Commit edd720e6 authored by Fang Yuedong's avatar Fang Yuedong
Browse files

Merge branch 'develop'

parents 959f0ebc 8df06b27
import numpy as np
import os
import shutil
import yaml
import galsim
import numpy as np
from astropy.time import Time
from ObservationSim.Config._util import get_obs_id
import ObservationSim.Instrument._util as _util
class Pointing(object):
def __init__(self, id=0, ra=0., dec=0., img_pa=0., timestamp=1621915200, sat_x=0., sat_y=0., sat_z=0., sun_x=0., sun_y=0., sun_z=0., sat_vx=0., sat_vy=0., sat_vz=0., exp_time=150., pointing_type='MS'):
def __init__(self, id=0, ra=0., dec=0., img_pa=0., timestamp=1621915200, sat_x=0., sat_y=0., sat_z=0., sun_x=0., sun_y=0., sun_z=0., sat_vx=0., sat_vy=0., sat_vz=0., exp_time=150., pointing_type='SCI', pointing_type_code='101', pointing_id = '00000001', obs_config_file=None, t_shutter_open = 1.3, t_shutter_close = 1.3):
self.id = id
self.ra = ra
self.dec = dec
......@@ -14,15 +20,58 @@ class Pointing(object):
self.sat_vx, self.sat_vy, self.sat_vz = sat_vx, sat_vy, sat_vz
self.exp_time = exp_time
self.pointing_type = pointing_type
self.jdt = 0.
self.pointing_type_code = pointing_type_code
self.obs_id = pointing_id
self.survey_field_type = 'WIDE'
self.jdt = 0.
self.obs_config_file = obs_config_file
self.t_shutter_open = t_shutter_open
self.t_shutter_close = t_shutter_close
self.output_dir = "."
if self.obs_config_file is not None:
with open(self.obs_config_file, "r") as stream:
try:
self.obs_param = yaml.safe_load(stream)
except yaml.YAMLError as exc:
print(exc)
if self.obs_param["obs_type"]:
self.pointing_type = self.obs_param["obs_type"]
if self.obs_param["obs_type_code"]:
self.pointing_type_code = self.obs_param["obs_type_code"]
if self.obs_param["obs_id"]:
self.obs_id = str(self.obs_param["obs_id"])
def get_full_depth_exptime(self, filter_type):
if self.survey_field_type == 'WIDE':
if filter_type in _util.SPEC_FILTERS:
return 150. * 4
else:
if filter_type.lower() in ['nuv', 'y']:
return 150. * 4
elif filter_type.lower() in ['u', 'g', 'r', 'i', 'z']:
return 150. * 2
else:
return max(150., self.exp_time) # [TODO] for FGS
elif self.survey_field_type == 'DEEP':
if filter_type in _util.SPEC_FILTERS:
return 250. * 4 * 4
else:
if filter_type.lower() in ['nuv', 'y']:
return 250. * 4 * 4
elif filter_type.lower() in ['u', 'g', 'r', 'i', 'z']:
return 250. * 2 * 4
else:
return max(150., self.exp_time) # [TODO] for FGS
def read_pointing_columns(self, columns, id=0, t=1621915200, pointing_type='MS'):
def read_pointing_columns(self, columns, id=0, t=1621915200, pointing_type='SCI'):
self.id = id
col_len = len(columns)
self.ra = float(columns[0])
self.dec = float(columns[1])
self.img_pa = float(columns[4]) * galsim.degrees
self.pointing_type = pointing_type
# self.pointing_type = pointing_type
if col_len > 5:
jdt = np.double(columns[5])
t_temp = Time(jdt, format='jd')
......@@ -33,10 +82,55 @@ class Pointing(object):
self.sat_z = float(columns[8])
self.sun_x = float(columns[9])
self.sun_y = float(columns[10])
self.sun_z = float(columns[1])
self.sun_z = float(columns[11])
self.sat_vx = float(columns[15])
self.sat_vy = float(columns[16])
self.sat_vz = float(columns[17])
self.exp_time = float(columns[18])
is_deep = float(columns[19])
# [TODO] Can also define other survey types
if is_deep != -1.0:
self.survey_field_type = "DEEP"
if not self.obs_config_file:
self.obs_config_file = str(columns[20])
with open(self.obs_config_file, "r") as stream:
try:
self.obs_param = yaml.safe_load(stream)
except yaml.YAMLError as exc:
print(exc)
