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Liu Dezi
csst_msc_sim
Commits
a88bded7
Commit
a88bded7
authored
Oct 07, 2023
by
Zhang Xin
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parent
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tests/TestSpecDisperse.py
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tests/TestStraylight.py
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import
unittest
from
ObservationSim.Straylight
import
Straylight
import
numpy
as
np
import
math
import
astropy.constants
as
cons
import
galsim
from
astropy.table
import
Table
from
scipy
import
interpolate
import
matplotlib.pyplot
as
plt
hubbleAverZodiacal
=
{
'nuv'
:
0.0035
,
'u'
:
0.0163
,
'g'
:
0.1109
,
'r'
:
0.1471
,
'i'
:
0.1568
,
'z'
:
0.0953
,
'y'
:
0.0283
}
hubbleAverEarthShine
=
{
'nuv'
:
0.00024
,
'u'
:
0.0051
,
'g'
:
0.0506
,
'r'
:
0.0591
,
'i'
:
0.0568
,
'z'
:
0.0315
,
'y'
:
0.0090
}
def
transRaDec2D
(
ra
,
dec
):
x1
=
np
.
cos
(
dec
/
57.2957795
)
*
np
.
cos
(
ra
/
57.2957795
);
y1
=
np
.
cos
(
dec
/
57.2957795
)
*
np
.
sin
(
ra
/
57.2957795
);
z1
=
np
.
sin
(
dec
/
57.2957795
);
return
np
.
array
([
x1
,
y1
,
z1
])
def
getAngle132
(
x1
=
0
,
y1
=
0
,
z1
=
0
,
x2
=
0
,
y2
=
0
,
z2
=
0
,
x3
=
0
,
y3
=
0
,
z3
=
0
):
cosValue
=
0
;
angle
=
0
;
x11
=
x1
-
x3
;
y11
=
y1
-
y3
;
z11
=
z1
-
z3
;
x22
=
x2
-
x3
;
y22
=
y2
-
y3
;
z22
=
z2
-
z3
;
tt
=
np
.
sqrt
((
x11
*
x11
+
y11
*
y11
+
z11
*
z11
)
*
(
x22
*
x22
+
y22
*
y22
+
z22
*
z22
));
if
(
tt
==
0
):
return
0
;
cosValue
=
(
x11
*
x22
+
y11
*
y22
+
z11
*
z22
)
/
tt
;
if
(
cosValue
>
1
):
cosValue
=
1
;
if
(
cosValue
<
-
1
):
cosValue
=
-
1
;
angle
=
math
.
acos
(
cosValue
);
return
angle
*
360
/
(
2
*
math
.
pi
);
def
calculateAnglePwithEarth
(
sat
=
np
.
array
([
0
,
0
,
0
]),
pointing
=
np
.
array
([
0
,
0
,
0
]),
sun
=
np
.
array
([
0
,
0
,
0
])):
modSat
=
np
.
sqrt
(
sat
[
0
]
*
sat
[
0
]
+
sat
[
1
]
*
sat
[
1
]
+
sat
[
2
]
*
sat
[
2
])
modPoint
=
np
.
sqrt
(
pointing
[
0
]
*
pointing
[
0
]
+
pointing
[
1
]
*
pointing
[
1
]
+
pointing
[
2
]
*
pointing
[
2
])
withLocalZenithAngle
=
(
pointing
[
0
]
*
sat
[
0
]
+
pointing
[
1
]
*
sat
[
1
]
+
pointing
[
2
]
*
sat
[
2
])
/
(
modPoint
*
modSat
)
innerM_sat_sun
=
sat
[
0
]
*
sun
[
0
]
+
sat
[
1
]
*
sun
[
1
]
+
sat
[
2
]
*
sun
[
2
]
cosAngle
=
innerM_sat_sun
/
(
modSat
*
cons
.
au
.
value
/
1000
)
isInSunSide
=
1
if
(
cosAngle
<
-
0.3385737
):
#cos109.79
isInSunSide
=
-
1
;
elif
cosAngle
>=
-
0.3385737
and
cosAngle
<=
0.3385737
:
isInSunSide
=
0
;
return
math
.
acos
(
withLocalZenithAngle
)
*
180
/
math
.
pi
,
isInSunSide
class
TestStraylight
(
unittest
.
TestCase
):
def
__init__
(
self
,
methodName
=
'runTest'
,
datFn
=
''
,
filter
=
'i'
,
grating
=
"GI"
):
super
(
TestStraylight
,
self
).
