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author | Aaron LI <aly@aaronly.me> | 2017-12-12 14:07:29 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-12-12 14:07:29 +0800 |
commit | 26dfdb16d9ff943084da0b21a8a1be1be0b80ead (patch) | |
tree | f32a7d8dfc982df1786c37c52d754723d3a73f70 /astro/suzaku | |
parent | 48923e3afd3b8ee049b199d352e2912dceca5476 (diff) | |
download | atoolbox-26dfdb16d9ff943084da0b21a8a1be1be0b80ead.tar.bz2 |
Add astro/suzaku/make_photon_list.py: implement ``mkphlist`` for suzaku simulation
Diffstat (limited to 'astro/suzaku')
-rwxr-xr-x | astro/suzaku/make_photon_list.py | 390 |
1 files changed, 390 insertions, 0 deletions
diff --git a/astro/suzaku/make_photon_list.py b/astro/suzaku/make_photon_list.py new file mode 100755 index 0000000..d8fe679 --- /dev/null +++ b/astro/suzaku/make_photon_list.py @@ -0,0 +1,390 @@ +#!/usr/bin/env python3 +# +# Copyright (c) 2017 Weitian LI <weitian@aaronly.me> +# MIT License +# + +""" +Make/simulate the X-ray photon list from the object's image and +spectral models. + +The simulated X-ray photon list will be used to simulate the +Suzaku event observation by ``xissim`` tool. + +This script is intended to replace and extend the abilities of the +``mkphlist`` tool. + +NOTE +---- +The environment variable ``HEADAS`` should be set in order to help +locate the ``PyXspec`` module and XSPEC shared libraries. + +References +---------- +* mkphlist: https://heasarc.gsfc.nasa.gov/lheasoft/ftools/headas/mkphlist.txt +* xissim: https://heasarc.gsfc.nasa.gov/lheasoft/ftools/headas/xissim.txt +* PyXspec: https://heasarc.gsfc.nasa.gov/xanadu/xspec/python/html/index.html + +Example Configuration File +----------------------------------------------------------------------- +# image to determine the photon counts distribution +image: imgbox800_e500-7000_sm.fits +# region (annuli below) center; in "image" coordinate +center: [400, 399] +nh: 0.03 # 1e22 [cm^-2] +redshift: 0.0137 +# simulated photon energy range [keV] +erange: [0.3, 10.0] +# number of energy bins (logarithmic) +ebins: 1000 +# total photon counts that will be generated +counts: 300000 +# exposure [ks] +exposure: 50 +# a set of annular regions, with several pie regions inside each +# annulus; each pie region can have a different spectral model. +regions: + # annulus 1, with 3 pies + - radius: [0, 100] + angle: [0, 120, 200] + temperature: [1.0, 1.5, 2.0] + abundance: [0.5, 1.0, 1.5] + weight: [1, 2, 1.5] + # annulus 2, with 3 pies + - radius: [100, 200] + angle: [0, 90, 250] + temperature: [0.5, 1.0, 1.5] + abundance: [1.5, 2.0, 1.0] + weight: [0.5, 1, 1.5] + # annulus 3, with 4 pies + - radius: [200, 400] + angle: [50, 150, 220, 300] + temperature: [0.8, 1.2, 1.5, 1.3] + abundance: [1.1, 2.0, 1.5, 1.2] + weight: [0.2, 1.5, 0.7, 2] +clobber: True +outfiles: + photons_table: photons.fits + counts_map: counts_map.fits + temperature_map: temperature_map.fits + abundance_map: abundance_map.fits +----------------------------------------------------------------------- +""" + +import os +import sys + +try: + headas = os.environ["HEADAS"] + healib = os.path.join(headas, "lib") +except KeyError: + raise ValueError("env variable 'HEADAS' not set") + +if ("LD_LIBRARY_PATH" not in os.environ) or ( + os.environ["LD_LIBRARY_PATH"].find(healib) < 0): + os.environ["LD_LIBRARY_PATH"] = ":".join([ + healib, os.environ.get("LD_LIBRARY_PATH", "") + ]) + try: + # Hack the ``LD_LIBRARY_PATH`` to import Xspec + # Credit: https://stackoverflow.com/a/25457751/4856091 + print("sys.argv:", sys.argv) + os.execv(sys.argv[0], sys.argv) + except Exception: + print("ERROR: failed to re-exec with new LD_LIBRARY_PATH") + raise + +sys.path.append(os.path.join(healib, "python")) +import xspec +print("Imported XSPEC!") + +import argparse +import logging +from pprint import pprint + +import yaml +import numpy as np +from astropy.io import fits +from astropy.wcs import WCS + + +logging.basicConfig(level=logging.INFO, + format="[%(levelname)s:%(lineno)d] %(message)s") +logger = logging.getLogger() + + +class Pie: + """ + Pie region + """ + def __init__(self, xc, yc, rin, rout, abegin, aend): + self.xc = xc + self.yc = yc + self.rin = rin + self.rout = rout + self.abegin = abegin # [deg] beginning angle + self.aend = aend # [deg] ending angle (may be > 360) + # spectral model parameters + self._modelpars = {} + + @staticmethod + def cart2pol(x, y): + rho = np.sqrt(x**2 + y**2) + phi = 180 + np.rad2deg(np.arctan2(y, x)) # 0-360 [deg] + return (rho, phi) + + def make_mask(self, shape): + try: + nrow, ncol = shape + except TypeError: + nrow = ncol = shape + # HACK: to make the masks consistent with ``rand_position()`` + ix = self.xc - np.arange(ncol) + iy = self.yc - np.arange(nrow) + mx, my = np.meshgrid(ix, iy) + rho, phi = self.cart2pol(mx, my) + mask_rho = (rho >= self.rin) & (rho <= self.rout) + mask_phi = (phi >= self.abegin) & (phi <= self.aend) + if self.aend > 360: + mask_phi |= (phi <= (self.aend-360)) + mask = mask_rho & mask_phi + return mask + + def rand_position(self, n=None): + if n is None: + n = self.modelpar("counts") + theta = np.random.uniform(low=self.abegin, high=self.aend, size=n) + r = np.sqrt(np.random.uniform(low=self.rin**2, high=self.rout**2, + size=n)) + x = r * np.cos(np.deg2rad(theta)) + self.xc + y = r * np.sin(np.deg2rad(theta)) + self.yc + return (x, y) + + def modelpar(self, key=None, value=None): + if key is None: + return self._modelpars + elif value is None: + return self._modelpars.get(key) + else: + self._modelpars[key] = value + + def set_model(self, nh, redshift): + model = xspec.Model("wabs*apec") + model.wabs.nH = nh + model.apec.Redshift = redshift + model.apec.kT = self.modelpar("temperature") + model.apec.Abundanc = self.modelpar("abundance") + self._model = model + + def rand_photons(self, n=None): + if n is None: + n = self.modelpar("counts") + model = self._model + mvalues = np.array(model.values(0), dtype=float) # len: ebins + p = mvalues / mvalues.sum() + menergies = np.array(model.energies(0), dtype=float) # len: ebins+1 + mebins = np.sqrt(menergies[1:] * menergies[:-1]) + photons = np.random.choice(mebins, size=n, p=p) + return photons # [keV] + + +class Regions: + """ + Configured regions + """ + def __init__(self, configs): + self.configs = configs + self.xc, self.yc = configs["center"] + + @property + def rmax(self): + rmax = 0 + for annulus in self.configs["regions"]: + rin, rout = annulus["radius"] + if rmax < rout: + rmax = rout + return rmax + + def make_mask(self, shape): + try: + nrow, ncol = shape + except TypeError: + nrow = ncol = shape + ix = np.arange(ncol) - self.xc + iy = np.arange(nrow) - self.yc + mx, my = np.meshgrid(ix, iy) + rho = np.sqrt(mx**2 + my**2) + mask = (rho <= self.rmax) + return mask + + @property + def regions(self): + reg_all = [] + for annulus in self.configs["regions"]: + reg_annulus = [] + rin, rout = annulus["radius"] + abegin = annulus["angle"] + aend = abegin[1:] + [abegin[0]+360] + npie = len(abegin) + temperature = annulus["temperature"] + abundance = annulus["abundance"] + weight = annulus.get("weight", [1]*npie) + for i in range(npie): + pie = Pie(xc=self.xc, yc=self.yc, rin=rin, rout=rout, + abegin=abegin[i], aend=aend[i]) + pie.modelpar("temperature", temperature[i]) + pie.modelpar("abundance", abundance[i]) + pie.modelpar("weight", weight[i]) + reg_annulus.append(pie) + reg_all.append(reg_annulus) + return reg_all + + +def pixel2world(x, y, wcs): + pix = np.column_stack([x, y]) + world = wcs.wcs_pix2world(pix, 0) + ra = world[:, 0] + dec = world[:, 1] + return (ra, dec) # [deg] + + +def main(): + parser = argparse.ArgumentParser( + description="Make/simulate X-ray photon list for Suzaku simulation") + parser.add_argument("config", help="configuration file in YAML format") + args = parser.parse_args() + + configs = yaml.load(open(args.config)) + logger.info("Load configuration file: %s" % args.config) + logger.info("Configurations:") + pprint(configs) + + # Update XSPEC settings + emin, emax = configs["erange"] # [keV] + ebins = configs["ebins"] + xspec.AllModels.setEnergies("%.1f %.1f %d log" % (emin, emax, ebins)) + logger.info("Energy range: [%.1f, %.1f] [keV]" % (emin, emax)) + logger.info("Energy: %d logarithmic channels" % ebins) + + with fits.open(configs["image"]) as f: + header = f[0].header + image = f[0].data + shape = image.shape + logger.info("Image size: %dx%d" % (shape[1], shape[0])) + + wcs = WCS(header) + regions = Regions(configs) + reg_all = regions.regions + mask_all = regions.make_mask(shape=shape) + weight_all = np.sum(image[mask_all]) + + counts_all = configs["counts"] + logger.info("Total counts: %d" % counts_all) + + logger.info("nH: %.4f [1e22 cm^-2]" % configs["nh"]) + logger.info("Redshift: %.5f" % configs["redshift"]) + exposure = configs["exposure"] * 1e3 # [s] + logger.info("Exposure time: %.1f [s]" % exposure) + + logger.info("Determining photons counts in each region ...") + counts_sum = 0 + for i, annulus in enumerate(reg_all): + for j, pie in enumerate(annulus): + label = "annu#%d/pie#%d" % (i+1, j+1) + mask = pie.make_mask(shape=shape) + pixels = np.sum(mask) + weight = np.sum(image[mask]) * pie.modelpar("weight") + counts = int(counts_all * weight / weight_all) + counts_sum += counts + pie.modelpar("pixels", pixels) + pie.modelpar("counts", counts) + logger.info("%s: %d pixels, %d photons" % (label, pixels, counts)) + + logger.info("Determined counts sum: %d" % counts_sum) + logger.info("Adjusting total counts -> %d" % counts_all) + for i, annulus in enumerate(reg_all): + for j, pie in enumerate(annulus): + label = "annu#%d/pie#%d" % (i+1, j+1) + counts_old = pie.modelpar("counts") + counts_new = round(counts_old * counts_all / counts_sum) + pie.modelpar("counts", counts_new) + logger.info("%s: adjusted photon counts: %d -> %d" % + (label, counts_old, counts_new)) + + # Output files + temp_map = np.zeros_like(image) + abund_map = np.zeros_like(image) + counts_map = np.zeros_like(image) + weights_map = np.zeros_like(image) + photonlist = [] + + for i, annulus in enumerate(reg_all): + for j, pie in enumerate(annulus): + label = "annu#%d/pie#%d" % (i+1, j+1) + pie.set_model(nh=configs["nh"], redshift=configs["redshift"]) + mask = pie.make_mask(shape=shape) + temp = pie.modelpar("temperature") + abund = pie.modelpar("abundance") + counts = pie.modelpar("counts") + logger.info("%s: kT=%.2f, Z=%.2f, %d photons" % + (label, temp, abund, counts)) + + logger.info("%s: sampling photon positions ..." % label) + x, y = pie.rand_position(n=counts) + ra, dec = pixel2world(x, y, wcs=wcs) + logger.info("%s: sampling photon energies ..." % label) + energies = pie.rand_photons(n=counts) + time = np.random.uniform(low=0, high=exposure, size=counts) + photons = np.column_stack([time, energies, ra, dec]) + photonlist.append(photons) + + logger.info("%s: spatially binning photons ..." % label) + rbins = np.arange(shape[0]+1, dtype=int) + cbins = np.arange(shape[1]+1, dtype=int) + hist2d, __, __ = np.histogram2d(y, x, bins=(rbins, cbins)) + counts_map += hist2d + + temp_map[mask] = temp + abund_map[mask] = abund + weights_map[mask] = pie.modelpar("weight") + + logger.info("Creating output FITS header ...") + header_out = fits.Header() + header_out.extend(wcs.to_header(), update=True) + header_out["CREATOR"] = os.path.basename(sys.argv[0]) + header_out.add_history(" ".join(sys.argv)) + logger.info("Creating photons table ...") + photons = np.row_stack(photonlist) + photons.sort(axis=0) # sort by time in place + hdu = fits.BinTableHDU.from_columns([ + fits.Column(name="PHOTON_TIME", format="D", unit="s", + array=photons[:, 0]), + fits.Column(name="PHOTON_ENERGY", format="E", unit="keV", + array=photons[:, 1]), + fits.Column(name="RA", format="E", unit="deg", array=photons[:, 2]), + fits.Column(name="DEC", format="E", unit="deg", array=photons[:, 3]), + ], header=header_out) + hdu.name = "PHOTON_LIST" + outfile = configs["outfiles"]["photons_table"] + hdu.writeto(outfile, overwrite=configs["clobber"]) + logger.info("Wrote photons table to: %s" % outfile) + + data = np.stack([counts_map, weights_map], axis=0) + hdu = fits.PrimaryHDU(data=data, header=header_out) + outfile = configs["outfiles"]["counts_map"] + hdu.writeto(outfile, overwrite=configs["clobber"]) + logger.info("Wrote counts/weights map to: %s" % outfile) + # + hdu = fits.PrimaryHDU(data=temp_map, header=header_out) + outfile = configs["outfiles"]["temperature_map"] + hdu.writeto(outfile, overwrite=configs["clobber"]) + logger.info("Wrote temperature map to: %s" % outfile) + # + hdu = fits.PrimaryHDU(data=abund_map, header=header_out) + outfile = configs["outfiles"]["abundance_map"] + hdu.writeto(outfile, overwrite=configs["clobber"]) + logger.info("Wrote abundance map to: %s" % outfile) + + +if __name__ == "__main__": + main() |