self.pointing_type_code = columns[21][0:3]
self.obs_id = columns[21][3:]
self.pointing_type = self.obs_param["obs_type"]
else:
self.timestamp = t
def make_output_pointing_dir(self, overall_config, copy_obs_config=False):
run_dir = os.path.join(overall_config["work_dir"], overall_config["run_name"])
if not os.path.exists(run_dir):
try:
os.makedirs(run_dir, exist_ok=True)
except OSError:
pass
self.output_prefix = get_obs_id(
img_type=self.pointing_type,
project_cycle=overall_config["project_cycle"],
run_counter=overall_config["run_counter"],
pointing_id=self.obs_id,
pointing_type_code = self.pointing_type_code)
self.output_dir = os.path.join(run_dir, self.output_prefix)
if not os.path.exists(self.output_dir):
try:
os.makedirs(self.output_dir, exist_ok=True)
except OSError:
pass
if copy_obs_config and self.obs_config_file:
obs_config_output_path = os.path.join(self.output_dir, os.path.basename(self.obs_config_file))
if not os.path.exists(obs_config_output_path):
try:
shutil.copy(self.obs_config_file, self.output_dir)
except OSError:
pass
from .Config import *
from .ChipOutput import ChipOutput
from .Pointing import Pointing
\ No newline at end of file
def get_obs_id(img_type='SCI', project_cycle=6, run_counter=0, pointing_id='00000001',pointing_type_code='101'):
# obs_type = {'SCI': '01', 'BIAS': '03', 'DARK': '07', 'FLAT': '11', 'CRS': '98', 'CRD': '99'}
# obs_type = {'SCIE': '01', 'BIAS': '03', 'DARK': '07', 'FLAT': '11', 'CRS': '98', 'CRD': '99', 'CAL': '01'}
obs_id = pointing_type_code + str(int(project_cycle)).rjust(2, '0') + str(int(run_counter)) + pointing_id
return obs_id
# def get_obs_id(img_type='SCI', project_cycle=6, run_counter=0, pointing_num=0):
# # obs_type = {'SCI': '01', 'BIAS': '03', 'DARK': '07', 'FLAT': '11', 'CRS': '98', 'CRD': '99'}
# obs_type = {'SCIE': '01', 'BIAS': '03', 'DARK': '07', 'FLAT': '11', 'CRS': '98', 'CRD': '99', 'CAL': '01'}
# obs_id = '1'+ obs_type[img_type] + str(int(project_cycle)).rjust(2, '0') + str(int(run_counter)) + str(pointing_num).rjust(8,'0')
# return obs_id
def get_file_type(img_type='SCI'):
file_type = {'SCI':'SCI', 'BIAS':'BIAS', 'DARK':'DARK', 'FLAT':'FLAT', 'CRS':'CRS', 'CRD':'CRD','CALS':'CALS','CALF':'CALF'}
return file_type[img_type]
\ No newline at end of file
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import os
import galsim
import ctypes
import numpy as np
from astropy.io import fits
from datetime import datetime
from ObservationSim.Instrument.Chip import Effects as effects
from ObservationSim.Config.Header import generatePrimaryHeader, generateExtensionHeader
try:
import importlib.resources as pkg_resources
except ImportError:
# Try backported to PY<37 'importlib_resources'
import importlib_resources as pkg_resources
def log_info(msg, logger=None):
if logger:
logger.info(msg)
else:
print(msg, flush=True)
def getChipSLSGratingID(chipID):
gratingID = ['','']
if chipID == 1: gratingID = ['GI2', 'GI1']
if chipID == 2: gratingID = ['GV4', 'GV3']
if chipID == 3: gratingID = ['GU2', 'GU1']
if chipID == 4: gratingID = ['GU4', 'GU3']
if chipID == 5: gratingID = ['GV2', 'GV1']
if chipID == 10: gratingID = ['GI4', 'GI3']
if chipID == 21: gratingID = ['GI6', 'GI5']
if chipID == 26: gratingID = ['GV8', 'GV7']
if chipID == 27: gratingID = ['GU6', 'GU5']
if chipID == 28: gratingID = ['GU8', 'GU7']
if chipID == 29: gratingID = ['GV6', 'GV5']
if chipID == 30: gratingID = ['GI8', 'GI7']
return gratingID
def getChipSLSConf(chipID):
confFile = ''
if chipID == 1: confFile = ['CSST_GI2.conf', 'CSST_GI1.conf']
if chipID == 2: confFile = ['CSST_GV4.conf', 'CSST_GV3.conf']