__init__
(
methodName
)
self
.
pointingData
=
np
.
loadtxt
(
datFn
,
dtype
=
np
.
double
)
self
.
filter
=
filter
self
.
grating
=
grating
def
test_EarthShineFilter
(
self
):
d_sh
=
self
.
pointingData
.
shape
sl_e_pix
=
np
.
zeros
([
d_sh
[
0
],
3
],
dtype
=
np
.
double
)
for
i
in
np
.
arange
(
d_sh
[
0
]):
# if i > 50:
# continue
ju
=
self
.
pointingData
[
i
,
5
]
# pointing = transRaDec2D(self.pointingData[i, 0], self.pointingData[i, 1])
# print(ju, pointing, surveylist[i,3:9])
sl
=
Straylight
(
jtime
=
ju
,
sat_pos
=
self
.
pointingData
[
i
,
6
:
9
],
pointing_radec
=
np
.
array
([
self
.
pointingData
[
i
,
0
],
self
.
pointingData
[
i
,
1
]]),
sun_pos
=
self
.
pointingData
[
i
,
9
:
12
])
e1
,
py
=
sl
.
calculateEarthShineFilter
(
filter
=
self
.
filter
)
earthZenithAngle
,
isInSunSide
=
calculateAnglePwithEarth
(
sat
=
self
.
pointingData
[
i
,
6
:
9
],
pointing
=
sl
.
pointing
,
sun
=
self
.
pointingData
[
i
,
9
:
12
])
# e2, _ = sl.calculateZodiacalFilter2(filter='i', sun_pos=sl.sun_pos)
# e3 = sl.calculateStarLightFilter(filter='i', pointYaxis=py)
# e_all = sl.calculateStrayLightFilter(filter='i')
# s_pix, spec = sl.calculateStrayLightGrating(grating='GI')
sl_e_pix
[
i
,
0
]
=
e1
sl_e_pix
[
i
,
1
]
=
earthZenithAngle
sl_e_pix
[
i
,
2
]
=
isInSunSide
median
=
np
.
median
(
sl_e_pix
[:,
0
])
print
(
' average Earthshine %s: %e'
%
(
self
.
filter
,
median
))
self
.
assertTrue
(
median
-
hubbleAverEarthShine
[
self
.
filter
]
<
0.1
)
plt
.
figure
()
ids1
=
sl_e_pix
[:,
2
]
==
1
ids2
=
sl_e_pix
[:,
2
]
!=
1
plt
.
plot
(
sl_e_pix
[
ids1
,
0
],
sl_e_pix
[
ids1
,
1
],
'r.'
)
plt
.
plot
(
sl_e_pix
[
ids2
,
0
],
sl_e_pix
[
ids2
,
1
],
'b.'
)
plt
.
legend
([
'In Sun Side'
,
'In Earths shadow'
])
plt
.
xlabel
(
'straylight-earthshine(e-/pixel/s)'
)
plt
.
ylabel
(
'Angle with local zenith(degree)'
)
plt
.
show
()
def
test_ZodiacalFilter
(
self
):
d_sh
=
self
.
pointingData
.
shape
sl_e_pix
=
np
.
zeros
([
d_sh
[
0
],
2
],
dtype
=
np
.
double
)
for
i
in
np
.
arange
(
d_sh
[
0
]):
ju
=
self
.
pointingData
[
i
,
5
]
sl
=
Straylight
(
jtime
=
ju
,
sat_pos
=
self
.
pointingData
[
i
,
6
:
9
],
pointing_radec
=
np
.
array
([
self
.
pointingData
[
i
,
0
],
self
.
pointingData
[
i
,
1
]]),
sun_pos
=
self
.
pointingData
[
i
,
9
:
12
])
e1
,
_
=
sl
.
calculateZodiacalFilter2
(
filter
=
self
.
filter
,
sun_pos
=
sl
.
sun_pos
)
sl_e_pix
[
i
,
0
]
=
e1
sl_e_pix
[
i
,
1
]
=
getAngle132
(
x1
=
self
.
pointingData
[
i
,
9
],
y1
=
self
.
pointingData
[
i
,
10
],
z1
=
self
.
pointingData
[
i
,
11
],
x2
=
sl
.
pointing
[
0
],
y2
=
sl
.
pointing
[
1
],
z2
=
sl
.
pointing
[
2
],
x3
=
0
,
y3
=
0
,
z3
=
0
)
plt
.
figure
()
plt
.
plot
(
sl_e_pix
[:,
0
],
sl_e_pix
[:,
1
],
'r.'
