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authorAaron LI <aly@aaronly.me>2017-08-18 12:12:49 +0800
committerAaron LI <aly@aaronly.me>2017-08-18 12:13:39 +0800
commit4858d2775f69e3c2c569ceaa9d8aa48071bd6102 (patch)
treeec9b5d30ff9f4debeb5eaf6b20f308c16856e976 /astro
parent8a93c569256e4b639ae82292d13d3b20b1dc804c (diff)
downloadatoolbox-4858d2775f69e3c2c569ceaa9d8aa48071bd6102.tar.bz2
get_slice_zfreq.py: Rewrite to work with "make_lightcone.py"
Diffstat (limited to 'astro')
-rwxr-xr-xastro/21cm/get_slice_zfreq.py142
-rwxr-xr-xastro/21cm/make_lightcone.py2
2 files changed, 83 insertions, 61 deletions
diff --git a/astro/21cm/get_slice_zfreq.py b/astro/21cm/get_slice_zfreq.py
index cd3dd39..161b714 100755
--- a/astro/21cm/get_slice_zfreq.py
+++ b/astro/21cm/get_slice_zfreq.py
@@ -5,78 +5,118 @@
#
"""
-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.
+Get the slices at the specified redshifts/frequencies from the HI
+light-cone cube (created by `make_lightcone.py`), and use linear
+interpolation.
"""
-import os
import sys
import argparse
+import logging
+from datetime import datetime, timezone
import numpy as np
from astropy.io import fits
-from astropy.wcs import WCS
+from astropy.cosmology import FlatLambdaCDM
from z2freq import z2freq, freq2z
-class FITSCube:
+logging.basicConfig(level=logging.INFO)
+logger = logging.getLogger()
+
+cosmo = FlatLambdaCDM(H0=71, Om0=0.27)
+
+
+class LightCone:
+ """
+ Light-cone cube mimic the observation of HI signal.
+ """
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)
+ logger.info("Loaded light-cone cube: %dx%d (cells) * %d (slices)" %
+ (self.Nside, self.Nside, self.Nslice))
@property
- def nslice(self):
+ 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 Nside(self):
+ return self.header["Nside"]
+
+ @property
+ def slices_Dc(self):
+ """
+ The comoving distances of each slice in the light-cone cube.
+ The slices are evenly distributed along the LoS with equal
+ comoving step. [Mpc]
+ """
+ Dc_step = self.header["Dc_step"]
+ Dc_min = self.header["Dc_min"]
+ Dc = np.array([Dc_min + Dc_step*i for i in range(self.Nslice)])
+ return Dc
def get_slice(self, z):
- redshifts = self.redshifts
- if z < redshifts.min() or z > redshifts.max():
+ Dc = cosmo.comoving_distance(z).value # [Mpc]
+ slices_Dc = self.slices_Dc
+ if Dc < slices_Dc.min() or Dc > slices_Dc.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)
+
+ i2 = (slices_Dc <= Dc).sum()
+ i1 = i2 - 1
+ Dc1, s1 = slices_Dc[i1], self.data[i1, :, :]
+ Dc2, s2 = slices_Dc[i2], self.data[i2, :, :]
+ slope = (s2 - s1) / (Dc2 - Dc1)
+ return s1 + slope * (Dc - Dc1)
+
+ def write_slice(self, outfile, data, z, clobber=False):
+ freq = z2freq(z)
+ Dc = cosmo.comoving_distance(z).value # [Mpc]
+ header = fits.Header()
+ header["BUNIT"] = (self.header["BUNIT"],
+ self.header.comments["BUNIT"])
+ header["Lside"] = (self.header["Lside"],
+ self.header.comments["Lside"])
+ header["Nside"] = (self.header["Nside"],
+ self.header.comments["Lside"])
+ header["REDSHIFT"] = (z, "redshift of this slice")
+ header["FREQ"] = (freq, "[MHz] observed HI signal frequency")
+ header["Dc"] = (Dc, "[cMpc] comoving distance")
+ header["DATE"] = (datetime.now(timezone.utc).astimezone().isoformat(),
+ "File creation date")
+ header.add_history(" ".join(sys.argv))
+ hdu = fits.PrimaryHDU(data=data, header=header)
+ try:
+ hdu.writeto(outfile, overwrite=clobber)
+ except TypeError:
+ hdu.writeto(outfile, clobber=clobber)
+ logger.info("Wrote slice to file: %s" % outfile)
def main():
- outfile_default = "{prefix}_f{freq:06.2f}_z{z:06.3f}.fits"
+ outfile_pattern = "{prefix}_f{freq:06.2f}_z{z:06.3f}.fits"
+ outfile_prefix = "deltaTb"
parser = argparse.ArgumentParser(
- description="Get slices at requested redshifts/frequencies")
+ description="Get slices at requested redshifts/frequencies " +
+ "from light-cone cube")
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")
+ help="input light-cone 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")
+ default=outfile_pattern,
+ help="output image slice filename pattern FITS " +
+ "(default: %s)" % outfile_pattern)
+ parser.add_argument("-p", "--prefix", dest="prefix",
+ default=outfile_prefix,
+ help="prefix of output slices (default: %s)" %
+ outfile_prefix)
exgrp = parser.add_mutually_exclusive_group(required=True)
exgrp.add_argument("-z", "--redshifts", dest="redshifts", nargs="+",
help="redshifts where to interpolate slices")
@@ -91,30 +131,12 @@ def main():
freqs = [float(f) for f in args.freqs]
redshifts = freq2z(freqs, print_=False)
- cube = FITSCube(args.infile)
+ lightcone = LightCone(args.infile)
for z, f in zip(redshifts, freqs):
outfile = args.outfile.format(prefix=args.prefix, z=z, freq=f)
- print("z=%06.3f, freq=%06.2f MHz : %s" % (z, f, outfile))
- zslice = cube.get_slice(z)
- header = fits.Header()
- try:
- header["BUNIT"] = (cube.header["BUNIT"],
- cube.header.comments["BUNIT"])
- except KeyError:
- pass
- try:
- header["LSIDE"] = (cube.header["LSIDE"],
- cube.header.comments["LSIDE"])
- except KeyError:
- pass
- 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)
+ logger.info("z=%06.3f, freq=%06.2f MHz : %s ..." % (z, f, outfile))
+ data = lightcone.get_slice(z)
+ lightcone.write_slice(outfile, data=data, z=z, clobber=args.clobber)
if __name__ == "__main__":
diff --git a/astro/21cm/make_lightcone.py b/astro/21cm/make_lightcone.py
index 1e888d0..a17c217 100755
--- a/astro/21cm/make_lightcone.py
+++ b/astro/21cm/make_lightcone.py
@@ -260,7 +260,7 @@ class LightCone:
@property
def header(self):
- dDc = self.configs.Lside / self.configs.Nside
+ dDc = self.configs.Dc_cell
Dc_min, Dc_max = self.configs.Dc_limit
header = fits.Header()
header["BUNIT"] = (self.configs.unit, "Data unit")