if chipID == 3: confFile = ['CSST_GU2.conf', 'CSST_GU1.conf']
if chipID == 4: confFile = ['CSST_GU4.conf', 'CSST_GU3.conf']
if chipID == 5: confFile = ['CSST_GV2.conf', 'CSST_GV1.conf']
if chipID == 10: confFile = ['CSST_GI4.conf', 'CSST_GI3.conf']
if chipID == 21: confFile = ['CSST_GI6.conf', 'CSST_GI5.conf']
if chipID == 26: confFile = ['CSST_GV8.conf', 'CSST_GV7.conf']
if chipID == 27: confFile = ['CSST_GU6.conf', 'CSST_GU5.conf']
if chipID == 28: confFile = ['CSST_GU8.conf', 'CSST_GU7.conf']
if chipID == 29: confFile = ['CSST_GV6.conf', 'CSST_GV5.conf']
if chipID == 30: confFile = ['CSST_GI8.conf', 'CSST_GI7.conf']
return confFile
def generateHeader(chip, pointing, img_type=None, img_type_code=None, project_cycle='9', run_counter='1'):
if (img_type is None) or (img_type_code is None):
img_type = pointing.pointing_type
img_type_code = pointing.pointing_type_code
h_prim = generatePrimaryHeader(
xlen=chip.npix_x,
ylen=chip.npix_y,
pointing_id = pointing.obs_id,
pointing_type_code = img_type_code,
ra=pointing.ra,
dec=pointing.dec,
pixel_scale=chip.pix_scale,
time_pt = pointing.timestamp,
exptime=pointing.exp_time,
im_type=img_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=project_cycle,
run_counter=run_counter,
chip_name=str(chip.chipID).rjust(2, '0'))
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=img_type,
timestamp=pointing.timestamp,
exptime=pointing.exp_time,
readoutTime=chip.readout_time,
t_shutter_open=pointing.t_shutter_open,
t_shutter_close=pointing.t_shutter_close)
return h_prim, h_ext
def output_fits_image(chip, pointing, img, output_dir, img_type=None, img_type_code=None, project_cycle='9', run_counter='1'):
h_prim, h_ext = generateHeader(
chip=chip,
pointing=pointing,
img_type=img_type,
img_type_code=img_type_code,
project_cycle=project_cycle,
run_counter=run_counter)
hdu1 = fits.PrimaryHDU(header=h_prim)
hdu1.add_checksum()
hdu1.header.comments['CHECKSUM'] = 'HDU checksum'
hdu1.header.comments['DATASUM'] = 'data unit checksum'
hdu2 = fits.ImageHDU(img.array, header=h_ext)
hdu2.add_checksum()
hdu2.header.comments['XTENSION'] = 'extension type'
hdu2.header.comments['CHECKSUM'] = 'HDU checksum'
hdu2.header.comments['DATASUM'] = 'data unit checksum'
hdu1 = fits.HDUList([hdu1, hdu2])
fname = os.path.join(output_dir, h_prim['FILENAME']+'.fits')
hdu1.writeto(fname, output_verify='ignore', overwrite=True)
def add_sky_background(img, filt, exptime, sky_map=None, tel=None):
# Add sky background
if sky_map is None:
sky_map = filt.getSkyNoise(exptime=exptime)
sky_map = sky_map * np.ones_like(img.array)
sky_map = galsim.Image(array=sky_map)
# Apply Poisson noise to the sky map
# # (NOTE): only for photometric chips if it utilizes the photon shooting to draw stamps
# if self.survey_type == "photometric":
# sky_map.addNoise(poisson_noise)
elif img.array.shape != sky_map.shape:
raise ValueError("The shape img and sky_map must be equal.")
elif tel is not None: # If sky_map is given in flux
sky_map = sky_map * tel.pupil_area * exptime
img += sky_map
return img, sky_map
def get_flat(img, seed):
flat_img = effects.MakeFlatSmooth(
GSBounds=img.bounds,
seed=seed)
flat_normal = flat_img / np.mean(flat_img.array)
return flat_img, flat_normal
def add_cosmic_rays(img, chip, exptime=150, seed=0):
cr_map, cr_event_num = effects.produceCR_Map(
xLen=chip.npix_x, yLen=chip.npix_y,
exTime=exptime+0.5*chip.readout_time,
cr_pixelRatio=0.003*(exptime+0.5*chip.readout_time)/600.,
gain=chip.gain,
attachedSizes=chip.attachedSizes,
seed=seed) # seed: obj-imaging:+0; bias:+1; dark:+2; flat:+3;
