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MANIFEST.in
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MANIFEST.in
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include nuwavsource/pixpos/nuApixpos20100101v007.fits
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include nuwavsource/pixpos/nuBpixpos20100101v007.fits
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50
README.md
50
README.md
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# wavsource_nustar
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# nuwavsource
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This package is supposed to be used to detect the sources in NuStar observations and generate a mask excluding the signal from the sources of any kind.
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Additionaly, it generates a table containing:
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Useful data about the observation:
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1. OBS_ID
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2. Detector
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3. Coordinates in equatorial (ra,dec) and galactical (lon,lat) systems
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4. Time of the observation in seconds
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5. Exposure
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Useful algorythm-related data:
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6. Average count rate on unmasked area
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7. Portion of unmasked area
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8. Specific statistical metric[1] before and after masking the detected sources
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9. Root-mean-square of counts in unmasked area
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## Installation
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This package is to be used with Python 3.x.x
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To install tha package write
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```bash
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pip install nuwavsource
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```
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## Usage
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To use the package in your project, import it in by writing
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```python
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from nuwavsource import nuwavsource
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```
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You can process the cl.evt file by creating an Observation class object:
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```python
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obs = nuwavsource.Observation(path_to_evt_file)
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```
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Additionally, the energy band in KeV to get events from can be passed as an argument. The default value is [3,20].
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```python
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obs = nuwavsource.Observation(path_to_evt_file,E_borders=[E_min,E_max])
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```
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Binary file not shown.
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# %%
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from get_region_pack import *
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import numpy as np
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from pandas import DataFrame, read_csv
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from astropy.table import Table
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from astropy.coordinates import SkyCoord
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from astropy import units as u
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from multiprocessing import get_context, cpu_count
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import warnings
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import time
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import os
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warnings.filterwarnings('ignore')
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# %%
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def poisson_divider(array):
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sub_arrays = np.zeros((4,180,180))
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for i in range(2):
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for j in range(2):
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sub_arrays[i+2*j] = array[180*i:180*(i+1),180*j:180*(j+1)].filled(-1000)
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pix_sum = 0
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for layer in sub_arrays:
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_masked_array = np.ma.masked_less(layer,0)
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pix_sum += ((_masked_array-_masked_array.mean())**2/_masked_array.mean()).sum()
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pix_sum /= np.logical_not(array.mask).sum()
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return pix_sum
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def process(argument):
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idx, obs_name = argument
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bin_num = 6
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try:
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obs = Observation(obs_name)
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sky_coord = SkyCoord(ra=obs.ra*u.deg,dec=obs.dec*u.deg,frame='fk5').transform_to('galactic')
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lon, lat = sky_coord.l.value, sky_coord.b.value
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rem_signal, rem_area, poiss_comp, rms = np.zeros((4,2**bin_num))
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region = np.zeros(obs.data.shape, dtype=bool)
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rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
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masked_obs = np.ma.masked_array(obs.data, mask = region)
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good_lvl = np.zeros(bin_num,dtype=bool)
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good_idx = 0
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if obs.exposure > 1000:
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wav_obs = obs.wavdecomp('gauss',(5,3),occ_coeff=True)
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occ_coeff = obs.get_coeff()
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for idx, lvl in enumerate(binary_array(bin_num)):
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try:
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# region = np.array([layer>0 for layer in wav_obs[2:-1][lvl]]).sum(0).astype(bool)
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region = wav_obs[2:-1][lvl].sum(0)>0
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except ValueError:
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region = np.zeros(obs.data.shape,dtype=bool)
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masked_obs = np.ma.masked_array(obs.data, mask = region)*occ_coeff
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rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
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rem_signal[idx] = 1-obs.data[region].sum()/obs.data.sum()
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rem_area[idx] = 1 - rem_region.sum()/np.logical_not(obs.data.mask).sum()
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# poiss_comp[idx] = poisson_divider(masked_obs)
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poiss_comp[idx] = np.mean((masked_obs-masked_obs.mean())**2/masked_obs.mean())
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rms[idx] = np.sqrt(((masked_obs-masked_obs.mean())**2).mean())
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parameter = lambda idx: ((poiss_comp[idx])**2+((1-rem_area[idx])*0.5)**2)
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if (parameter(idx)<parameter(good_idx)):
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good_idx = idx
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good_lvl = lvl
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try:
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# region = np.array([layer>0 for layer in wav_obs[2:-1][lvl]]).sum(0).astype(bool)
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region = wav_obs[2:-1][good_lvl].sum(0)>0
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except ValueError:
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region = np.zeros(obs.data.shape,dtype=bool)
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masked_obs = np.ma.masked_array(obs.data, mask = region)
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rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
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to_table = [obs.obs_id,
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obs.det,
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obs.ra,
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obs.dec,
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lon,
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lat,
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obs.time_start,
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obs.exposure,
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masked_obs.mean()/obs.exposure, #count rate
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1 - rem_region.sum()/np.logical_not(obs.data.mask).sum(), #rem_area
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poiss_comp[good_idx],
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poiss_comp[0],
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rms[good_idx]
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]
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else:
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to_table = [obs.obs_id,
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obs.det,
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obs.ra,
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obs.dec,
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lon,
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lat,
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obs.time_start,
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obs.exposure,
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-1,
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-1, #rem_signal
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-1, #rem_area
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-1,
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-1,
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-1
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]
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return to_table, region.astype(int)
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except TypeError:
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return obs_name, np.zeros((360,360))
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#%%
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if __name__ == '__main__':
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#DIALOGUE
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print('Enter path to the input folder')
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input_folder = input()
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obs_list = get_link_list(input_folder,sort_list = True)[:]
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print('Create new file for this processing? y/n')
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continue_old = input()
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if continue_old == 'y':
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start_new = True
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elif continue_old == 'n':
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start_new = False
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else:
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print('Cannot interprete input, closing script')
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raise SystemExit(0)
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print(f'Enter path to the output folder')
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fits_folder = input()
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region_folder = f'{fits_folder}\\Region'
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#INIT ALL NECESSARY FILES AND VARIBALES
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start = time.perf_counter()
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processing = True
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group_size = 50
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os.makedirs(region_folder,exist_ok = True)
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#FILTERING BY THE FILE SIZE
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print(f'Finished scanning folders. Found {len(obs_list)} observations.')
