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authorAaron LI <aly@aaronly.me>2017-11-04 22:28:40 +0800
committerAaron LI <aly@aaronly.me>2017-11-04 22:28:40 +0800
commitc5ba47499baa00c11f0f51e71720b24ac1ffc6d3 (patch)
tree3945531272a21b6ce757c6d280d42144c531d507 /astro
parent30dad264ec305433dd661834addbb1e8b1345af8 (diff)
downloadatoolbox-c5ba47499baa00c11f0f51e71720b24ac1ffc6d3.tar.bz2
astro/ps2d.py: Add get_pixelsize(); and improve get_frequencies()
Diffstat (limited to 'astro')
-rwxr-xr-xastro/ps2d.py51
1 files changed, 36 insertions, 15 deletions
diff --git a/astro/ps2d.py b/astro/ps2d.py
index b5b76dc..f7c9801 100755
--- a/astro/ps2d.py
+++ b/astro/ps2d.py
@@ -39,7 +39,6 @@ import numpy as np
from scipy import fftpack
from scipy import signal
from astropy.io import fits
-from astropy.wcs import WCS
from astropy.cosmology import FlatLambdaCDM
import astropy.constants as ac
@@ -64,19 +63,41 @@ OmegaM0 = 0.27
cosmo = FlatLambdaCDM(H0=H0, Om0=OmegaM0)
-@lru_cache()
def freq2z(freq):
z = freq21cm / freq - 1.0
return z
-@lru_cache()
-def get_frequencies(wcs, nfreq):
- pix = np.zeros(shape=(nfreq, 3), dtype=int)
- pix[:, -1] = np.arange(nfreq)
- world = wcs.wcs_pix2world(pix, 0)
- freqMHz = world[:, -1] / 1e6
- return freqMHz
+def get_frequencies(header):
+ """
+ Get the frequencies for each cube slice.
+ Unit: [MHz]
+ """
+ nfreq = header["NAXIS3"]
+ freq0 = header["CRVAL3"] # [Hz]
+ freqstep = header["CDELT3"] # [Hz]
+ frequencies = freq0 + freqstep*np.arange(nfreq)
+ return frequencies / 1e6 # [MHz]
+
+
+def get_pixelsize(header):
+ """
+ Get the pixel size of cube image.
+ Unit: [arcsec]
+ """
+ try:
+ pixelsize = header["PixSize"] # [arcsec]
+ except KeyError:
+ try:
+ pixelsize = header["CDELT1"] # [deg]
+ if abs(pixelsize-1.0) < 1e-8:
+ # Place-holder value set by ``fitscube.py``
+ pixelsize = None
+ else:
+ pixelsize = abs(pixelsize)*3600 # [arcsec]
+ except KeyError:
+ pixelsize = None
+ return pixelsize
class PS2D:
@@ -508,8 +529,8 @@ def main():
action="store_true",
help="plot the 2D power spectrum and save")
parser.add_argument("-p", "--pixelsize", dest="pixelsize", type=float,
- help="spatial pixel size [arcsec] (default: " +
- "obtain from FITS header WCS info)")
+ help="spatial pixel size [arcsec] (required " +
+ "if cannot obtain from FITS header)")
parser.add_argument("-w", "--window", dest="window",
choices=["nuttall"],
help="apply window along frequency axis " +
@@ -544,13 +565,13 @@ def main():
else:
raise ValueError("cube has different unit: %s" % bunit2)
- wcs = WCS(header)
- nfreq = cube.shape[0]
- frequencies = get_frequencies(wcs, nfreq)
+ frequencies = get_frequencies(header)
if args.pixelsize:
pixelsize = args.pixelsize # [arcsec]
else:
- pixelsize = abs(wcs.wcs.cdelt[0]) * 3600 # [deg] -> [arcsec]
+ pixelsize = get_pixelsize(header)
+ if pixelsize is None:
+ raise RuntimeError("--pixelsize required")
ps2d = PS2D(cube=cube, pixelsize=pixelsize, frequencies=frequencies,
meanstd=args.meanstd, unit=bunit,