img += cr_map
cr_map[cr_map > 65535] = 65535
cr_map[cr_map < 0] = 0
crmap_gsimg = galsim.Image(cr_map, dtype=np.uint16)
del cr_map
return img, crmap_gsimg, cr_event_num
def add_PRNU(img, chip, seed=0):
prnu_img = effects.PRNU_Img(
xsize=chip.npix_x,
ysize=chip.npix_y,
sigma=0.01,
seed=seed)
img *= prnu_img
return img, prnu_img
def get_poisson(seed=0, sky_level=0.):
rng_poisson = galsim.BaseDeviate(seed)
poisson_noise = galsim.PoissonNoise(rng_poisson, sky_level=sky_level)
return rng_poisson, poisson_noise
def get_base_img(img, chip, read_noise, readout_time, dark_noise, exptime=150., InputDark=None):
if InputDark == None:
# base_level = read_noise**2 + dark_noise*(exptime+0.5*readout_time)
## base_level = dark_noise*(exptime+0.5*readout_time)
base_level = dark_noise*(exptime)
base_img1 = base_level * np.ones_like(img.array)
else:
base_img1 = np.zeros_like(img.array)
ny = int(chip.npix_y/2)
nx = chip.npix_x
arr = np.arange(ny).reshape(ny, 1)
arr = np.broadcast_to(arr, (ny, nx))
base_img2 = np.zeros_like(img.array)
base_img2[:ny, :] = arr
base_img2[ny:, :] = arr[::-1,:]
base_img2[:,:] = base_img2[:,:]*(readout_time/ny)*dark_noise
return base_img1+base_img2
def add_poisson(img, chip, exptime=150., seed=0, sky_level=0., poisson_noise=None, dark_noise=None, InputDark=None):
if poisson_noise is None:
_, poisson_noise = get_poisson(seed=seed, sky_level=sky_level)
read_noise = chip.read_noise
if dark_noise is None:
dark_noise = chip.dark_noise
base_img = get_base_img(img=img, chip=chip, read_noise=read_noise, readout_time=chip.readout_time, dark_noise=dark_noise, exptime=exptime, InputDark=InputDark)
img += base_img
img.addNoise(poisson_noise)
# img -= read_noise**2
if InputDark != None:
hdu = fits.open(InputDark) ##"Instrument/data/dark/dark_1000s_example_0.fits"
img += hdu[0].data/hdu[0].header['exptime']*exptime
hdu.close()
return img, base_img
def add_brighter_fatter(img):
#Inital dynamic lib
try:
with pkg_resources.files('ObservationSim.Instrument.Chip.libBF').joinpath("libmoduleBF.so") as lib_path:
lib_bf = ctypes.CDLL(lib_path)
except AttributeError:
with pkg_resources.path('ObservationSim.Instrument.Chip.libBF', "libmoduleBF.so") as lib_path:
lib_bf = ctypes.CDLL(lib_path)
lib_bf.addEffects.argtypes = [ctypes.c_int, ctypes.c_int, ctypes.POINTER(ctypes.c_float), ctypes.POINTER(ctypes.c_float), ctypes.c_int]
# Set bit flag
bit_flag = 1
bit_flag = bit_flag | (1 << 2)
nx, ny = img.array.shape
nn = nx * ny
arr_ima= (ctypes.c_float*nn)()
arr_imc= (ctypes.c_float*nn)()
arr_ima[:]= img.array.reshape(nn)
arr_imc[:]= np.zeros(nn)
lib_bf.addEffects(nx, ny, arr_ima, arr_imc, bit_flag)
img.array[:, :] = np.reshape(arr_imc, [nx, ny])
del arr_ima, arr_imc
return img
"""
def add_inputdark(img, chip, exptime):
fname = "/share/home/weichengliang/CSST_git/test_new_sim/csst-simulation/ObservationSim/Instrument/data/dark/dark_1000s_example_0.fits"
hdu = fits.open(fname)
#ny, nx = img.array.shape
#inputdark = np.zeros([ny, nx])
img.array[:, :] += hdu[0].data/hdu[0].header['exptime']*exptime
hdu.close()
del inputdark
return img
"""
def AddPreScan(GSImage, pre1=27, pre2=4, over1=71, over2=80, nsecy = 2, nsecx=8):
img= GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
imgt=np.zeros([int(nsecy*nsecx), int(ny/nsecy+pre2+over2), int(nx/nsecx+pre1+over1)])
for iy in range(nsecy):
for ix in range(nsecx):
if iy % 2 == 0:
tx = ix
else:
tx = (nsecx-1)-ix
ty = iy
chunkidx = int(tx+ty*nsecx) #chunk1-[1,2,3,4], chunk2-[5,6,7,8], chunk3-[9,10,11,12], chunk4-[13,14,15,16]