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table = {
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'obs_id':[], 'detector':[], 'ra':[], 'dec':[], 'lon':[], 'lat':[], 't_start':[], 'exposure':[],
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'count_rate':[], 'remaining_area':[], 'poisson_chi2':[], 'poisson_chi2_full':[], 'rms':[]
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}
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if start_new:
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out_table = DataFrame(table)
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out_table.to_csv(f'{fits_folder}\\test.csv')
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out_table.to_csv(f'{fits_folder}\\test_skipped.csv')
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#FILTERING OUT PROCESSED OBSERVATIONS
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already_processed_list = read_csv(f'{fits_folder}\\test.csv',index_col=0,dtype={'obs_id':str})
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already_skipped_list = read_csv(f'{fits_folder}\\test_skipped.csv',index_col=0,dtype={'obs_id':str})
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already_processed = (already_processed_list['obs_id'].astype(str)+already_processed_list['detector']).values
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already_skipped = (already_skipped_list['obs_id'].astype(str)+already_skipped_list['detector']).values
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obs_list_names = [curr[curr.index('nu')+2:curr.index('_cl.evt')-2] for curr in obs_list]
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not_processed = np.array([(curr not in already_processed) for curr in obs_list_names])
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not_skipped = np.array([(curr not in already_skipped) for curr in obs_list_names])
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obs_list = obs_list[np.logical_and(not_processed,not_skipped)]
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print(f'Removed already processed observations. {len(obs_list)} observations remain.')
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#START PROCESSING
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if processing:
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print('Started processing...')
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num = 0
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for group_idx in range(len(obs_list)//group_size+1):
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print(f'Started group {group_idx}')
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group_list = obs_list[group_size*group_idx:min(group_size*(group_idx+1),len(obs_list))]
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max_size = np.array([stat(file).st_size/2**20 for file in group_list]).max()
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process_num = cpu_count() if max_size<50 else (cpu_count()//2 if max_size<200 else (cpu_count()//4 if max_size<1000 else 1))
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print(f"Max file size in group is {max_size:.2f}Mb, create {process_num} processes")
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with get_context('spawn').Pool(processes=process_num) as pool:
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for result,region in pool.imap(process,enumerate(group_list)):
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if type(result) is np.str_:
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obs_id = result[result.index('nu'):result.index('_cl.evt')]
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print(f'{num:>3} is skipped. File {obs_id}')
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num +=1
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continue
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for key,value in zip(table.keys(),result):
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table[key] = [value]
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if table['exposure'][0] < 1000:
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print(f'{num:>3} {str(result[0])+result[1]} is skipped. Exposure < 1000')
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DataFrame(table).to_csv(f'{fits_folder}\\test_skipped.csv',mode='a',header=False)
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num +=1
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continue
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DataFrame(table).to_csv(f'{fits_folder}\\test.csv',mode='a',header=False)
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fits.writeto(f'{region_folder}\\{str(result[0])+result[1]}_region.fits', region, overwrite= True)
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print(f'{num:>3} {str(result[0])+result[1]} is written.')
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num +=1
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print('Converting generated csv to fits file...')
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print(f'Current time in: {(time.perf_counter()-start):.2f}')
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print(f'Processed {num/len(obs_list)*100:.2f} percent')
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csv_file = read_csv(f'{fits_folder}\\test.csv',index_col=0,dtype={'obs_id':str})
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Table.from_pandas(csv_file).write(f'{fits_folder}\\test.fits',overwrite=True)
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print(f'Finished writing: {time.perf_counter()-start}')
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# %%
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# %%
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import numpy as np
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import itertools
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from os import stat
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from scipy.signal import fftconvolve, convolve2d
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from astropy.io import fits
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from astropy.wcs import WCS
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from glob import glob
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# %%
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def binary_array(num):
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variants = [[0,1],]*num
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out = np.zeros((2**num,num),bool)
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for idx, level in enumerate(itertools.product(*variants)):
