdated
,
pos_shear
=
obj
.
drawObj_multiband
(
tel
=
tel
,
pos_img
=
pos_img
,
psf_model
=
psf_model
,
bandpass_list
=
filt
.
bandpass_sub_list
,
filt
=
filt
,
chip
=
chip
,
g1
=
obj
.
g1
,
g2
=
obj
.
g2
,
exptime
=
pointing
.
exp_time
,
fd_shear
=
fd_shear
)
elif
chip
.
survey_type
==
"spectroscopic"
and
not
self
.
overall_config
[
"run_option"
][
"out_cat_only"
]:
isUpdated
,
pos_shear
=
obj
.
drawObj_slitless
(
tel
=
tel
,
pos_img
=
pos_img
,
psf_model
=
psf_model
,
bandpass_list
=
filt
.
bandpass_sub_list
,
filt
=
filt
,
chip
=
chip
,
g1
=
obj
.
g1
,
g2
=
obj
.
g2
,
exptime
=
pointing
.
exp_time
,
normFilter
=
norm_filt
,
fd_shear
=
fd_shear
)
if
isUpdated
==
1
:
# TODO: add up stats
self
.
chip_output
.
cat_add_obj
(
obj
,
pos_img
,
pos_shear
)
pass
elif
isUpdated
==
0
:
missed_obj
+=
1
self
.
chip_output
.
Log_error
(
"Objected missed: %s"
%
(
obj
.
id
))
else
:
self
.
chip_output
.
Log_error
(
"Draw error, object omitted: %s"
%
(
obj
.
id
))
continue
except
Exception
as
e
:
traceback
.
print_exc
()
self
.
chip_output
.
Log_error
(
e
)
# Unload SED:
obj
.
unload_SED
()
del
obj
gc
.
collect
()
del
psf_model
gc
.
collect
()
self
.
chip_output
.
Log_info
(
"Running checkpoint #1 (Object rendering finished): pointing-%d chip-%d pid-%d memory-%6.2fGB"
%
(
pointing
.
id
,
chip
.
chipID
,
os
.
getpid
(),
(
psutil
.
Process
(
os
.
getpid
()).
memory_info
().
rss
/
1024
/
1024
/
1024
)
))
self
.
chip_output
.
Log_info
(
"# objects that are too bright %d out of %d"
%
(
bright_obj
,
nobj
))
self
.
chip_output
.
Log_info
(
"# objects that are too dim %d out of %d"
%
(
dim_obj
,
nobj
))
self
.
chip_output
.
Log_info
(
"# objects that are missed %d out of %d"
%
(
missed_obj
,
nobj
))
# Apply flat fielding (with shutter effects)
flat_normal
=
np
.
ones_like
(
chip
.
img
.
array
)
if
obs_param
[
"flat_fielding"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
flat_img
.
array
/
np
.
mean
(
chip
.
flat_img
.
array
)
if
obs_param
[
"shutter_effect"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
shutter_img
flat_normal
=
np
.
array
(
flat_normal
,
dtype
=
'float32'
)
chip
.
img
*=
flat_normal
del
flat_normal
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/add_pattern_noise.py
0 → 100644
View file @
88aea0d6
from
numpy.random
import
Generator
,
PCG64
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
from
ObservationSim.Instrument.Chip
import
Effects
def
apply_PRNU
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
chip
.
img
*=
chip
.
prnu_img
return
chip
,
filt
,
tel
,
pointing
def
add_poisson_and_dark
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
# Add dark current & Poisson noise
InputDark
=
False
if
obs_param
[
"add_dark"
]
==
True
:
if
InputDark
:
chip
.
img
=
chip_utils
.
add_inputdark
(
img
=
chip
.
img
,
chip
=
chip
,
exptime
=
pointing
.
exp_time
)
else
:
chip
.
img
,
_
=
chip_utils
.
add_poisson
(
img
=
chip
.
img
,
chip
=
chip
,
exptime
=
pointing
.
exp_time
,
poisson_noise
=
chip
.
poisson_noise
)
else
:
chip
.
img
,
_
=
chip_utils
.
add_poisson
(
img
=
chip
.
img
,
chip
=
self
,
exptime
=
pointing
.
exp_time
,
poisson_noise
=
chip
.
poisson_noise
,
dark_noise
=
0.
)
return
chip
,
filt
,
tel
,
pointing
def
add_detector_defects
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
# Add Hot Pixels or/and Dead Pixels
rgbadpix
=
Generator
(
PCG64
(
int
(
self
.
overall_config
[
"random_seeds"
][
"seed_defective"
]
+
chip
.
chipID
)))
badfraction
=
5E-5
*
(
rgbadpix
.
random
()
*
0.5
+
0.7
)
chip
.
img
=
Effects
.
