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Commit 663e096c authored by Zhang Xin's avatar Zhang Xin
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ImageHeader.py 0 → 100644
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chip_definition.json 0 → 100644
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extension_header.header 0 → 100644
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XTENSION= 'IMAGE ' / extension type BITPIX = 16 / bits per data value NAXIS = 2 / number of data axes NAXIS1 = 9216 / length of first array axis NAXIS2 = 9232 / length of second array axis PCOUNT = 0 GCOUNT = 1 EXTNAME = 'SCI ' EXTVER = 1 BSCALE = 1 BZERO = 32768 BUNIT = 'ADU ' / physical unit of array values COMMENT ================================================================== COMMENT Detector information COMMENT ================================================================== CAMERA = 'MS' / camera of main survey DETSN = '12345678' / detector serial number DETNAME = 'CCD' / detector type DETTEMP1= 173.0 / detector temperature at EXPSTART(in Kelvin) DETTEMP2= 173.0 / detector temperature at EXPEND(in Kelvin) DETTEMP3= 173.0 / detector temperature at READT1(in Kelvin) DETSIZE = '9560x9264' / detector size DATASECT= '9216x9232' / data section PIXSCAL1= 0.074 / pixel scale for axis 1 PIXSCAL2= 0.074 / pixel scale for axis 2 PIXSIZE1= 10 / pixel size for axis 1 (in um) PIXSIZE2= 10 / pixel size for axis 2 (in um) COMMENT ================================================================== COMMENT CCD chip information COMMENT ================================================================== CHIPID = '08' / chip ID CHIPLAB = 'y-1' / chip label FILTER = 'y' / filter name NCHAN = 16 / number of readout channels PSCAN1 = 27 / horizontal prescan width, per readout channel PSCAN2 = 8 / vertical prescan width, per readout channel OSCAN1 = 16 / horizontal overscan width,per readout channel OSCAN2 = 16 / vertical overscan width,per readout channel COMMENT ================================================================== COMMENT WORLD COORDINATE SYSTEM AND RELATED PARAMETERS COMMENT ================================================================== WCSAXES = 2 / number of World Coordinate System axes CRPIX1 = -10017.0 / x-coordinate of reference pixel CRPIX2 = 24876.0 / y-coordinate of reference pixel CRVAL1 = 62.228226 / first axis value at reference pixel CRVAL2 = -42.316932 / second axis value at reference pixel CTYPE1 = 'RA---TAN' / the coordinate type for the first axis CTYPE2 = 'DEC--TAN' / the coordinate type for the second axis CD1_1 = 1.88602083707394E-05 / partial of first axis coordinate w.r.t.x CD1_2 = 8.17455836176000E-06 / partial of first axis coordinate w.r.t.y CD2_1 = -8.1745583617600E-06 / partial of second axis coordinate w.r.t.x CD2_2 = 1.88602083707394E-05 / partial of second axis coordinate w.r.t.y OTHERS = '' / COMMENT ================================================================== COMMENT Readout information COMMENT ================================================================== GAINLVL = '01' / gain level GAIN01 = 1.1 / gain (channel 01) GAIN02 = 1.1 / gain (channel 02) GAIN03 = 1.1 / gain (channel 03) GAIN04 = 1.1 / gain (channel 04) GAIN05 = 1.1 / gain (channel 05) GAIN06 = 1.1 / gain (channel 06) GAIN07 = 1.1 / gain (channel 07) GAIN08 = 1.1 / gain (channel 08) GAIN09 = 1.1 / gain (channel 09) GAIN10 = 1.1 / gain (channel 10) GAIN11 = 1.1 / gain (channel 11) GAIN12 = 1.1 / gain (channel 12) GAIN13 = 1.1 / gain (channel 13) GAIN14 = 1.1 / gain (channel 14) GAIN15 = 1.1 / gain (channel 15) GAIN16 = 1.1 / gain (channel 16) RON01 = 5.0 / read noise (channel 01) RON02 = 5.0 / read noise (channel 02) RON03 = 5.0 / read noise (channel 03) RON04 = 5.0 / read noise (channel 04) RON05 = 5.0 / read noise (channel 05) RON06 = 5.0 / read noise (channel 06) RON07 = 5.0 / read noise (channel 07) RON08 = 5.0 / read noise (channel 08) RON09 = 5.0 / read noise (channel 09) RON10 = 5.0 / read noise (channel 10) RON11 = 5.0 / read noise (channel 11) RON12 = 5.0 / read noise (channel 12) RON13 = 5.0 / read noise (channel 13) RON14 = 