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out[idx] = np.array(level,dtype=bool)
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return out
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def create_array(filename,mode='Sky'):
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temp = fits.getdata(filename,1)
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if mode == 'Sky':
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return np.histogram2d(temp['Y'],temp['X'],1000,[[0, 1000], [0, 1000]])[0]
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if mode == 'Det':
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return np.histogram2d(temp['DET1Y'],temp['DET1X'],360,[[0, 360], [0, 360]])[0]
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def get_wcs(file):
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header = file[1].header
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wcs = WCS({
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'CTYPE1': header['TCTYP38'], 'CTYPE2': header['TCTYP39'],
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'CUNIT1': header['TCUNI38'], 'CUNIT2': header['TCUNI39'],
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'CDELT1': header['TCDLT38'], 'CDELT2': header['TCDLT39'],
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'CRPIX1': header['TCRPX38'], 'CRPIX2': header['TCRPX39'],
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'CRVAL1': header['TCRVL38'], 'CRVAL2': header['TCRVL39'],
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'NAXIS1': header['TLMAX38'], 'NAXIS2': header['TLMAX39']
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})
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return wcs
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def get_link_list(folder, sort_list=True):
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links = glob(f'{folder}\\**\\*_cl.evt',recursive=True)
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if sort_list:
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sorted_list = sorted(links, key=lambda x: stat(x).st_size)
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return np.array(sorted_list)
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else:
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return np.array(links)
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def atrous(level = 0, resize = False, max_size = 1001):
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base = 1/256*np.array([
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[1, 4, 6, 4, 1],
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[4, 16, 24, 16, 4],
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[6, 24, 36, 24, 6],
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[4, 16, 24, 16, 4],
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[1, 4, 6, 4, 1],
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])
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size = 2**level * (base.shape[0]-1)+1
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output = np.zeros((size,size))
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output[::2**level, ::2**level] = base
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if resize:
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output = np.pad(output, pad_width=2**(level+1))
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if output.shape[0]>max_size:
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return output[(size-1)//2-(max_size-1)//2:(size-1)//2+(max_size-1)//2+1, (size-1)//2-(max_size-1)//2:(size-1)//2+(max_size-1)//2+1]
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return output
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def gauss(level=0, resize=False, max_size = 1000):
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size = min(5*2**(level+1)+1, max_size)
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sigma = 2**(level)
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A = 1/(2*np.pi*sigma**2)**0.5
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x = A*np.exp( (-(np.arange(size)-(size-1)//2)**2)/(2*sigma**2))
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out = np.multiply.outer(x,x)
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return out
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def adjecent(array):
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grid = np.array([
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[1,1,1],
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[1,0,1],
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[1,1,1]
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])
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output = fftconvolve(array,grid,mode='same') >= 0.5
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try:
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output = np.logical_and(np.logical_and(output, np.logical_not(array)),np.logical_not(array.mask))
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except AttributeError:
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output = np.logical_and(output, np.logical_not(array))
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output = np.argwhere(output == True)
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return output[:,0], output[:,1]
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def add_borders(array,middle=True):
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mask = np.zeros(array.shape)
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datax, datay = np.any(array>0,0), np.any(array>0,1)
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#Add border masks
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x_min, y_min = np.argmax(datax), np.argmax(datay)
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x_max, y_max = len(datax) - np.argmax(datax[::-1]), len(datay) - np.argmax(datay[::-1])
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mask[y_min:y_max,x_min:x_max] = True
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if middle is True:
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mask[176:191,:] = False
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mask[:,176:191] = False
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mask = np.logical_not(mask)
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return mask
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def fill_poisson(array, size_input=32):
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if not(isinstance(array,np.ma.MaskedArray)):
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print('No mask found')