)
plt
.
xlabel
(
'straylight-zodiacal(e-/pixel/s)'
)
plt
.
ylabel
(
'Angle between pointing and sun(degree)'
)
plt
.
show
()
median
=
np
.
median
(
sl_e_pix
[:,
0
])
print
(
' average Zodiacal %s: %f'
%
(
self
.
filter
,
median
))
self
.
assertTrue
(
median
-
hubbleAverZodiacal
[
self
.
filter
]
<
0.1
)
def
test_StarFilter
(
self
):
d_sh
=
self
.
pointingData
.
shape
sl_e_pix
=
np
.
zeros
(
d_sh
[
0
],
dtype
=
np
.
double
)
tnum
=
10
for
i
in
np
.
arange
(
tnum
):
# if i > 50:
# continue
ju
=
self
.
pointingData
[
i
,
5
]
# pointing = transRaDec2D(self.pointingData[i, 0], self.pointingData[i, 1])
# print(ju, pointing, surveylist[i,3:9])
sl
=
Straylight
(
jtime
=
ju
,
sat_pos
=
self
.
pointingData
[
i
,
6
:
9
],
pointing_radec
=
np
.
array
([
self
.
pointingData
[
i
,
0
],
self
.
pointingData
[
i
,
1
]]),
sun_pos
=
self
.
pointingData
[
i
,
9
:
12
])
e1
,
py
=
sl
.
calculateEarthShineFilter
(
filter
=
self
.
filter
)
# e2, _ = sl.calculateZodiacalFilter2(filter='i', sun_pos=sl.sun_pos)
e3
=
sl
.
calculateStarLightFilter
(
filter
=
self
.
filter
,
pointYaxis
=
py
)
# e_all = sl.calculateStrayLightFilter(filter='i')
# s_pix, spec = sl.calculateStrayLightGrating(grating='GI')
sl_e_pix
[
i
]
=
e3
median
=
np
.
median
(
sl_e_pix
[
0
:
tnum
])
print
(
' average Earthshine %s: %e'
%
(
self
.
filter
,
median
))
self
.
assertTrue
(
median
-
hubbleAverEarthShine
[
self
.
filter
]
<
0.2
)
def
test_GratingStraylight
(
self
):
d_sh
=
self
.
pointingData
.
shape
sl_e_pix
=
np
.
zeros
(
d_sh
[
0
],
dtype
=
np
.
double
)
tnum
=
10
for
i
in
np
.
arange
(
tnum
):
# if i > 50:
# continue
ju
=
self
.
pointingData
[
i
,
5
]
# pointing = transRaDec2D(self.pointingData[i, 0], self.pointingData[i, 1])
# print(ju, pointing, surveylist[i,3:9])
sl
=
Straylight
(
jtime
=
ju
,
sat_pos
=
self
.
pointingData
[
i
,
6
:
9
],
pointing_radec
=
np
.
array
([
self
.
pointingData
[
i
,
0
],
self
.
pointingData
[
i
,
1
]]),
sun_pos
=
self
.
pointingData
[
i
,
9
:
12
])
# e1, py = sl.calculateEarthShineFilter(filter=self.filter)
# e2, _ = sl.calculateZodiacalFilter2(filter='i', sun_pos=sl.sun_pos)
# e3 = sl.calculateStarLightFilter(filter=self.filter, pointYaxis=py)
# e_all = sl.calculateStrayLightFilter(filter='i')
s_pix
,
spec
=
sl
.
calculateStrayLightGrating
(
grating
=
self
.
grating
)
sl_e_pix
[
i
]
=
s_pix
plt
.
figure
()
plt
.
plot
(
spec
[
'WAVELENGTH'
],
spec
[
'FLUX'
],
'r'
)
plt
.
xlabel
(
'WAVELENGTH'
)
plt
.
ylabel
(
'F$\lambda$(erg/s/cm2/A/arcsec2)'
)
plt
.
xlim
(
2000
,
10000
)
plt
.
show
()
median
=
np
.
median
(
sl_e_pix
[
0
:
tnum
])
print
(
' average Earthshine %s: %e'
%
(
self
.
grating
,
median
))
self
.
assertTrue
(
median
<
0.8
)
if
__name__
==
'__main__'
:
suit
=
unittest
.
TestSuite
()
# case1 = TestStraylight('test_EarthShineFilter',datFn = 'Straylight_test.dat', filter = 'i')
# suit.addTest(case1)
# case2 = TestStraylight('test_ZodiacalFilter',datFn = 'Straylight_test.dat',filter = 'i')
# suit.addTest(case2)
# case3 = TestStraylight('test_StarFilter', datFn='Straylight_test.dat', filter='i')
# suit.addTest(case3)
case4
=
TestStraylight
(
'test_GratingStraylight'
,
datFn
=
'Straylight_test.dat'
,
grating
=
'GI'
)
suit
.
addTest
(
case4
)
unittest
.
TextTestRunner
(
verbosity
=
2
).
run
(
suit
)
\ No newline at end of file
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