energy interpolation added, convergence condition updated

This commit is contained in:
2025-06-16 16:21:19 +03:00
parent ea741219ce
commit 54febb8bbf
3 changed files with 402 additions and 1 deletions

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source_detection2.py Normal file
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import asyncio
import numpy as np
from astropy.io import fits
import matplotlib.pyplot as plt
from astropy.wcs import WCS
import tqdm
from multiprocessing.pool import ThreadPool
from chan_psf import solve_for_locations, solve_for_locations_eintp
psfe = np.array([1.8, 1.9, 3.0, 4.0, 6.0, 7.0, 8.0, 9.0])
def prepare_psf(evt):
"""
find all unique psf for observation and load in single 3d data cuve
return data cube with events slices indexes
"""
u, ui = np.unique(evt["psf_cube"], return_inverse=True)
data = np.array([np.load(p[3:])[:, ::-1,::-1].copy() for p in u])
return data, ui
def select_xychunksize(wcs, halfpsfsize=36./3600.):
"""
get wcs and find wcs pixel size of psf reach
"""
sizex = int(abs(halfpsfsize/wcs.wcs.cdelt[1])) + 2
sizey = int(abs(halfpsfsize/wcs.wcs.cdelt[0])) + 2
print(sizex, sizey)
return sizex, sizey
def read_wcs(h):
"""
read events wcs header
"""
w = WCS(naxis=2)
w.wcs.ctype = [h["TCTYP11"], h["TCTYP12"]]
w.wcs.crval = [h["TCRVL11"], h["TCRVL12"]]
w.wcs.cdelt = [h["TCDLT11"], h["TCDLT12"]]
w.wcs.crpix = [h["TCRPX11"], h["TCRPX12"]]
w = WCS(w.to_header())
return w
def create_neighboring_blocks(x, y, sizex, sizey):
"""
schematically all sky is splitted on squares, which are approximatelly ~ 10 times greater then the psf
events for corresponding square are joined :: squer + diluttaion of psf reach
coordinate system with events and all required coefficiets are fed to psf solver
current psf size is 25*0.5 arcsec (with up to \sqrt(2) factor in case of worst rolls -> 36''
"""
"""
event list already contains x and y for each event
"""
iix = (x//sizex + 0.5).astype(int)
iiy = (y//sizey + 0.5).astype(int)
isx, isy = np.mgrid[-1:2:1, -1:2:1]
oidx = np.repeat(np.arange(x.size), 9)
xyu, iixy, xyc = np.unique(np.array([np.repeat(iix, 9) + np.tile(isx.ravel(), x.size),
np.repeat(iiy, 9)+ np.tile(isy.ravel(), x.size)]), axis=1, return_counts=True, return_inverse=True)
sord = np.argsort(iixy)
return oidx[sord], xyu, xyc
def make_srccount_and_detmap(emap, evt, h, wcs=None):
psfdata, ui = prepare_psf(evt)
if wcs is None:
wcs = read_wcs(h)
x, y = evt["x"], evt["y"]
else:
ewcs = read_wcs(h)
x, y = wcs.all_world2pix(ewcs.all_pix2world(np.array([x, y]).T, 0), 0).T
eidx = np.searchsorted(psfe*1e3, evt["ENERGY"])
eidx = np.maximum((evt["ENERGY"]/1000. - psfe[eidx])/(psfe[eidx + 1] - psfe[eidx]), 0.)
sizex, sizey = select_xychunksize(wcs)
iidx, xyu, cts = create_neighboring_blocks(x, y, sizex, sizey)
cc = np.zeros(cts.size + 1, int)
cc[1:] = np.cumsum(cts)
cmap, pmap = np.zeros(emap.shape, float), np.zeros(emap.shape, float)
#xe, ye, pk, roll, psfi = np.copy(evt["x"][iidx]), np.copy(evt["y"][iidx]), np.copy((evt["quant_eff"]/evt["bkg_model"])[iidx]), np.copy(evt["roll_pnt"][iidx]), np.copy(ui[iidx])
xe = np.copy(x[iidx]).astype(float)
ye = np.copy(y[iidx]).astype(float)
ee = np.copy(eidx[iidx]).astype(float)
pk = np.copy(evt["src_spec"][iidx]/evt["bkg_spec"][iidx]).astype(float)
roll = np.copy(np.deg2rad(evt["roll_pnt"][iidx])).astype(float)
psfi = np.copy(ui[iidx])
yg, xg = np.mgrid[0:sizey:1, 0:sizex:1]
def worker(ixys):
i, (xs, ys) = ixys
eloc = emap[ys*sizey:ys*sizey+sizey, xs*sizex:xs*sizex+sizex]
mask = eloc > 0.
xl = (xg[mask] + xs*sizex).astype(float)
yl = (yg[mask] + ys*sizey).astype(float)
ell = (eloc[mask]).astype(float)
if np.any(mask):
cr, pr = solve_for_locations_eintp(psfi[cc[i]:cc[i+1]], ee[cc[i]:cc[i + 1]], xe[cc[i]:cc[i+1]], ye[cc[i]:cc[i+1]], roll[cc[i]:cc[i+1]], pk[cc[i]:cc[i+1]], xl, yl, ell, psfdata)
else:
xl, yl, cr, pr = np.empty(0, int),np.empty(0, int),np.empty(0, float),np.empty(0, float)
return xl.astype(int), yl.astype(int), cr, pr
tpool = ThreadPool(8)
for xl, yl, cr, pr in tqdm.tqdm(tpool.imap_unordered(worker, enumerate(xyu.T)), total=xyu.shape[1]):
cmap[yl, xl] = cr
pmap[yl, xl] = pr
return wcs, cmap, pmap
if __name__ == "__main__":
p1 = fits.open("test.fits")
#emap = fits.getdata("exp.map.gz") #np.full((8192, 8192), 10000.)
emap = fits.getdata("eR_spec_asp_0.fits.gz") #np.full((8192, 8192), 10000.)
wcs, cmap, pmap = make_srccount_and_detmap(emap, p1[1].data, p1[1].header)
fits.HDUList([fits.PrimaryHDU(), fits.ImageHDU(pmap - cmap, header=p1[1].header), fits.ImageHDU(cmap, header=p1[1].header)]).writeto("tmap4.fits.gz", overwrite=True)
#fits.ImageHDU(data=pmap, header=wcs.to_header()).writeto("tmap4.fits.gz", overwrite=True)