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return array
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size = size_input
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output = array.data.copy()
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mask = array.mask.copy()
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while mask.sum()>1:
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kernel = np.ones((size,size))/size**2
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coeff = fftconvolve(np.logical_not(mask),kernel,mode='same')
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mean = fftconvolve(output,kernel,mode='same')
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idx = np.where(np.logical_and(mask,coeff>0.1))
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output[idx] = np.random.poisson(np.abs(mean[idx]/coeff[idx]))
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mask[idx] = False
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size *= 2
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return output
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def fill_mean(array,size_input=3):
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size = size_input
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if not(isinstance(array,np.ma.MaskedArray)):
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print('No mask found')
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return array
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output = array.filled(0)
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for i,j in zip(*np.where(array.mask)):
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output[i,j] = array[max(0,i-size):min(array.shape[0]-1,i+size+1),max(0,j-size):min(array.shape[1]-1,j+size+1)].mean()
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while np.isnan(output).any():
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size += 5
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for i,j in zip(*np.where(np.isnan(output))):
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output[i,j] = array[max(0,i-size):min(array.shape[0]-1,i+size+1),max(0,j-size):min(array.shape[1]-1,j+size+1)].mean()
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return output
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def mirror(array):
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size = array.shape[0]
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output = np.tile(array,(3,3))
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output[0:size] = np.flipud(output[0:size])
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output[2*size:3*size] = np.flipud(output[2*size:3*size])
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output[:,0:size] = np.fliplr(output[:,0:size])
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output[:,2*size:3*size] = np.fliplr(output[:,2*size:3*size])
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return output
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class Observation:
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def __init__(self, file_name, E_borders=[3,20]):
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self.filename = file_name
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self.name = file_name[file_name.find('nu'):].replace('_cl.evt','')
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with fits.open(file_name) as file:
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self.obs_id = file[0].header['OBS_ID']
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self.ra = file[0].header['RA_NOM']
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self.dec = file[0].header['DEC_NOM']
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||||
self.time_start = file[0].header['TSTART']
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self.header = file[0].header
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self.det = self.header['INSTRUME'][-1]
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self.wcs = get_wcs(file)
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self.data = np.ma.masked_array(*self.get_data(file,E_borders))
|
||||
self.hard_mask = add_borders(self.data.data,middle=False)
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||||
shift = shift = int((360-64)/2)
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self.model = (fits.getdata(f'D:\Programms\Jupyter\Science\Source_mask\Model/det1_fpm{self.det}.cxb.fits',0)
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||||
*(180/np.pi/10150)**2)[shift:360+shift,shift:360+shift]
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||||
self.exposure = self.header['EXPOSURE']
|
||||
def get_coeff(self):
|
||||
coeff = np.array([0.977,0.861,1.163,1.05]) if self.det=='A' else np.array([1.004,0.997,1.025,0.979])
|
||||
resized_coeff = (coeff).reshape(2,2).repeat(180,0).repeat(180,1)
|
||||
return resized_coeff
|
||||
def get_data(self, file, E_borders=[3,20]):
|
||||
PI_min, PI_max = (np.array(E_borders)-1.6)/0.04
|
||||
data = file[1].data.copy()
|
||||
idx_mask = (data['STATUS'].sum(1) == 0)
|
||||
idx_output = np.logical_and(idx_mask,np.logical_and((data['PI']>PI_min),(data['PI']<PI_max)))
|
||||
data_output = data[idx_output]
|
||||
data_mask = data[np.logical_not(idx_mask)]
|
||||
build_hist = lambda array: np.histogram2d(array['DET1Y'],array['DET1X'],360,[[0,360],[0,360]])[0]
|
||||
output = build_hist(data_output)
|
||||
mask = build_hist(data_mask)
|
||||
mask = np.logical_or(mask,add_borders(output))
|
||||
mask = np.logical_or(mask, self.get_bad_pix(file))
|
||||
return output, mask
|
||||
def get_bad_pix(self, file):
|
||||
output = np.zeros((360,360))
|
||||
kernel = np.ones((5,5))
|
||||
for i in range(4):
|
||||
pixpos_file = fits.getdata(f'D:\\Programms\\Jupyter\\Science\\Source_mask\\Pixpos\\nu{self.det}pixpos20100101v007.fits',i+1)
|
||||
bad_pix_file = file[3+i].data.copy()
|
||||
temp = np.zeros(len(pixpos_file),dtype=bool)
|
||||
for x,y in zip(bad_pix_file['rawx'],bad_pix_file['rawy']):
|
||||
temp = np.logical_or(temp, np.equal(pixpos_file['rawx'],x)*np.equal(pixpos_file['rawy'],y))
|
||||
temp = pixpos_file[temp]
|
||||
output += np.histogram2d(temp['REF_DET1Y'],temp['REF_DET1X'], 360, [[0,360],[0,360]])[0]
|
||||
output = convolve2d(output, kernel, mode='same') > 0
|
||||
return output
|
||||
def wavdecomp(self, mode = 'atrous', thresh=False,occ_coeff = False):
|
||||
#THRESHOLD
|
||||
if type(thresh) is int: thresh_max, thresh_add = thresh, thresh/2
|
||||
elif type(thresh) is tuple: thresh_max, thresh_add = thresh
|
||||
#INIT NEEDED VARIABLES