imgtemp = np.zeros([int(ny/nsecy+pre2+over2), int(nx/nsecx+pre1+over1)])
if int(chunkidx/4) == 0:
imgtemp[pre2:pre2+dy, pre1:pre1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp
if int(chunkidx/4) == 1:
imgtemp[pre2:pre2+dy, over1:over1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[:, ::-1]
if int(chunkidx/4) == 2:
imgtemp[over2:over2+dy, over1:over1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[::-1, ::-1]
if int(chunkidx/4) == 3:
imgtemp[over2:over2+dy, pre1:pre1+dx] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgt[chunkidx, :, :] = imgtemp #[::-1, :]
imgtx1 = np.hstack(imgt[:nsecx:, :, :]) #hstack chunk(1,2)-[1,2,3,4,5,6,7,8]
imgtx2 = np.hstack(imgt[:(nsecx-1):-1, :, :]) #hstack chunk(4,3)-[16,15,14,13,12,11,,10,9]
newimg = galsim.Image(int(nx+(pre1+over1)*nsecx), int(ny+(pre2+over2)*nsecy), init_value=0)
newimg.array[:, :] = np.concatenate([imgtx1, imgtx2]) #vstack chunk(1,2) & chunk(4,3)
newimg.wcs = GSImage.wcs
return newimg
def AddPreScanFO(GSImage, pre1=27, pre2=4, over1=71, over2=80, nsecy = 1, nsecx=16):
img= GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
newimg = galsim.Image(int(nx+(pre1+over1)*nsecx), int(ny+(pre2+over2)*nsecy), init_value=0)
for ix in range(nsecx):
newimg.array[pre2:pre2+dy, pre1+ix*(dx+pre1+over1):pre1+dx+ix*(dx+pre1+over1)] = img[0:dy, 0+ix*dx:dx+ix*dx]
newimg.wcs = GSImage.wcs
return newimg
def formatOutput(GSImage, nsecy = 2, nsecx=8):
img = GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
imgt = np.zeros([int(nsecx*nsecy), dy, dx])
for iy in range(nsecy):
for ix in range(nsecx):
if iy % 2 == 0:
tx = ix
else:
tx = (nsecx-1)-ix
ty = iy
chunkidx = int(tx+ty*nsecx)
if int(chunkidx/4) == 0:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 1:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 2:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
if int(chunkidx/4) == 3:
imgt[chunkidx, :, :] = img[iy*dy:(iy+1)*dy, ix*dx:(ix+1)*dx]
imgttx0 = np.hstack(imgt[ 0:4:, :, :])
imgttx1 = np.hstack(imgt[ 4:8:, :, ::-1])
imgttx2 = np.hstack(imgt[8:12:, ::-1, ::-1])
imgttx3 = np.hstack(imgt[12:16:,::-1, :])
newimg = galsim.Image(int(dx*nsecx*nsecy), dy, init_value=0)
newimg.array[:, :] = np.hstack([imgttx0, imgttx1, imgttx2, imgttx3])
return newimg
def formatRevert(GSImage, nsecy = 1, nsecx=16):
img = GSImage.array
ny, nx = img.shape
dx = int(nx/nsecx)
dy = int(ny/nsecy)
newimg = galsim.Image(int(dx*8), int(dy*2), init_value=0)
for ix in range(0,4):
tx = ix
newimg.array[0:dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx]
for ix in range(4,8):
tx = ix
newimg.array[0:dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][:, ::-1]
for ix in range(8,12):
tx = 7-(ix-8)
newimg.array[0+dy:dy+dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][::-1, ::-1]
for ix in range(12,16):
tx = 7-(ix-8)
newimg.array[0+dy:dy+dy, 0+tx*dx:dx+tx*dx] = img[:, 0+ix*dx:dx+ix*dx][::-1, :]
return newimg
#include <math.h>
#include <stdio.h>
#include <stdlib.h>
#include <string.h>
#include "nrutil.h"
#define ISSETBITFLAG(x,b) ((x) & (1 << (b)))
#define ADD_DIFFUSION 1
#define ADD_BF_FILTER 2
float linearInterp(float xp, float x0, float y0, float x1, float y1);
void addEffects(int ngx_ima, int ngy_ima, float *arr_ima, float *arr_imc, int bit_flag)
{
int nx, ny, i,j,k,ks;
int it,jt,itt,jtt;
int diffuidx[26][2],diffuN,ilow,ih,im,dim[3];
float diffua[5][5],cdiffu[26],**bfa;
double mvar,mcov,tmp,ma,mb,mc;
char fname[100];
nx = ngx_ima; //input-image size
ny = ngy_ima;
//0. init. original image with an input array (arr_ima)
//1. Adding diffusion effect.