DefectivePixels
(
chip
.
img
,
IfHotPix
=
obs_param
[
"hot_pixels"
],
IfDeadPix
=
obs_param
[
"dead_pixels"
],
fraction
=
badfraction
,
seed
=
self
.
overall_config
[
"random_seeds"
][
"seed_defective"
]
+
chip
.
chipID
,
biaslevel
=
0
)
# Apply Bad columns
if
obs_param
[
"bad_columns"
]
==
True
:
chip
.
img
=
Effects
.
BadColumns
(
chip
.
img
,
seed
=
self
.
overall_config
[
"random_seeds"
][
"seed_badcolumns"
],
chipid
=
chip
.
chipID
)
return
chip
,
filt
,
tel
,
pointing
def
add_nonlinearity
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Applying Non-Linearity on the chip image"
)
chip
.
img
=
Effects
.
NonLinearity
(
GSImage
=
chip
.
img
,
beta1
=
5.e-7
,
beta2
=
0
)
return
chip
,
filt
,
tel
,
pointing
def
add_blooming
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Applying CCD Saturation & Blooming"
)
chip
.
img
=
Effects
.
SaturBloom
(
GSImage
=
chip
.
img
,
nsect_x
=
1
,
nsect_y
=
1
,
fullwell
=
int
(
chip
.
full_well
))
return
chip
,
filt
,
tel
,
pointing
def
add_bias
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Adding Bias level and 16-channel non-uniformity"
)
if
obs_param
[
"bias_16channel"
]
==
True
:
chip
.
img
=
Effects
.
AddBiasNonUniform16
(
chip
.
img
,
bias_level
=
float
(
chip
.
bias_level
),
nsecy
=
chip
.
nsecy
,
nsecx
=
chip
.
nsecx
,
seed
=
self
.
overall_config
[
"random_seeds"
][
"seed_biasNonUniform"
]
+
chip
.
chipID
)
elif
obs_param
[
"bias_16channel"
]
==
False
:
chip
.
img
+=
self
.
bias_level
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/add_sky_background.py
0 → 100644
View file @
88aea0d6
import
numpy
as
np
import
galsim
from
ObservationSim.Straylight
import
calculateSkyMap_split_g
def
add_sky_background_sci
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
flat_normal
=
np
.
ones_like
(
chip
.
img
.
array
)
if
obs_param
[
"flat_fielding"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
flat_img
.
array
/
np
.
mean
(
chip
.
flat_img
.
array
)
if
obs_param
[
"shutter_effect"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
shutter_img
flat_normal
=
np
.
array
(
flat_normal
,
dtype
=
'float32'
)
if
obs_param
[
"enable_straylight_model"
]:
# Filter.sky_background, Filter.zodical_spec will be updated
filt
.
setFilterStrayLightPixel
(
jtime
=
pointing
.
jdt
,
sat_pos
=
np
.
array
([
pointing
.
sat_x
,
pointing
.
sat_y
,
pointing
.
sat_z
]),
pointing_radec
=
np
.
array
([
pointing
.
ra
,
pointing
.
dec
]),
sun_pos
=
np
.
array
([
pointing
.
sun_x
,
pointing
.
sun_y
,
pointing
.
sun_z
]))
self
.
chip_output
.
Log_info
(
"================================================"
)
self
.
chip_output
.
Log_info
(
"sky background + stray light pixel flux value: %.5f"
%
(
filt
.
sky_background
))
if
chip
.
survey_type
==
"photometric"
:
sky_map
=
filt
.
getSkyNoise
(
exptime
=
obs_param
[
"exptime"
])
sky_map
=
sky_map
*
np
.
ones_like
(
chip
.
img
.
array
)
*
flat_normal
sky_map
=
galsim
.
Image
(
array
=
sky_map
)
else
:
# chip.loadSLSFLATCUBE(flat_fn='flat_cube.fits')
sky_map
=
calculateSkyMap_split_g
(
skyMap
=
flat_normal
,
blueLimit
=
filt
.
blue_limit
,
redLimit
=
filt
.
red_limit
,
conf
=
chip
.
sls_conf
,
pixelSize
=
chip
.
pix_scale
,
isAlongY
=
0
,
flat_cube
=
chip
.
flat_cube
,
zoldial_spec
=
filt
.
zodical_spec
)
sky_map
=
(
sky_map
+
filt
.
sky_background
)
*
obs_param
[
"exptime"
]
# sky_map = sky_map * tel.pupil_area * obs_param["exptime"]
chip
.
img
+=
sky_map
return
chip
,
filt
,
tel
,
pointing
def
add_sky_flat_calibration
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
if
not
hasattr
(
self
,
'h_ext'
):
_
,
_
=
self
.
prepare_headers
(
chip
=
chip
,
pointing
=
pointing
)
chip_wcs
=
galsim
.