|
||||
wavelet = globals()[mode]
|
||||
max_level = 8
|
||||
conv_out = np.zeros((max_level+1,self.data.shape[0],self.data.shape[1]))
|
||||
size = self.data.shape[0]
|
||||
#PREPARE ORIGINAL DATA FOR ANALYSIS: FILL THE HOLES + MIRROR + DETECTOR CORRECTION
|
||||
data = fill_poisson(self.data)
|
||||
if occ_coeff: data = data*self.get_coeff()
|
||||
data = mirror(data)
|
||||
data_bkg = data.copy()
|
||||
#ITERATIVELY CONDUCT WAVLET DECOMPOSITION
|
||||
for i in range(max_level):
|
||||
conv = fftconvolve(data,wavelet(i),mode='same')
|
||||
temp_out = data-conv
|
||||
#ERRORMAP CALCULATION
|
||||
if thresh_max != 0:
|
||||
sig = ((wavelet(i)**2).sum())**0.5
|
||||
bkg = fftconvolve(data_bkg, wavelet(i),mode='same')
|
||||
bkg[bkg<0] = 0
|
||||
# err = (1+np.sqrt(bkg/sig**2 + 0.75))*sig**3
|
||||
err = (1+np.sqrt(bkg+0.75))*sig
|
||||
# significant = (np.abs(temp_out)> thresh_max*err)[size:2*size,size:2*size]
|
||||
significant = (temp_out > thresh_max*err)[size:2*size,size:2*size]
|
||||
if thresh_add != 0:
|
||||
# add_significant = (np.abs(temp_out)> thresh_add*err)[size:2*size,size:2*size]
|
||||
add_significant = (temp_out > thresh_add*err)[size:2*size,size:2*size]
|
||||
adj = adjecent(significant)
|
||||
add_condition = np.logical_and(add_significant[adj[0],adj[1]],np.logical_not(significant[adj[0],adj[1]]))
|
||||
while (add_condition).any():
|
||||
to_add = adj[0][add_condition], adj[1][add_condition]
|
||||
significant[to_add[0],to_add[1]] = True
|
||||
adj = adjecent(significant)
|
||||
add_condition = np.logical_and(add_significant[adj[0],adj[1]],np.logical_not(significant[adj[0],adj[1]]))
|
||||
# add_condition = np.logical_and(np.abs(temp_out)[adj[0],adj[1]] >= thresh_add*err[adj[0],adj[1]], np.logical_not(significant)[adj[0],adj[1]])
|
||||
temp_out[size:2*size,size:2*size][np.logical_not(significant)] = 0
|
||||
#WRITING THE WAVELET DECOMP LAYER
|
||||
conv_out[i] = +temp_out[size:2*size,size:2*size]
|
||||
conv_out[i][conv_out[i]<0]=0 #leave only positive data to prevent problems while summing layers
|
||||
data = conv
|
||||
conv_out[max_level] = conv[size:2*size,size:2*size]
|
||||
return conv_out
|
||||
# %%
|
1
nuwavsource/__init__.py
Normal file
1
nuwavsource/__init__.py
Normal file
@ -0,0 +1 @@
|
||||
name = 'nuwavsource'
|
BIN
nuwavsource/__pycache__/__init__.cpython-39.pyc
Normal file
BIN
nuwavsource/__pycache__/__init__.cpython-39.pyc
Normal file
Binary file not shown.
BIN
nuwavsource/__pycache__/nuwavsource.cpython-39.pyc
Normal file
BIN
nuwavsource/__pycache__/nuwavsource.cpython-39.pyc
Normal file
Binary file not shown.
441
nuwavsource/nuwavsource.py
Normal file
441
nuwavsource/nuwavsource.py
Normal file
@ -0,0 +1,441 @@
|
||||
# %%
|
||||
import numpy as np
|
||||
import itertools
|
||||
from pandas import DataFrame, read_csv
|
||||
from astropy.table import Table, unique
|
||||
from astropy.coordinates import SkyCoord
|
||||
from astropy import units as u
|
||||
from multiprocessing import get_context, cpu_count
|
||||
from time import perf_counter
|
||||
from os import stat, makedirs
|
||||
from os.path import dirname
|
||||
from scipy.signal import fftconvolve, convolve2d
|
||||
from astropy.io import fits
|
||||
from astropy.wcs import WCS
|
||||
from glob import glob
|
||||
from warnings import filterwarnings
|
||||
filterwarnings('ignore')
|
||||
|
||||
|
||||
def get_link_list(folder, sort_list=True):
|
||||
links = glob(f'{folder}\\**\\*_cl.evt', recursive=True)
|
||||
if sort_list:
|
||||
sorted_list = sorted(links, key=lambda x: stat(x).st_size)
|
||||
return np.array(sorted_list)
|
||||
else:
|
||||
return np.array(links)
|
||||
|
||||
|
||||
def binary_array(num):
|
||||
variants = [[0, 1], ]*num
|
||||
out = np.zeros((2**num, num), bool)
|
||||
for idx, level in enumerate(itertools.product(*variants)):
|
||||
out[idx] = np.array(level, dtype=bool)
|
||||
return out
|
||||
|
||||
|
||||
def create_array(filename, mode='Sky'):
|
||||
temp = fits.getdata(filename, 1)
|
||||
if mode == 'Sky':
|
||||
return np.histogram2d(temp['Y'],
|
||||
temp['X'],
|
||||
1000,
|
||||
[[0, 1000], [0, 1000]])[0]
|
||||
if mode == 'Det':
|
||||
return np.histogram2d(temp['DET1Y'],
|
||||
temp['DET1X'],
|
||||
360,
|
||||
[[0, 360], [0, 360]])[0]
|
||||
|
||||
|
||||
def get_wcs(file):
|
||||
header = file[1].header
|
||||
wcs = WCS({
|
||||
'CTYPE1': header['TCTYP38'], 'CTYPE2': header['TCTYP39'],
|
||||
'CUNIT1': header['TCUNI38'], 'CUNIT2': header['TCUNI39'],
|
||||
'CDELT1': header['TCDLT38'], 'CDELT2': header['TCDLT39'],
|
||||
'CRPIX1': header['TCRPX38'], 'CRPIX2': header['TCRPX39'],
|
||||
'CRVAL1': header['TCRVL38'], 'CRVAL2': header['TCRVL39'],
|
||||
'NAXIS1': header['TLMAX38'], 'NAXIS2': header['TLMAX39']
|
||||
})
|
||||
return wcs
|
||||
|
||||
|
||||
def atrous(level=0, max_size=1001):
|
||||
base = 1/256*np.array([
|
||||
[1, 4, 6, 4, 1],
|
||||
[4, 16, 24, 16, 4],
|
||||
[6, 24, 36, 24, 6],
|
||||
[4, 16, 24, 16, 4],
|
||||
[1, 4, 6, 4, 1],
|
||||
])
|
||||
size = 2**level * (base.shape[0]-1)+1
|
||||
output = np.zeros((size, size))
|
||||
output[::2**level, ::2**level] = base
|
||||
if output.shape[0] > max_size:
|
||||
return output[(size-1)//2-(max_size-1)//2:(size-1)//2+(max_size-1)//2+1,
|
||||
(size-1)//2-(max_size-1)//2:(size-1)//2+(max_size-1)//2+1]
|
||||
return output
|
||||
|
||||
|
||||
def gauss(level=0, max_size=1000):
|
||||
size = min(5*2**(level+1)+1, max_size)
|
||||
sigma = 2**(level)
|
||||
A = 1/(2*np.pi*sigma**2)**0.5
|
||||
x = A*np.exp((-(np.arange(size)-(size-1)//2)**2)/(2*sigma**2))
|
||||
out = np.multiply.outer(x, x)
|
||||
return out
|
||||
|
||||
|
||||
def adjecent(array):
|
||||
grid = np.array([
|
||||
[1, 1, 1],
|
||||
[1, 0, 1],
|
||||
[1, 1, 1]
|
||||
])
|
||||
output = fftconvolve(array, grid, mode='same') >= 0.5
|
||||
try:
|
||||
output = np.logical_and(np.logical_and(output, np.logical_not(array)),
|
||||
np.logical_not(array.mask))
|
||||
except AttributeError:
|
||||
output = np.logical_and(output, np.logical_not(array))
|
||||
output = np.argwhere(output == True)
|
||||
return output[:, 0], output[:, 1]
|
||||
|
||||
|
||||
def add_borders(array, middle=True):
|
||||
mask = np.zeros(array.shape)
|
||||
datax, datay = np.any(array > 0, 0), np.any(array > 0, 1)
|
||||
# Add border masks
|
||||
x_min, y_min = np.argmax(datax), np.argmax(datay)
|
||||
x_max = len(datax) - np.argmax(datax[::-1])
|
||||
y_max = len(datay) - np.argmax(datay[::-1])
|
||||
mask[y_min:y_max, x_min:x_max] = True
|
||||
if middle is True:
|
||||
mask[176:191, :] = False
|
||||
mask[:, 176:191] = False
|
||||
mask = np.logical_not(mask)
|
||||
return mask
|
||||
|
||||
|
||||
def fill_poisson(array, size_input=32):