if(ISSETBITFLAG(bit_flag, ADD_DIFFUSION))
{
printf("adding diffusion.....\n");
printf("ERR: no diffusion filter ...");
exit(0);
}
//2. Adding BF effect
if(ISSETBITFLAG(bit_flag, ADD_BF_FILTER))
{
printf("Adding BF effect...\n");
//setup BF correlation fliter
float neX;
float neP1 = 50000;
float bfaP1[9]={0.9707182, 0.002143905, 0.004131103, 0.001149542, 0.0005501739, 0.0005469659, 0.0003726081, 0.0003795207, 0.0001633302};
float neP2 = 10000;
float bfaP2[9]={0.9945288, 0.0003041936, 0.0007539311, 0.0002424675, 0.0001226098, 0.00009308617, 0.00008027447, 0.00006309676, 0.00006400052};
bfa=matrix(-2,2,-2,2);
// smooth with the BF filter
for(i=0;i<nx;i++)for(j=0;j<ny;j++) arr_imc[j+i*ny]=0;
for(i=0;i<nx;i++)
{
for(j=0;j<ny;j++)
{
//rescale BF filter with the local pix value
neX = arr_ima[j+i*ny];
if(neX >= 10000)
{
bfa[0][0]=0; //linearInterp(neX, neP1, bfaP1[0], neP2, bfaP2[0]); //0;
bfa[0][1]=bfa[0][-1]=linearInterp(neX, neP1, bfaP1[1], neP2, bfaP2[1]); //0.01575;
bfa[-1][0]=bfa[1][0]=linearInterp(neX, neP1, bfaP1[2], neP2, bfaP2[2]); //0.00652;
bfa[-1][-1]=bfa[1][1]=bfa[-1][1]=bfa[1][-1]=linearInterp(neX, neP1, bfaP1[3], neP2, bfaP2[3]); //0.00335;
bfa[0][-2]=bfa[0][2]=linearInterp(neX, neP1, bfaP1[4], neP2, bfaP2[4]);
bfa[-2][0]=bfa[2][0]=linearInterp(neX, neP1, bfaP1[5], neP2, bfaP2[5]); //0.00118;
bfa[-2][-1]=bfa[-2][1]=bfa[2][1]=bfa[2][-1]=linearInterp(neX, neP1, bfaP1[6], neP2, bfaP2[6]);
bfa[-1][-2]=bfa[1][2]=bfa[-1][2]=bfa[1][-2]=linearInterp(neX, neP1, bfaP1[7], neP2, bfaP2[7]); //0.00083;
bfa[-2][-2]=bfa[-2][2]=bfa[2][-2]=bfa[2][2]=linearInterp(neX, neP1, bfaP1[8], neP2, bfaP2[8]); //0.00043;
}
else
{
neX=10000;
bfa[0][0]=0;
bfa[0][1]=bfa[0][-1]=bfaP2[1];
bfa[-1][0]=bfa[1][0]=bfaP2[2];
bfa[-1][-1]=bfa[1][1]=bfa[-1][1]=bfa[1][-1]=bfaP2[3];
bfa[0][-2]=bfa[0][2]=bfaP2[4];
bfa[-2][0]=bfa[2][0]=bfaP2[5];
bfa[-2][-1]=bfa[-2][1]=bfa[2][1]=bfa[2][-1]=bfaP2[6];
bfa[-1][-2]=bfa[1][2]=bfa[-1][2]=bfa[1][-2]=bfaP2[7];
bfa[-2][-2]=bfa[-2][2]=bfa[2][-2]=bfa[2][2]=bfaP2[8];
}
tmp = 0;
for(it=-2;it<=2;it++)
for(jt=-2;jt<=2;jt++)
{
bfa[it][jt] = bfa[it][jt]/neX*arr_ima[j+i*ny];
tmp += bfa[it][jt];
}
bfa[0][0]=1.-tmp;
// assign electrons according to the BF filter bfat
for(it=-2;it<=2;it++)
{
for(jt=-2;jt<=2;jt++)
{
itt=i+it;
jtt=j+jt;
if(itt>=0 && jtt>=0 && itt<nx && jtt<ny)
//c0[itt][jtt]+=bfa[it][jt]*b[i][j];
arr_imc[jtt+itt*ny] += bfa[it][jt]*arr_ima[j+i*ny];
}
}
}
}
free_matrix(bfa,-2,2,-2,2);
}
else
{
for(i=0;i<nx;i++) for(j=0;j<ny;j++) arr_imc[j+i*ny]=arr_ima[j+i*ny]; ////for ADD_BF False
}
}
float linearInterp(float xp, float x0, float y0, float x1, float y1)
{
float yp;
yp = y0 + ((y1-y0)/(x1-x0)) * (xp - x0);
return yp;
}
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/* CAUTION: This is the ANSI C (only) version of the Numerical Recipes
utility file nrutil.h. Do not confuse this file with the same-named
file nrutil.h that may be supplied in a 'misc' subdirectory.
