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csst-sims
csst_mci_sim
Commits
4bb76b08
Commit
4bb76b08
authored
Oct 25, 2024
by
Yan Zhaojun
Browse files
Delete zodiacal.py
parent
5e1c7f2b
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csst_mci_sim/zodiacal.py
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import
numpy
as
np
import
julian
from
datetime
import
datetime
from
astropy.time
import
Time
from
astropy.coordinates
import
get_sun
from
astropy.coordinates
import
SkyCoord
import
pandas
as
pd
from
astropy
import
units
as
u
from
scipy
import
interpolate
def
zodiacal
(
ra
,
dec
,
time
,
path
):
"""
For given RA, DEC and TIME, return the interpolated zodical spectrum in Leinert-1998.
:param ra: RA in unit of degree, ICRS frame
:param dec: DEC in unit of degree, ICRS frame
:param time: the specified string that in ISO format i.e., yyyy-mm-dd.
:param path: the relative file path
:return:
wave_A: wavelength of the zodical spectrum
spec_erg: flux of the zodical spectrum, in unit of erg/s/cm^2/A/sr
"""
# get solar position
dt
=
datetime
.
fromisoformat
(
time
)
jd
=
julian
.
to_jd
(
dt
,
fmt
=
'jd'
)
###jd = time2jd(dt)
t
=
Time
(
jd
,
format
=
'jd'
,
scale
=
'utc'
)
astro_sun
=
get_sun
(
t
)
ra_sun
,
dec_sun
=
astro_sun
.
gcrs
.
ra
.
deg
,
astro_sun
.
gcrs
.
dec
.
deg
radec_sun
=
SkyCoord
(
ra
=
ra_sun
*
u
.
degree
,
dec
=
dec_sun
*
u
.
degree
,
frame
=
'gcrs'
)
lb_sun
=
radec_sun
.
transform_to
(
'geocentrictrueecliptic'
)
# get offsets between the target and sun.
radec_obj
=
SkyCoord
(
ra
=
ra
*
u
.
degree
,
dec
=
dec
*
u
.
degree
,
frame
=
'icrs'
)
lb_obj
=
radec_obj
.
transform_to
(
'geocentrictrueecliptic'
)
beta
=
abs
(
lb_obj
.
lat
.
degree
)
lamda
=
abs
(
lb_obj
.
lon
.
degree
-
lb_sun
.
lon
.
degree
)
# interpolated zodical surface brightness at 0.5 um
zodi
=
pd
.
read_csv
(
path
+
'MCI_inputData/refs/zodi_map.dat'
,
sep
=
'\s+'
,
header
=
None
,
comment
=
'#'
)
beta_angle
=
np
.
array
([
0
,
5
,
10
,
15
,
20
,
25
,
30
,
45
,
60
,
75
])
lamda_angle
=
np
.
array
([
0
,
5
,
10
,
15
,
20
,
25
,
30
,
35
,
40
,
45
,
60
,
75
,
90
,
105
,
120
,
135
,
150
,
165
,
180
])
xx
,
yy
=
np
.
meshgrid
(
beta_angle
,
lamda_angle
)
f
=
interpolate
.
interp2d
(
xx
,
yy
,
zodi
,
kind
=
'linear'
)
zodi_obj
=
f
(
beta
,
lamda
)
# 10^�? W m�? sr�? um�?
# read the zodical spectrum in the ecliptic
cat_spec
=
pd
.
read_csv
(
path
+
'MCI_inputData/refs/solar_spec.dat'
,
sep
=
'\s+'
,
header
=
None
,
comment
=
'#'
)
wave
=
cat_spec
[
0
].
values
# A
spec0
=
cat_spec
[
1
].
values
# 10^-8 W m^�? sr^�? μm^�?
zodi_norm
=
252
# 10^-8 W m^�? sr^�? μm^�?
spec
=
spec0
*
(
zodi_obj
/
zodi_norm
)
*
1e-8
# W m^�? sr^�? μm^�?
# convert to the commonly used unit of MJy/sr, erg/s/cm^2/A/sr
wave_A
=
wave
# A
#spec_mjy = spec * 0.1 * wave_A**2 / 3e18 * 1e23 * 1e-6 # MJy/sr
spec_erg
=
spec
*
0.1
# erg/s/cm^2/A/sr
spec_erg2
=
spec_erg
/
4.25452e10
# erg/s/cm^2/A/arcsec^2
return
wave_A
,
spec_erg2
###############################
# path='/home/yan/MCI/'
# wave0, zodi0=zodiacal(10.0, 20.0, '2024-04-04', path)
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