|
||||
if not (isinstance(array, np.ma.MaskedArray)):
|
||||
print('No mask found')
|
||||
return array
|
||||
size = size_input
|
||||
output = array.data.copy()
|
||||
mask = array.mask.copy()
|
||||
while mask.sum() > 1:
|
||||
kernel = np.ones((size, size))/size**2
|
||||
coeff = fftconvolve(np.logical_not(mask), kernel, mode='same')
|
||||
mean = fftconvolve(output, kernel, mode='same')
|
||||
idx = np.where(np.logical_and(mask, coeff > 0.1))
|
||||
output[idx] = np.random.poisson(np.abs(mean[idx]/coeff[idx]))
|
||||
mask[idx] = False
|
||||
size *= 2
|
||||
return output
|
||||
|
||||
|
||||
def mirror(array):
|
||||
size = array.shape[0]
|
||||
output = np.tile(array, (3, 3))
|
||||
output[0:size] = np.flipud(output[0:size])
|
||||
output[2*size:3*size] = np.flipud(output[2*size:3*size])
|
||||
output[:, 0:size] = np.fliplr(output[:, 0:size])
|
||||
output[:, 2*size:3*size] = np.fliplr(output[:, 2*size:3*size])
|
||||
return output
|
||||
|
||||
|
||||
class Observation:
|
||||
def __init__(self, file_name, E_borders=[3,20]):
|
||||
self.filename = file_name
|
||||
self.name = file_name[file_name.find('nu'):].replace('_cl.evt','')
|
||||
with fits.open(file_name) as file:
|
||||
self.obs_id = file[0].header['OBS_ID']
|
||||
self.ra = file[0].header['RA_NOM']
|
||||
self.dec = file[0].header['DEC_NOM']
|
||||
self.time_start = file[0].header['TSTART']
|
||||
self.header = file[0].header
|
||||
self.det = self.header['INSTRUME'][-1]
|
||||
self.wcs = get_wcs(file)
|
||||
self.data = np.ma.masked_array(*self.get_data(file, E_borders))
|
||||
self.hard_mask = add_borders(self.data.data, middle=False)
|
||||
self.exposure = self.header['EXPOSURE']
|
||||
|
||||
def get_coeff(self):
|
||||
coeff = np.array([0.977, 0.861, 1.163, 1.05]) if self.det == 'A' else np.array([1.004, 0.997, 1.025, 0.979])
|
||||
resized_coeff = (coeff).reshape(2, 2).repeat(180, 0).repeat(180, 1)
|
||||
return resized_coeff
|
||||
|
||||
def get_data(self, file, E_borders=[3, 20]):
|
||||
PI_min, PI_max = (np.array(E_borders)-1.6)/0.04
|
||||
data = file[1].data.copy()
|
||||
idx_mask = (data['STATUS'].sum(1) == 0)
|
||||
idx_output = np.logical_and(idx_mask, np.logical_and((data['PI'] > PI_min), (data['PI'] < PI_max)))
|
||||
data_output = data[idx_output]
|
||||
data_mask = data[np.logical_not(idx_mask)]
|
||||
build_hist = lambda array: np.histogram2d(array['DET1Y'], array['DET1X'], 360, [[0, 360], [0, 360]])[0]
|
||||
output = build_hist(data_output)
|
||||
mask = build_hist(data_mask)
|
||||
mask = np.logical_or(mask, add_borders(output))
|
||||
mask = np.logical_or(mask, self.get_bad_pix(file))
|
||||
return output, mask
|
||||
|
||||
def get_bad_pix(self, file):
|
||||
output = np.zeros((360, 360))
|
||||
kernel = np.ones((5, 5))
|
||||
for i in range(4):
|
||||
current_dir = dirname(__file__)
|
||||
pixpos_file = fits.getdata(f'{current_dir}\\pixpos\\nu{self.det}pixpos20100101v007.fits',i+1)
|
||||
bad_pix_file = file[3+i].data.copy()
|
||||
temp = np.zeros(len(pixpos_file), dtype=bool)
|
||||
for x, y in zip(bad_pix_file['rawx'], bad_pix_file['rawy']):
|
||||
temp = np.logical_or(temp, np.equal(pixpos_file['rawx'], x)*np.equal(pixpos_file['rawy'], y))
|
||||
temp = pixpos_file[temp]
|
||||
output += np.histogram2d(temp['REF_DET1Y'], temp['REF_DET1X'], 360, [[0, 360],[0, 360]])[0]
|
||||
output = convolve2d(output, kernel, mode='same') > 0
|
||||
return output
|
||||
|
||||
def wavdecomp(self, mode='gauss', thresh=False, occ_coeff=False):
|
||||
# THRESHOLD
|
||||
if type(thresh) is int:
|
||||
thresh_max, thresh_add = thresh, thresh/2
|
||||
elif type(thresh) is tuple:
|
||||
thresh_max, thresh_add = thresh
|
||||
# INIT NEEDED VARIABLES
|
||||
wavelet = globals()[mode]
|
||||
max_level = 8
|
||||
conv_out = np.zeros((max_level+1, self.data.shape[0], self.data.shape[1]))
|
||||
size = self.data.shape[0]
|
||||
# PREPARE ORIGINAL DATA FOR ANALYSIS: FILL THE HOLES + MIRROR + DETECTOR CORRECTION
|
||||
data = fill_poisson(self.data)
|
||||
if occ_coeff:
|
||||
data = data*self.get_coeff()
|
||||
data = mirror(data)
|
||||
data_bkg = data.copy()
|
||||
# ITERATIVELY CONDUCT WAVLET DECOMPOSITION
|
||||
for i in range(max_level):
|
||||
conv = fftconvolve(data, wavelet(i), mode='same')
|
||||
temp_out = data-conv
|
||||
# ERRORMAP CALCULATION
|
||||
if thresh_max != 0:
|
||||
sig = ((wavelet(i)**2).sum())**0.5
|
||||
bkg = fftconvolve(data_bkg, wavelet(i), mode='same')
|
||||
bkg[bkg < 0] = 0
|
||||
err = (1+np.sqrt(bkg+0.75))*sig
|
||||
significant = (temp_out > thresh_max*err)[size:2*size, size:2*size]
|
||||
if thresh_add != 0:
|
||||
add_significant = (temp_out > thresh_add*err)[size:2*size, size:2*size]
|
||||
adj = adjecent(significant)
|
||||
add_condition = np.logical_and(add_significant[adj[0], adj[1]],
|
||||
np.logical_not(significant[adj[0], adj[1]]))
|
||||
while (add_condition).any():
|
||||
to_add = adj[0][add_condition], adj[1][add_condition]
|
||||
significant[to_add[0], to_add[1]] = True
|
||||
adj = adjecent(significant)
|
||||
add_condition = np.logical_and(add_significant[adj[0], adj[1]],
|
||||
np.logical_not(significant[adj[0],adj[1]]))
|
||||
temp_out[size:2*size, size:2*size][np.logical_not(significant)] = 0
|
||||
# WRITING THE WAVELET DECOMP LAYER
|
||||
conv_out[i] = +temp_out[size:2*size, size:2*size]
|
||||
# DISCARDING NEGATIVE COMPONENTS OF WAVELETS TO MAKE MASK BY SUMMING WAVELET LAYERS
|
||||
conv_out[i][conv_out[i] < 0] = 0
|
||||
data = conv
|
||||
conv_out[max_level] = conv[size:2*size, size:2*size]
|
||||
return conv_out
|
||||
|
||||
def region_to_raw(self, region):
|
||||
x_region, y_region = np.where(region)
|
||||
tables = []
|
||||
for i in range(4):
|
||||
current_dir = dirname(__file__)
|
||||
pixpos = Table(fits.getdata(f'{current_dir}\\pixpos\\nu{self.det}pixpos20100101v007.fits', i+1))
|
||||
pixpos = pixpos[pixpos['REF_DET1X'] != -1]
|
||||
test = np.zeros(len(pixpos['REF_DET1X']), dtype=bool)
|
||||
for idx, (x, y) in enumerate(zip(pixpos['REF_DET1X'], pixpos['REF_DET1Y'])):
|
||||
test[idx] = np.logical_and(np.equal(x, x_region), np.equal(y, y_region)).any()
|
||||
table = Table({'RAWX': pixpos['RAWX'][test], 'RAWY': pixpos['RAWY'][test]})
|
||||
if not table:
|
||||
tables.append(table)
|
||||
else:
|
||||
tables.append(unique(table))
|
||||
hdu_list = fits.HDUList([
|
||||
fits.PrimaryHDU(),
|
||||
fits.table_to_hdu(tables[0]),
|
||||
fits.table_to_hdu(tables[1]),
|
||||
fits.table_to_hdu(tables[2]),
|
||||
fits.table_to_hdu(tables[3]),
|
||||
])
|
||||
return hdu_list
|
||||
|
||||
|
||||
def process(args):
|
||||
"""
|
||||
Creates a mask using wavelet decomposition and produces some statistical and metadata about the passed observation.