*That* file is the one from the book, and contains both ANSI and
traditional K&R versions, along with #ifdef macros to select the
correct version. *This* file contains only ANSI C. */
#ifndef _NR_UTILS_H_
#define _NR_UTILS_H_
static float sqrarg;
#define SQR(a) ((sqrarg=(a)) == 0.0 ? 0.0 : sqrarg*sqrarg)
static double dsqrarg;
#define DSQR(a) ((dsqrarg=(a)) == 0.0 ? 0.0 : dsqrarg*dsqrarg)
static double dmaxarg1,dmaxarg2;
#define DMAX(a,b) (dmaxarg1=(a),dmaxarg2=(b),(dmaxarg1) > (dmaxarg2) ?\
(dmaxarg1) : (dmaxarg2))
static double dminarg1,dminarg2;
#define DMIN(a,b) (dminarg1=(a),dminarg2=(b),(dminarg1) < (dminarg2) ?\
(dminarg1) : (dminarg2))
static float maxarg1,maxarg2;
#define FMAX(a,b) (maxarg1=(a),maxarg2=(b),(maxarg1) > (maxarg2) ?\
(maxarg1) : (maxarg2))
static float minarg1,minarg2;
#define FMIN(a,b) (minarg1=(a),minarg2=(b),(minarg1) < (minarg2) ?\
(minarg1) : (minarg2))
static long lmaxarg1,lmaxarg2;
#define LMAX(a,b) (lmaxarg1=(a),lmaxarg2=(b),(lmaxarg1) > (lmaxarg2) ?\
(lmaxarg1) : (lmaxarg2))
static long lminarg1,lminarg2;
#define LMIN(a,b) (lminarg1=(a),lminarg2=(b),(lminarg1) < (lminarg2) ?\
(lminarg1) : (lminarg2))
static int imaxarg1,imaxarg2;
#define IMAX(a,b) (imaxarg1=(a),imaxarg2=(b),(imaxarg1) > (imaxarg2) ?\
(imaxarg1) : (imaxarg2))
static int iminarg1,iminarg2;
#define IMIN(a,b) (iminarg1=(a),iminarg2=(b),(iminarg1) < (iminarg2) ?\
(iminarg1) : (iminarg2))
#define SIGN(a,b) ((b) >= 0.0 ? fabs(a) : -fabs(a))
void nrerror(char error_text[]);
float *vector(long nl, long nh);
int *ivector(long nl, long nh);
unsigned char *cvector(long nl, long nh);
long *lvector(long nl, long nh);
double *dvector(long nl, long nh);
float **matrix(long nrl, long nrh, long ncl, long nch);
double **dmatrix(long nrl, long nrh, long ncl, long nch);
int **imatrix(long nrl, long nrh, long ncl, long nch);
float **submatrix(float **a, long oldrl, long oldrh, long oldcl, long oldch,
long newrl, long newcl);
float **convert_matrix(float *a, long nrl, long nrh, long ncl, long nch);
float ***f3tensor(long nrl, long nrh, long ncl, long nch, long ndl, long ndh);
void free_vector(float *v, long nl, long nh);
void free_ivector(int *v, long nl, long nh);
void free_cvector(unsigned char *v, long nl, long nh);
void free_lvector(long *v, long nl, long nh);
void free_dvector(double *v, long nl, long nh);
void free_matrix(float **m, long nrl, long nrh, long ncl, long nch);
void free_dmatrix(double **m, long nrl, long nrh, long ncl, long nch);
void free_imatrix(int **m, long nrl, long nrh, long ncl, long nch);
void free_submatrix(float **b, long nrl, long nrh, long ncl, long nch);
void free_convert_matrix(float **b, long nrl, long nrh, long ncl, long nch);
void free_f3tensor(float ***t, long nrl, long nrh, long ncl, long nch,
long ndl, long ndh);
int ***i3tensor(long nrl, long nrh, long ncl, long nch, long ndl, long ndh);
void free_i3tensor(int ***t, long nrl, long nrh, long ncl, long nch,
long ndl, long ndh);
unsigned char ***b3tensor(long nrl, long nrh, long ncl, long nch, long ndl, long ndh);
void free_b3tensor(unsigned char ***t, long nrl, long nrh, long ncl, long nch,
long ndl, long ndh);
double ***d3tensor(long nrl, long nrh, long ncl, long nch, long ndl, long ndh);
void free_d3tensor(double ***t, long nrl, long nrh, long ncl, long nch,
long ndl, long ndh);
char **cmatrix(long nrl, long nrh, long ncl, long nch);
void free_cmatrix(char **m, long nrl, long nrh, long ncl, long nch);
#endif /* _NR_UTILS_H_ */
from ctypes import CDLL, POINTER, c_int, c_double,c_float,c_long,c_char_p
from numpy.ctypeslib import ndpointer
import numpy.ctypeslib as clb
import numpy as np
from astropy.io import fits
from scipy.stats import randint
from glob import glob
from datetime import datetime
