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author | Aaron LI <aly@aaronly.me> | 2017-11-04 22:28:40 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-11-04 22:28:40 +0800 |
commit | c5ba47499baa00c11f0f51e71720b24ac1ffc6d3 (patch) | |
tree | 3945531272a21b6ce757c6d280d42144c531d507 /astro | |
parent | 30dad264ec305433dd661834addbb1e8b1345af8 (diff) | |
download | atoolbox-c5ba47499baa00c11f0f51e71720b24ac1ffc6d3.tar.bz2 |
astro/ps2d.py: Add get_pixelsize(); and improve get_frequencies()
Diffstat (limited to 'astro')
-rwxr-xr-x | astro/ps2d.py | 51 |
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, |