5.0 / read noise (channel 14) RON15 = 5.0 / read noise (channel 15) RON16 = 5.0 / read noise (channel 16) READT0 = '2024-00-00T00:00:00'/ readout start time(UTC) READT1 = '2024-00-00T00:00:00'/ readout end time(UTC) ROSPEED = 10.0 / readout speed (in MHz) EXPTIME = 150.0 / exposure duration DARKTIME= 150.0 / dark current time COMMENT ================================================================== COMMENT Shutter information COMMENT ================================================================== SHTSTAT = T / shutter status SHTOPEN0= 0.0 / shutter open time (begin) SHTOPEN1= 0.0 / shutter open time (end) SHTCLOS0= 0.0 / shutter close time (begin) SHTCLOS1= 0.0 / shutter close time (end) COMMENT ================================================================== COMMENT LED information COMMENT ================================================================== LEDFLAG = 0 / main/backup LED LEDSTAT = '00000000000000' / LED status LEDEXPT = 0.0 / LED flash time (s) LEDTEMP = 173.0 / LED temperature (in K) COMMENT ================================================================== COMMENT Other information COMMENT ================================================================== CHECKSUM= '''abcde''' / HDU checksum updated yyyy-mm-ddTHH:MM:SS DATASUM = '''abcde''' / data unit checksum updated yyyy-mm-ddTHH:MM:SS END
filter.lst 0 → 100644
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GV GI y z y GI GU r u NUV i GV GU g NUV NUV g GU GV i NUV u r GU GI y z y GI GV
3 3 3 1 1 1 3 2 2 1 1 1 4 2 3 2 1 1 4 2 4 1 1 2 4 2 2 4 2 2
26 21 16 11 6 1 27 22 17 12 7 2 28 23 18 13 8 3 29 24 19 14 9 4 30 25 20 15 10 5
gen_calib_catalog.py 0 → 100644
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from cgitb import reset
from tkinter.tix import INTEGER
import astropy.coordinates as coord
from astropy import units as u
from pylab import *
import numpy as np
import galsim
import math
from astropy.table import Table, vstack
from astropy.io import fits
from astropy.wcs import WCS
import os
import json
import ImageHeader
# from numba import jit
ALL_FILTERS = ["NUV", "u", "g", "r", "i", "z", "y", "GU", "GV", "GI", "FGS"]
class Chip(object):
def __init__(self, chipID):
self.chipID = chipID
self.nchip_x = 6
self.nchip_y = 5
self.npix_tot_x = 59516
self.npix_tot_y = 49752
self.npix_gap_x = (534, 1309)
self.npix_gap_y = 898
self.cen_pix_x = 0
self.cen_pix_y = 0
self.npix_x = 9216
self.npix_y = 9232
self.pix_scale = 0.074
chip_dict = json.load(open("chip_definition.json", "r"))[str(self.chipID)]
for key in chip_dict:
setattr(self, key, chip_dict[key])
self.filter_id, self.filter_type = self.getChipFilter()
def getTanWCS(
self, ra, dec, img_rot, pix_scale=None, xcen=None, ycen=None, logger=None
):
"""Get the WCS of the image mosaic using Gnomonic/TAN projection
Parameter:
ra, dec: float
(RA, Dec) of pointing of optical axis
img_rot: galsim Angle object
Rotation of image
pix_scale: float
Pixel size in unit of as/pix
Returns:
WCS of the focal plane
"""
if logger is not None:
logger.info(
" Construct the wcs of the entire image mosaic using Gnomonic/TAN projection"
)
if (xcen == None) or (ycen == None):
xcen = self.cen_pix_x
ycen = self.cen_pix_y
if pix_scale == None:
pix_scale = self.pix_scale
# dudx = -np.cos(img_rot.rad) * pix_scale
# dudy = -np.sin(img_rot.rad) * pix_scale
# dvdx = -np.sin(img_rot.rad) * pix_scale
# dvdy = +np.cos(img_rot.rad) * pix_scale
dudx = -np.cos(img_rot.rad) * pix_scale
dudy = +np.sin(img_rot.rad) * pix_scale
dvdx = -np.sin(img_rot.rad) * pix_scale
dvdy = -np.cos(img_rot.rad) * pix_scale
moscen = galsim.PositionD(x=xcen, y=ycen)
sky_center = galsim.CelestialCoord(
ra=ra * galsim.degrees, dec=dec * galsim.degrees
)
affine = galsim.AffineTransform(dudx, dudy, dvdx, dvdy, origin=moscen)
WCS = galsim.TanWCS(affine, sky_center, units=galsim.arcsec)
return WCS
def getChipRowCol(self, chipID):
rowID = ((chipID - 1) % 5) + 1
colID = 6 - ((chipID - 1) // 5)
return rowID, colID
def getChipCenter(self):
"""Calculate the edges in pixel for a given CCD chip on the focal plane
NOTE: There are 5*4 CCD chips in the focus plane for photometric observation.