|
||||
args must contain two arguments: path to the file of interest and threshold, e.g. ('D:\Data\obs_cl.evt',(5,2))
|
||||
"""
|
||||
obs_path, thresh = args
|
||||
bin_num = 6
|
||||
try:
|
||||
obs = Observation(obs_path)
|
||||
sky_coord = SkyCoord(ra=obs.ra*u.deg, dec=obs.dec*u.deg, frame='fk5').transform_to('galactic')
|
||||
lon, lat = sky_coord.l.value, sky_coord.b.value
|
||||
rem_signal, rem_area, poiss_comp, rms = np.zeros((4, 2**bin_num))
|
||||
region = np.zeros(obs.data.shape, dtype=bool)
|
||||
region_raw = -1
|
||||
rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
|
||||
masked_obs = np.ma.masked_array(obs.data, mask=region)
|
||||
good_lvl = np.zeros(bin_num, dtype=bool)
|
||||
good_idx = 0
|
||||
if obs.exposure > 1000:
|
||||
wav_obs = obs.wavdecomp('gauss', thresh, occ_coeff=True)
|
||||
occ_coeff = obs.get_coeff()
|
||||
for idx, lvl in enumerate(binary_array(bin_num)):
|
||||
try:
|
||||
region = wav_obs[2:-1][lvl].sum(0) > 0
|
||||
except ValueError:
|
||||
region = np.zeros(obs.data.shape, dtype=bool)
|
||||
masked_obs = np.ma.masked_array(obs.data, mask=region)*occ_coeff
|
||||
rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
|
||||
rem_signal[idx] = 1-obs.data[region].sum()/obs.data.sum()
|
||||
rem_area[idx] = 1 - rem_region.sum()/np.logical_not(obs.data.mask).sum()
|
||||
poiss_comp[idx] = np.mean((masked_obs-masked_obs.mean())**2/masked_obs.mean())
|
||||
rms[idx] = np.sqrt(((masked_obs-masked_obs.mean())**2).mean())
|
||||
parameter = lambda idx: ((poiss_comp[idx])**2+((1-rem_area[idx])*0.5)**2)
|
||||
if (parameter(idx) < parameter(good_idx)):
|
||||
good_idx = idx
|
||||
good_lvl = lvl
|
||||
try:
|
||||
region = wav_obs[2:-1][good_lvl].sum(0) > 0
|
||||
if region.sum() > 0:
|
||||
region_raw = obs.region_to_raw(region.astype(int))
|
||||
except ValueError:
|
||||
region = np.zeros(obs.data.shape, dtype=bool)
|
||||
masked_obs = np.ma.masked_array(obs.data, mask=region)
|
||||
rem_region = np.logical_and(region, np.logical_not(obs.data.mask))
|
||||
to_table = [obs.obs_id,
|
||||
obs.det,
|
||||
obs.ra,
|
||||
obs.dec,
|
||||
lon,
|
||||
lat,
|
||||
obs.time_start,
|
||||
obs.exposure,
|
||||
masked_obs.mean()/obs.exposure, # count rate
|
||||
1 - rem_region.sum()/np.logical_not(obs.data.mask).sum(), # rem_area
|
||||
poiss_comp[good_idx],
|
||||
poiss_comp[0],
|
||||
rms[good_idx]
|
||||
]
|
||||
else:
|
||||
to_table = [obs.obs_id,
|
||||
obs.det,
|
||||
obs.ra,
|
||||
obs.dec,
|
||||
lon,
|
||||
lat,
|
||||
obs.time_start,
|
||||
obs.exposure,
|
||||
-1,
|
||||
-1, # rem_signal
|
||||
-1, # rem_area
|
||||
-1,
|
||||
-1,
|
||||
-1
|
||||
]
|
||||
return to_table, region.astype(int), region_raw
|
||||
except TypeError:
|
||||
return obs_path, -1, -1
|
||||
|
||||
|
||||
def process_folder(input_folder=None, start_new_file=None, fits_folder=None, thresh=None):
|
||||
# DIALOGUE
|
||||
if not (input_folder):
|
||||
print('Enter path to the input folder')
|
||||
input_folder = input()
|
||||
if not (start_new_file):
|
||||
print('Create new file for this processing? y/n')
|
||||
start_new_file = input()
|
||||
if start_new_file == 'y':
|
||||
start_new = True
|
||||
elif start_new_file == 'n':
|
||||
start_new = False
|
||||
else:
|
||||
print('Cannot interprete input, closing script')
|
||||
raise SystemExit(0)
|
||||
if not (fits_folder):
|
||||
print(f'Enter path to the output folder')
|
||||
fits_folder = input()
|
||||
region_folder = f'{fits_folder}\\Region'
|
||||
region_raw_folder = f'{fits_folder}\\Region_raw'
|
||||
if not thresh:
|
||||
print('Enter threshold values for wavelet decomposition:')
|
||||
print('General threshold:')
|
||||
_thresh_max = float(input())
|
||||
print('Additional threshold:')
|
||||
_thresh_add = float(input())
|
||||
thresh = (_thresh_max, _thresh_add)
|
||||
# CREATE ALL NECESSARY FILES AND VARIBALES
|
||||
obs_list = get_link_list(input_folder, sort_list=True)
|
||||
start = perf_counter()
|
||||
group_size = 50
|
||||
makedirs(region_folder, exist_ok=True)
|
||||
makedirs(region_raw_folder, exist_ok=True)
|
||||
# FILTERING BY THE FILE SIZE
|
||||
print(f'Finished scanning folders. Found {len(obs_list)} observations.')