FitsWCS
(
header
=
self
.
h_ext
)
expTime
=
obs_param
[
"exptime"
]
skyback_level
=
obs_param
[
"flat_level"
]
filter_param
=
FilterParam
()
sky_level_filt
=
obs_param
[
"flat_level_filt"
]
norm_scaler
=
skyback_level
/
expTime
/
filter_param
.
param
[
sky_level_filt
][
5
]
flat_normal
=
np
.
ones_like
(
chip
.
img
.
array
)
if
obs_param
[
"flat_fielding"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
flat_img
.
array
/
np
.
mean
(
chip
.
flat_img
.
array
)
if
obs_param
[
"shutter_effect"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
shutter_img
flat_normal
=
np
.
array
(
flat_normal
,
dtype
=
'float32'
)
if
chip
.
survey_type
==
"photometric"
:
sky_map
=
flat_normal
*
np
.
ones_like
(
chip
.
img
.
array
)
*
norm_scaler
*
filter_param
.
param
[
chip
.
filter_type
][
5
]
/
tel
.
pupil_area
*
expTime
elif
chip
.
survey_type
==
"spectroscopic"
:
# flat_normal = np.ones_like(chip.img.array)
if
obs_param
[
"flat_fielding"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
flat_img
.
array
/
np
.
mean
(
chip
.
flat_img
.
array
)
if
obs_param
[
"shutter_effect"
]
==
True
:
flat_normal
=
flat_normal
*
chip
.
shutter_img
flat_normal
=
np
.
array
(
flat_normal
,
dtype
=
'float32'
)
sky_map
=
calculateSkyMap_split_g
(
skyMap
=
flat_normal
,
blueLimit
=
filt
.
blue_limit
,
redLimit
=
filt
.
red_limit
,
conf
=
chip
.
sls_conf
,
pixelSize
=
chip
.
pix_scale
,
isAlongY
=
0
,
flat_cube
=
chip
.
flat_cube
)
sky_map
=
sky_map
*
norm_scaler
*
expTime
chip
.
img
+=
sky_map
return
chip
,
filt
,
tel
,
pointing
def
add_sky_background
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
if
not
hasattr
(
self
,
'h_ext'
):
_
,
_
=
self
.
prepare_headers
(
chip
=
chip
,
pointing
=
pointing
)
chip_wcs
=
galsim
.
FitsWCS
(
header
=
self
.
h_ext
)
if
"flat_level"
not
in
obs_param
or
"flat_level_filt"
not
in
obs_param
:
chip
,
filt
,
tel
,
pointing
=
self
.
add_sky_background_sci
(
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
)
else
:
if
obs_param
.
get
(
'flat_level'
)
is
None
or
obs_param
.
get
(
'flat_level_filt'
)
is
None
:
chip
,
filt
,
tel
,
pointing
=
self
.
add_sky_background_sci
(
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
)
else
:
chip
,
filt
,
tel
,
pointing
=
self
.
add_sky_flat_calibration
(
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
)
return
chip
,
filt
,
tel
,
pointing
\ No newline at end of file
ObservationSim/sim_steps/prepare_headers.py
0 → 100644
View file @
88aea0d6
from
ObservationSim.Config.Header
import
generatePrimaryHeader
,
generateExtensionHeader
def
prepare_headers
(
self
,
chip
,
pointing
):
self
.
h_prim
=
generatePrimaryHeader
(
xlen
=
chip
.
npix_x
,
ylen
=
chip
.
npix_y
,
pointNum
=
str
(
pointing
.
id
),
ra
=
pointing
.
ra
,
dec
=
pointing
.
dec
,
pixel_scale
=
chip
.
pix_scale
,
time_pt
=
pointing
.
timestamp
,
exptime
=
pointing
.
exp_time
,
im_type
=
pointing
.
pointing_type
,
sat_pos
=
[
pointing
.
sat_x
,
pointing
.
sat_y
,
pointing
.
sat_z
],
sat_vel
=
[
pointing
.
sat_vx
,
pointing
.
sat_vy
,
pointing
.
sat_vz
],
project_cycle
=
self
.
overall_config
[
"project_cycle"
],
run_counter
=
self
.
overall_config
[
"run_counter"
],
chip_name
=
str
(
chip
.
chipID
).
rjust
(
2
,
'0'
))
self
.
h_ext
=
generateExtensionHeader
(
chip
=
chip
,
xlen
=
chip
.
npix_x
,
ylen
=
chip
.
npix_y
,
ra
=
pointing
.
ra
,
dec
=
pointing
.
dec
,
pa
=
pointing
.
img_pa
.