Parameters:
chipID: int
the index of the chip
Returns:
A galsim BoundsD object
"""
chipID = self.chipID
rowID, colID = self.getChipRowCol(chipID)
gx1, gx2 = self.npix_gap_x
gy = self.npix_gap_y
# xlim of a given CCD chip
xrem = 2 * (colID - 1) - (self.nchip_x - 1)
xcen = (self.npix_x // 2 + gx1 // 2) * xrem
if chipID >= 26 or chipID == 21:
xcen = (self.npix_x // 2 + gx1 // 2) * xrem - (gx2 - gx1)
if chipID <= 5 or chipID == 10:
xcen = (self.npix_x // 2 + gx1 // 2) * xrem + (gx2 - gx1)
# nx0 = xcen - self.npix_x//2 + 1
# nx1 = xcen + self.npix_x//2
# ylim of a given CCD chip
yrem = (rowID - 1) - self.nchip_y // 2
ycen = (self.npix_y + gy) * yrem
# ny0 = ycen - self.npix_y//2 + 1
# ny1 = ycen + self.npix_y//2
return galsim.PositionD(xcen, ycen)
def getChipFilter(self, chipID=None):
"""Return the filter index and type for a given chip #(chipID)"""
filter_type_list = ALL_FILTERS
if chipID == None:
chipID = self.chipID
# updated configurations
if chipID > 42 or chipID < 1:
raise ValueError("!!! Chip ID: [1,42]")
if chipID in [6, 15, 16, 25]:
filter_type = "y"
if chipID in [11, 20]:
filter_type = "z"
if chipID in [7, 24]:
filter_type = "i"
if chipID in [14, 17]:
filter_type = "u"
if chipID in [9, 22]:
filter_type = "r"
if chipID in [12, 13, 18, 19]:
filter_type = "NUV"
if chipID in [8, 23]:
filter_type = "g"
if chipID in [1, 10, 21, 30]:
filter_type = "GI"
if chipID in [2, 5, 26, 29]:
filter_type = "GV"
if chipID in [3, 4, 27, 28]:
filter_type = "GU"
if chipID in range(31, 43):
filter_type = "FGS"
filter_id = filter_type_list.index(filter_type)
return filter_id, filter_type
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 getobsPA(ra, dec):
l1 = np.array([0, 0, 1])
l2 = transRaDec2D(ra, dec)
polar_ec = coord.SkyCoord(
0 * u.degree, 90 * u.degree, frame="barycentrictrueecliptic"
)
polar_eq = polar_ec.transform_to("icrs")
# print(polar_eq.ra.value,polar_eq.dec.value)
polar_d = transRaDec2D(polar_eq.ra.value, polar_eq.dec.value)
l1l2cross = np.cross(l2, l1)
pdl2cross = np.cross(l2, polar_d)
angle = math.acos(
np.dot(l1l2cross, pdl2cross)
/ (np.linalg.norm(l1l2cross) * np.linalg.norm(pdl2cross))
)
angle = (angle) / math.pi * 180
# if (ra>90 and ra< 270):
# angle=-angle
return angle
def getChipRangeInfo(chipID=8, ra=60.0, dec=-40.0, pa=113.0):
"""_summary_
Args:
chipID (int, optional): Chip ID.
ra (_type_, optional): Chip center ra.
dec (_type_, optional): Chip center dec.