import os
lib_path = os.path.dirname(os.path.realpath(__file__))
#lib_path += "/add_CTI.so"
lib_path += "/libmoduleCTI.so"
lib = CDLL(lib_path)
CTI_simul = lib.__getattr__('CTI_simul')
CTI_simul.argtypes = [POINTER(POINTER(c_int)),c_int,c_int,c_int,c_int,POINTER(c_float),POINTER(c_float),\
c_float,c_float,c_float,c_int,POINTER(c_int),c_int,POINTER(POINTER(c_int))]
'''
get_trap_h = lib.__getattr__('save_trap_map')
get_trap_h.argtypes = [POINTER(c_int), c_int, c_int, c_int, c_int, POINTER(c_float), c_float, c_float, c_char_p]
def get_trap_map(seeds,nx,ny,nmax,rho_trap,beta,c,out_dir):
hsp_result = np.zeros(ny*nx*nmax)
nsp = len(rho_trap)
seeds1 = seeds.astype(np.int32)
seeds_p = np.ctypeslib.as_ctypes(seeds1)
rho_trap1 = rho_trap.astype(np.float32)
rho_trap_p = np.ctypeslib.as_ctypes(rho_trap1)
filename = (out_dir+"/trap.bin").encode('utf-8')
get_trap_h(seeds_p,c_int(int(nsp)),c_int(int(nx)),c_int(int(ny)),\
c_int(int(nmax)),rho_trap_p,c_float(beta),\
c_float(c),filename)
def bin2fits(bin_file,fits_dir,nsp,nx,ny,nmax):
data = np.fromfile(bin_file,dtype=np.float32)
data = data.reshape(nx,nsp,ny,nmax).transpose(1,3,2,0)
for i in range(nsp):
print("transfering trap type "+str(i+1))
datai = data[i]
ntrap = datai[0,:,:]
for j in range(nmax-1):
h = datai[j+1,:,:]
h[np.where(ntrap<j+1)] = 0
datai[j+1,:,:] = h
fits.writeto(fits_dir+"/trap_"+str(i+1)+".fits",datai,overwrite=True)
'''
def numpy_matrix_to_int_pointer(arr):
int_pointer_array = (POINTER(c_int)*arr.shape[0])()
for i in range(arr.shape[0]):
arr1 = np.array(arr[i].copy().tolist(),dtype=np.int32)
int_pointer_array[i] = np.ctypeslib.as_ctypes(arr1)
return int_pointer_array
def pointer_to_numpy_matrix(arr_pointer,row,col):
arr = np.zeros((row,col))
for i in range(row):
for j in range(col):
arr[i,j] = arr_pointer[i][j]
return arr
def CTI_sim(im,nx,ny,noverscan,nsp,nmax,beta,w,c,t,rho_trap,trap_seeds,release_seed=0):
image = im.T
nx_c,ny_c,noverscan_c,nsp_c,nmax_c = c_int(nx),c_int(ny),c_int(noverscan),c_int(nsp),c_int(nmax)
ntotal = ny+noverscan
beta_c,w_c,c_c = c_float(beta),c_float(w),c_float(c)
t_p = np.ctypeslib.as_ctypes(t)
rho_trap_p = np.ctypeslib.as_ctypes(rho_trap)
image_p = numpy_matrix_to_int_pointer(image)
trap_seeds1 = trap_seeds.astype(np.int32)
trap_seeds_p = np.ctypeslib.as_ctypes(trap_seeds1)
release_seed_c = c_int(release_seed)
image_cti = np.zeros((nx,ntotal))
image_cti = image_cti.astype(np.int32)
image_cti_p = numpy_matrix_to_int_pointer(image_cti)
print(datetime.now())
CTI_simul(image_p,nx,ny,noverscan,nsp,rho_trap_p,t_p,beta,w,c,nmax,trap_seeds_p,release_seed_c,image_cti_p)
print(datetime.now())
image_cti_result = np.zeros((nx,ntotal))
for i in range(nx):
for j in range(ntotal):
image_cti_result[i,j] = image_cti_p[i][j]
return image_cti_result.T
"""
if __name__ =='__main__':
nx,ny,noverscan,nsp,nmax = 4608,4616,84,3,10
ntotal = 4700
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([0,100,1000],dtype=np.int32)
release_seed = 500
image = fits.getdata("inputdata/image.fits").astype(np.int32)
get_trap_map(trap_seeds,nx,ny,nmax,rho_trap,beta,c,".")
bin2fits("trap.bin",".",nsp,nx,ny,nmax)
image_cti = CTI_sim(image,nx,ny,noverscan,nsp,nmax,beta,w,c,t,rho_trap,trap_seeds,release_seed)
fits.writeto("output/image_CTI.fits",data=image_cti,overwrite=True)
"""
#include objects here:
objects = src/add_CTI1.o src/nrutil.o src/ran1.o src/ran2.o src/poidev.o src/gammln.o src/gasdev.o src/sort.o src/creattraps.o
add_CTI.so: $(objects)
gcc -shared -fPIC -std=c99 -o $@ $(objects) -lm
# general compilation rules
.SUFFIXES: .c .o
.c.o:
cc -c $< -O3 -shared -fPIC -std=c99 -o $@
.PHONY : clean
clean:
rm -f src/*.o add_CTI.so
CTI_lgl_v0.3/
add_CTIfinal.c >> add_CTI.c
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