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
,
extName
=
pointing
.
pointing_type
,
timestamp
=
pointing
.
timestamp
,
exptime
=
pointing
.
exp_time
,
readoutTime
=
chip
.
readout_time
)
return
self
.
h_prim
,
self
.
h_ext
\ No newline at end of file
ObservationSim/sim_steps/readout_output.py
0 → 100644
View file @
88aea0d6
import
os
import
galsim
import
numpy
as
np
from
astropy.io
import
fits
from
ObservationSim.Instrument.Chip
import
ChipUtils
as
chip_utils
from
ObservationSim.Instrument.Chip
import
Effects
def
add_prescan_overscan
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
"Apply pre/over-scan"
)
chip
.
img
=
chip_utils
.
AddPreScan
(
GSImage
=
chip
.
img
,
pre1
=
chip
.
prescan_x
,
pre2
=
chip
.
prescan_y
,
over1
=
chip
.
overscan_x
,
over2
=
chip
.
overscan_y
)
return
chip
,
filt
,
tel
,
pointing
def
add_readout_noise
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
seed
=
int
(
self
.
overall_config
[
"random_seeds"
][
"seed_readout"
])
+
pointing
.
id
*
30
+
chip
.
chipID
rng_readout
=
galsim
.
BaseDeviate
(
seed
)
readout_noise
=
galsim
.
GaussianNoise
(
rng
=
rng_readout
,
sigma
=
chip
.
read_noise
)
chip
.
img
.
addNoise
(
readout_noise
)
return
chip
,
filt
,
tel
,
pointing
def
apply_gain
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
self
.
chip_output
.
Log_info
(
" Applying Gain"
)
if
obs_param
[
"gain_16channel"
]
==
True
:
chip
.
img
,
chip
.
gain_channel
=
Effects
.
ApplyGainNonUniform16
(
chip
.
img
,
gain
=
chip
.
gain
,
nsecy
=
chip
.
nsecy
,
nsecx
=
chip
.
nsecx
,
seed
=
self
.
overall_config
[
"random_seeds"
][
"seed_gainNonUniform"
]
+
chip
.
chipID
)
elif
obs_param
[
"gain_16channel"
]
==
False
:
chip
.
img
/=
chip
.
gain
return
chip
,
filt
,
tel
,
pointing
def
quantization_and_output
(
self
,
chip
,
filt
,
tel
,
pointing
,
catalog
,
obs_param
):
if
obs_param
[
"format_output"
]
==
True
:
self
.
chip_output
.
Log_info
(
" Apply 1*16 format"
)
chip
.
img
=
chip_utils
.
formatOutput
(
GSImage
=
chip
.
img
)
chip
.
nsecy
=
1
chip
.
nsecx
=
16
chip
.
img
.
array
[
chip
.
img
.
array
>
65535
]
=
65535
chip
.
img
.
replaceNegative
(
replace_value
=
0
)
chip
.
img
.
quantize
()
chip
.
img
=
galsim
.
Image
(
chip
.
img
.
array
,
dtype
=
np
.
uint16
)
hdu1
=
fits
.
PrimaryHDU
(
header
=
self
.
h_prim
)
hdu1
.
add_checksum
()
hdu1
.
header
.
comments
[
'CHECKSUM'
]
=
'HDU checksum'
hdu1
.
header
.
comments
[
'DATASUM'
]
=
'data unit checksum'
hdu2
=
fits
.
ImageHDU
(
chip
.
img
.
array
,
header
=
self
.
h_ext
)
hdu2
.
add_checksum
()
hdu2
.
header
.
comments
[
'XTENSION'
]
=
'extension type'
hdu2
.
header
.
comments
[
'CHECKSUM'
]
=
'HDU checksum'
hdu2
.
header
.
comments
[
'DATASUM'
]
=
'data unit checksum'
hdu2
.
header
.
comments
[
"XTENSION"
]
=
"image extension"
hdu1
=
fits
.
HDUList
([
hdu1
,
hdu2
])
fname
=
os
.
path
.
join
(
self
.
chip_output
.
subdir
,
self
.
h_prim
[
'FILENAME'
]
+
'.fits'
)
hdu1
.
writeto
(
fname
,
output_verify
=
'ignore'
,
overwrite
=
True
)
return
chip
,
filt
,
tel
,
pointing
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