Returns:
_type_: [ra, dec, rotation angle]
"""
# chip_center = [ra, dec]
chip = Chip(chipID)
h_ext = ImageHeader.generateExtensionHeader(
chip=chip,
xlen=chip.npix_x,
ylen=chip.npix_y,
ra=ra,
dec=dec,
pa=pa,
gain=chip.gain,
readout=5.0,
dark=0.02,
saturation=90000,
pixel_scale=chip.pix_scale,
pixel_size=chip.pix_size,
xcen=chip.x_cen,
ycen=chip.y_cen,
extName="SCI",
timestamp=1621915200,
exptime=150,
readoutTime=chip.readout_time,
)
chip_wcs = WCS(h_ext)
return chip_wcs, chip.npix_x, chip.npix_y, chip.chipID, chip.filter_type
def formateSEDfile(inputDir, outputDir):
fileFns = os.listdir(inputDir)
for fn in fileFns:
if fn[0] == ".":
continue
if ".fits" not in fn:
continue
dfn = os.path.join(inputDir, fn)
outfn = os.path.join(outputDir, "GP_" + fn[0:-5] + ".fits")
f = fits.open(dfn)
data_tab = Table(f[1].data)
col_names = data_tab.colnames
if "loglam" in col_names:
print("1:" + fn)
w1 = pow(10, f[1].data["loglam"])
f1 = f[1].data["flux"] * 1e-17
elif "WAVELENGTH" in col_names:
print("2:" + fn)
w1 = np.array(data_tab["WAVELENGTH"].tolist()[0])
f1 = np.array(data_tab["FLUX"].tolist()[0]) * 1e-17
w = np.zeros(w1.shape[0] + 4)
w[0] = 2000
w[1] = w1[0] - 1
w[-2] = w1[-1] + 1
w[-1] = 15000
w[2:-2] = w1
fl = np.zeros(f1.shape[0] + 4)
fl[0] = 0
fl[1] = 0
fl[-2] = 0
fl[-1] = 0
fl[2:-2] = f1
t = Table([w, fl], names=["WAVELENGTH", "FLUX"])
# t = Table([pow(10,f[1].data['loglam']),f[1].data['flux']*1e-17],names=['WAVELENGTH','FLUX'])
t.write(outfn, overwrite=True)
def genOneChipCat(
ra=40.0,
dec=-40.0,
pa=23.5,
chipID=1,
pointSource_flag=True,
sersic_index=1.0,
re=0.078,
specFn="LMC-SMP-58_spectrum_csst.fits",
):
chip_wcs, chip_xlen, chip_ylen, _, filterT = getChipRangeInfo(
chipID=chipID, ra=ra, dec=dec, pa=pa
)
sppos = 3685
xSize = 15
ySize = 30
y_interval = 20
X2 = np.linspace(100, sppos - 100, xSize)
Y2 = np.linspace(100, chip_ylen - 300, ySize)
y_gap = np.arange(0, y_interval * xSize, y_interval)
x2, y2 = np.meshgrid(X2, Y2)
y2 = y2 + y_gap
x2 = x2.flatten()
y2 = y2.flatten()
X1 = np.linspace(sppos + 300, chip_xlen - 100, xSize)
Y1 = np.linspace(150, chip_ylen - 250, ySize)
y_gap = np.arange(0, y_interval * xSize, y_interval)
x1, y1 = np.meshgrid(X1, Y1)
y1 = y1 + y_gap
x1 = x1.flatten()
y1 = y1.flatten()
tab_size = x1.size + x2.size
x = np.zeros(tab_size)
y = np.zeros_like(x)
x[0 : x1.size] = x1
x[x1.size :] = x2
y[0 : x1.size] = y1
y[x1.size :] = y2
radecs = chip_wcs.pixel_to_world(x, y)
# ids = np.arange(0, tab_size, 1)
mags = np.zeros(tab_size) + -99
sns = np.zeros(tab_size) + sersic_index
res = np.zeros(tab_size) + re
namelist = []
ids = []
for i in np.arange(tab_size):
namelist.append(specFn)
ids.append(format(chipID, "02.0f") + format(i + 1, "04.0f"))
if pointSource_flag:
p_flag = np.ones(tab_size, dtype=bool) # True
else:
p_flag = np.zeros(tab_size, dtype=bool) # False
cat_t = Table(
[ids, radecs.ra.deg, radecs.dec.deg, res, sns, mags, namelist, p_flag],
names=(
"ID",
"RA",
"DEC",
"RE",
"SERSIC_N",
"MAG_g",
"SPEC_FN",
"POINTSOURCE_FLAG",
),
)
return cat_t
if __name__ == "__main__":
ra = 244.972773
dec = 39.895901
pa = 109.59452000342756
chipIDs = [1, 2, 3, 4, 5, 10, 21, 26, 27, 28, 29, 30]
cat_t = Table()
for chipID in chipIDs:
cat_one = genOneChipCat(
ra=ra,
dec=dec,
pa=pa,
chipID=chipID,
pointSource_flag=True,
specFn="LMC-SMP-58_spectrum_csst.fits",
)
cat_t = vstack([cat_t, cat_one])
cat_t.write(
"calibrationPNESPEC_CHIP_ALL_SLS.fits",
format="fits",
overwrite=True,
)
