From fa8208c993f5d74e67f506ed963b33bf4342401d Mon Sep 17 00:00:00 2001 From: Aaron LI Date: Sun, 11 Jun 2017 20:07:11 +0800 Subject: Add astro/21cm/get_slice_zfreq.py --- astro/21cm/get_slice_zfreq.py | 112 ++++++++++++++++++++++++++++++++++++++++++ 1 file changed, 112 insertions(+) create mode 100755 astro/21cm/get_slice_zfreq.py (limited to 'astro/21cm/get_slice_zfreq.py') diff --git a/astro/21cm/get_slice_zfreq.py b/astro/21cm/get_slice_zfreq.py new file mode 100755 index 0000000..c67d513 --- /dev/null +++ b/astro/21cm/get_slice_zfreq.py @@ -0,0 +1,112 @@ +#!/usr/bin/env python3 +# +# Copyright (c) 2017 Weitian LI +# MIT License +# + +""" +Get the slice of the specified redshift/frequency (21cm signal) from +the redshift cube (created by `extract_slice.py` and `fitscube.py`) +using linear interpolation in redshift. + +NOTE: +The cube slices are ordered in increasing redshifts. +""" + +import os +import sys +import argparse + +import numpy as np +from astropy.io import fits +from astropy.wcs import WCS + +from z2freq import z2freq, freq2z + + +class FITSCube: + def __init__(self, infile): + with fits.open(infile) as f: + self.data = f[0].data + self.header = f[0].header + self.wcs = WCS(self.header) + + @property + def nslice(self): + ns, __, __ = self.data.shape + return ns + + @property + def redshifts(self): + # Z-axis + nslice = self.nslice + pix = np.zeros(shape=(nslice, 3), dtype=np.int) + pix[:, 2] = np.arange(nslice) + world = self.wcs.wcs_pix2world(pix, 0) + return world[:, 2] + + def get_slice(self, z): + redshifts = self.redshifts + if z < redshifts.min() or z > redshifts.max(): + raise ValueError("requested redshift out of range: %.2f" % z) + idx2 = (redshifts <= z).sum() + idx1 = idx2 - 1 + z1, slice1 = redshifts[idx1], self.data[idx1, :, :] + z2, slice2 = redshifts[idx2], self.data[idx2, :, :] + if os.environ.get("DEBUG"): + print("DEBUG: redshifts: {0}".format(redshifts), file=sys.stderr) + print("DEBUG: z={0}".format(z), file=sys.stderr) + print("DEBUG: z1={0}, idx1={1}".format(z1, idx1), file=sys.stderr) + print("DEBUG: z2={0}, idx2={1}".format(z2, idx2), file=sys.stderr) + return slice1 + (slice2-slice1) * (z-z1) / (z2-z1) + + +def main(): + outfile_default = "{prefix}_z{z:05.2f}_f{freq:06.2f}.fits" + + parser = argparse.ArgumentParser( + description="Get slices at requested redshifts/frequencies") + parser.add_argument("-C", "--clobber", dest="clobber", + action="store_true", + help="overwrite existing files") + parser.add_argument("-i", "--infile", dest="infile", required=True, + help="input redshift data cube") + parser.add_argument("-o", "--outfile", dest="outfile", + default=outfile_default, + help="output FITS image slice (default: %s)" % + outfile_default) + parser.add_argument("-p", "--prefix", dest="prefix", required=True, + help="prefix for the output FITS image") + exgrp = parser.add_mutually_exclusive_group(required=True) + exgrp.add_argument("-z", "--redshifts", dest="redshifts", nargs="+", + help="redshifts where to interpolate slices") + exgrp.add_argument("-f", "--freqs", dest="freqs", nargs="+", + help="21cm frequencies [MHz] to interpolate slices") + args = parser.parse_args() + + if args.redshifts: + redshifts = [float(z) for z in args.redshifts] + freqs = z2freq(redshifts, print_=False) + else: + freqs = [float(f) for f in args.freqs] + redshifts = freq2z(freqs, print_=False) + + cube = FITSCube(args.infile) + for z, f in zip(redshifts, freqs): + outfile = args.outfile.format(prefix=args.prefix, z=z, freq=f) + print("z=%05.2f, freq=%06.2f MHz : %s" % (z, f, outfile)) + zslice = cube.get_slice(z) + header = fits.Header() + header["BUNIT"] = cube.header.get("BUNIT") + header["REDSHIFT"] = (z, "Slice where interpolated") + header["FREQ"] = (f, "21cm signal frequency [MHz]") + header.add_history(" ".join(sys.argv)) + hdu = fits.PrimaryHDU(data=zslice, header=header) + try: + hdu.writeto(outfile, overwrite=args.clobber) + except TypeError: + hdu.writeto(outfile, clobber=args.clobber) + + +if __name__ == "__main__": + main() -- cgit v1.2.2