|
||||
table = {
|
||||
'obs_id': [], 'detector': [], 'ra': [], 'dec': [],
|
||||
'lon': [], 'lat': [], 't_start': [], 'exposure': [],
|
||||
'count_rate': [], 'remaining_area': [], 'poisson_chi2': [],
|
||||
'poisson_chi2_full': [], 'rms': []
|
||||
}
|
||||
if start_new:
|
||||
out_table = DataFrame(table)
|
||||
out_table.to_csv(f'{fits_folder}\\test.csv')
|
||||
out_table.to_csv(f'{fits_folder}\\test_skipped.csv')
|
||||
# FILTERING OUT PROCESSED OBSERVATIONS
|
||||
already_processed_list = read_csv(f'{fits_folder}\\test.csv', index_col=0, dtype={'obs_id':str})
|
||||
already_skipped_list = read_csv(f'{fits_folder}\\test_skipped.csv', index_col=0, dtype={'obs_id':str})
|
||||
already_processed = (already_processed_list['obs_id'].astype(str)+already_processed_list['detector']).values
|
||||
already_skipped = (already_skipped_list['obs_id'].astype(str)+already_skipped_list['detector']).values
|
||||
obs_list_names = [curr[curr.index('nu')+2:curr.index('_cl.evt')-2] for curr in obs_list]
|
||||
not_processed = np.array([(curr not in already_processed) for curr in obs_list_names])
|
||||
not_skipped = np.array([(curr not in already_skipped) for curr in obs_list_names])
|
||||
obs_list = obs_list[np.logical_and(not_processed, not_skipped)]
|
||||
print(f'Removed already processed observations. {len(obs_list)} observations remain.')
|
||||
# START PROCESSING
|
||||
print('Started processing...')
|
||||
num = 0
|
||||
for group_idx in range(len(obs_list)//group_size+1):
|
||||
print(f'Started group {group_idx}')
|
||||
group_list = obs_list[group_size*group_idx:min(group_size*(group_idx+1), len(obs_list))]
|
||||
max_size = np.array([stat(file).st_size/2**20 for file in group_list]).max()
|
||||
process_num = cpu_count() if max_size < 50 else (cpu_count()//2 if max_size < 200 else (cpu_count()//4 if max_size < 1000 else 1))
|
||||
print(f"Max file size in group is {max_size:.2f}Mb, create {process_num} processes")
|
||||
with get_context('spawn').Pool(processes=process_num) as pool:
|
||||
packed_args = map(lambda _: (_, thresh), group_list)
|
||||
for result, region, region_raw in pool.imap(process, packed_args):
|
||||
if type(result) is np.str_:
|
||||
obs_id = result[result.index('nu'):result.index('_cl.evt')]
|
||||
print(f'{num:>3} is skipped. File {obs_id}')
|
||||
num += 1
|
||||
continue
|
||||
for key, value in zip(table.keys(), result):
|
||||
table[key] = [value]
|
||||
if table['exposure'][0] < 1000:
|
||||
print(f'{num:>3} {str(result[0])+result[1]} is skipped. Exposure < 1000')
|
||||
DataFrame(table).to_csv(f'{fits_folder}\\test_skipped.csv', mode='a', header=False)
|
||||
num +=1
|
||||
continue
|
||||
DataFrame(table).to_csv(f'{fits_folder}\\test.csv', mode='a', header=False)
|
||||
fits.writeto(f'{region_folder}\\{str(result[0])+result[1]}_region.fits', region, overwrite=True)
|
||||
if region_raw != -1:
|
||||
region_raw.writeto(f'{region_raw_folder}\\{str(result[0])+result[1]}_reg_raw.fits', overwrite=True)
|
||||
print(f'{num:>3} {str(result[0])+result[1]} is written.')
|
||||
num +=1
|
||||
print('Converting generated csv to fits file...')
|
||||
print(f'Current time in: {(perf_counter()-start):.2f}')
|
||||
print(f'Processed {num/len(obs_list)*100:.2f} percent')
|
||||
csv_file = read_csv(f'{fits_folder}\\test.csv', index_col=0, dtype={'obs_id': str})
|
||||
Table.from_pandas(csv_file).write(f'{fits_folder}\\test.fits', overwrite=True)
|
||||
print(f'Finished writing: {perf_counter()-start}')
|
27155
nuwavsource/pixpos/nuApixpos20100101v007.fits
Normal file
27155
nuwavsource/pixpos/nuApixpos20100101v007.fits
Normal file
File diff suppressed because one or more lines are too long
26144
nuwavsource/pixpos/nuBpixpos20100101v007.fits
Normal file
26144
nuwavsource/pixpos/nuBpixpos20100101v007.fits
Normal file
File diff suppressed because one or more lines are too long
5
requirements.txt
Normal file
5
requirements.txt
Normal file
@ -0,0 +1,5 @@
|
||||
astropy==5.1
|
||||
numpy==1.23.2
|
||||
pandas==1.4.4
|
||||
scipy==1.9.1
|
||||
setuptools==57.4.0
|
29
setup.py
Normal file
29
setup.py
Normal file
@ -0,0 +1,29 @@
|
||||
import setuptools
|
||||
|
||||
with open("README.md", "r") as fh:
|
||||
long_description = fh.read()
|
||||
|
||||
setuptools.setup(
|
||||
name="nuwavsource",
|
||||
version="0.0.4",
|
||||
author="Andrey Mukhin",
|
||||
author_email="amukhin@phystech.edu",
|
||||
description="A package for source exclusion in NuStar observation data using wavelet decomposition",
|
||||
long_description=long_description,
|
||||
long_description_content_type="text/markdown",
|
||||
url="https://github.com/Andreyousan/nuwavsource",
|
||||
packages=setuptools.find_packages(),
|
||||
include_package_data=True,
|
||||
classifiers=(
|
||||
"Programming Language :: Python :: 3",
|
||||
"License :: OSI Approved :: MIT License",
|
||||
"Operating System :: OS Independent",
|
||||
),
|
||||
install_requires = [
|
||||
'astropy==5.1',
|
||||
'numpy==1.23.2',
|
||||
'pandas==1.4.4',
|
||||
'scipy==1.9.1',
|
||||
'setuptools==57.4.0',
|
||||
]
|
||||
)
|
Loading…
x
Reference in New Issue
Block a user