global_header.header 0 → 100644
View file @ 663e096c
SIMPLE = T / conforms to FITS standard BITPIX = 8 / array data type NAXIS = 0 / number of array dimensions EXTEND = T NEXTEND = 1 / number of array dimensions GROUPS = F / ' ' DATE = '2021-03-04T09:30:00'/ the date on which this file was written FILENAME= 'MSC_MS_210304093000_100000000_06_raw' / file name FILETYPE= 'SCIE ' / observation type TELESCOP= 'CSST ' / telescope used to acquire data INSTRUME= 'MSC ' / instrument used to acquire data RADECSYS= 'ICRS ' / reference coordinates system EQUINOX = 2000.0 / FITSCREA= 'C6' / FITS create software version COMMENT ================================================================== COMMENT Object information COMMENT ================================================================== OBJECT = '00000000' / object name TARGET = '+000000000000' / target name (hhmmss+ddmmss) OBSID = '00000000' / observation ID OBJ_RA = 62.228226 / R.A. of the object (degrees) OBJ_DEC = -42.316932 / declination of the object (degrees) COMMENT ================================================================== COMMENT Telescope information COMMENT ================================================================== REFFRAME= 'CSSTGSC-1.0' / guide star catalog version DATE-OBS= '2021-03-04T09:30:00'/ date of the observation (yyyy-mm-dd hh:mm:ss) SATESWV = '0001' / software version in the satellite EXPSTART= 59130.5 / exposure start time (MJD) CABSTART= 59130.5 / (MJD) SUNANGL0= 50.0 / angle between sun and opt axis at CABSTART MOONANG0= 30.0 / angle between moon and opt axis at CABSTART TEL_ALT0= 20.0 / angle between opt axis and Elimb at CABSTART POS_ANG0= 20.0 / angle between y axis and NP at CABSTART POSI0_X = 0.0 / the orbital position in X at CABSTART POSI0_Y = 0.0 / the orbital position in Y at CABSTART POSI0_Z = 0.0 / the orbital position in Z at CABSTART VELO0_X = 0.0 / the orbital velocity in X at CABSTART VELO0_Y = 0.0 / the orbital velocity in Y at CABSTART VELO0_Z = 0.0 / the orbital velocity in Z at CABSTART EULER0_1= 0.0 / euler angle 1 at CABSTART EULER0_2= 0.0 / euler angle 2 at CABSTART EULER0_3= 0.0 / euler angle 3 at CABSTART RA_PNT0 = 0.0 / RA of the pointing (degrees) at CABSTART DEC_PNT0= 0.0 / DEC of the pointing (degrees) at CABSTART EXPEND = 0.0 / exposure end time (MJD) CABEND = 0.0 / (MJD) SUNANGL1= 50.0 / angle between sun and opt axis at CABEND MOONANG1= 30.0 / angle between moon and opt axis at CABEND TEL_ALT1= 20.0 / angle between opt axis and Elimb at CABEND POS_ANG1= 20.0 / angle between y axis and NP at CABEND POSI1_X = 0.0 / the orbital position in X at CABEND POSI1_Y = 0.0 / the orbital position in Y at CABEND POSI1_Z = 0.0 / the orbital position in Z at CABEND VELO1_X = 0.0 / the orbital velocity in X at CABEND VELO1_Y = 0.0 / the orbital velocity in Y at CABEND VELO1_Z = 0.0 / the orbital velocity in Z at CABEND EULER1_1= 0.0 / euler angle 1 at CABEND EULER1_2= 0.0 / euler angle 2 at CABEND EULER1_3= 0.0 / euler angle 3 at CABEND RA_PNT1 = 0.0 / RA of the pointing (degrees) at CABEND DEC_PNT1= 0.0 / DEC of the pointing (degrees) at CABEND EXPTIME = 150.0 / exposure duration EPOCH = 2000.0 / coordinate epoch COMMENT Other information COMMENT ================================================================== CHECKSUM= 'abcdefg ' / HDU checksum updated yyyy-mm-ddTHH:MM:SS DATASUM = 'abcdefg ' / data unit checksum updated yyyy-mm-ddTHH:MM:SS END
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