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authorAaron LI <aly@aaronly.me>2017-11-21 22:02:51 +0800
committerAaron LI <aly@aaronly.me>2017-11-21 22:06:30 +0800
commit9b7ca9c1885d2458034b4d90a8e8658ce231e880 (patch)
tree7f4947e28f29f71e8d2d3ad82ed1743978ed306b /astro
parentb97f35bfce69a4d5b6da3a95814812c5c3c8411f (diff)
downloadatoolbox-9b7ca9c1885d2458034b4d90a8e8658ce231e880.tar.bz2
astro/jybeam2k.py: Derive beam size using 'WSCNORMF' by default
* Add argument --use-fitted-beam to force to use the fitted beam * Change argument --beam to --beam-size
Diffstat (limited to 'astro')
-rwxr-xr-xastro/oskar/jybeam2k.py54
1 files changed, 45 insertions, 9 deletions
diff --git a/astro/oskar/jybeam2k.py b/astro/oskar/jybeam2k.py
index 0f774c1..6413069 100755
--- a/astro/oskar/jybeam2k.py
+++ b/astro/oskar/jybeam2k.py
@@ -42,16 +42,49 @@ def open_image(infile):
return (header, data)
+def calc_beam_size(header):
+ """
+ Calculate the beam/PSF size using the 'WSCNORMF' keyword recorded by
+ the WSClean imager, which applies to the natural-weighted image, and
+ is more accurate than the fitted beam (stored as 'BMAJ' and 'BMIN'.)
+ """
+ try:
+ weight = header["WSCWEIGH"]
+ normf = header["WSCNORMF"]
+ print("WSCWEIGH: %s" % weight)
+ print("WSCNORMF: %.1f" % normf)
+ except KeyError:
+ raise RuntimeError("NO necessary WSC* keyword; switch to " +
+ "--use-fitted-beam instead")
+ if weight.upper() != "NATURAL":
+ print("WARNING: weighting scheme is '%s' != natural!" % weight)
+ width = header["NAXIS1"]
+ height = header["NAXIS2"]
+ pixelsize = np.abs(header["CDELT1"]) * 3600 # [arcsec]
+ print("Image: %dx%d, %.1f [arcsec/pixel]" % (width, height, pixelsize))
+ beam_size = (width*height * pixelsize**2) / normf
+ return beam_size
+
+
def main():
parser = argparse.ArgumentParser(
- description="Convert image unit from [Jy/beam] to [K]")
+ description="Convert WSClean created image from [Jy/beam] to [K]",
+ epilog=("By default the 'WSCNORMF' keyword is taken to derive " +
+ "the beam/PSF size for natural-weighted image created " +
+ "by WSClean, which is more accurate than the fitted " +
+ "beam stored as 'BMAJ' and 'BMIN'."))
parser.add_argument("-C", "--clobber", dest="clobber",
action="store_true",
help="overwrite existing output file")
- parser.add_argument("-b", "--beam", dest="beam", type=float,
+ parser.add_argument("-B", "--use-fitted-beam", dest="use_fitted_beam",
+ action="store_true",
+ help="use the fitted beam (i.e., BMAJ and BMIN) " +
+ "or the beam size specified by --beam-size.")
+ parser.add_argument("-b", "--beam-size", dest="beam_size", type=float,
help="instrumental beam size [arcsec^2] " +
"(=pi*bmajor*bminor/4/ln(2)) (default: obtain " +
- "from the header BMAJ and BMIN keywords)")
+ "from the header BMAJ and BMIN keywords); this " +
+ "argument also implies --use-fitted-beam")
parser.add_argument("-f", "--frequency", dest="frequency",
help="frequency [MHz] of the input image (NOTE: " +
"required if failed to obtain from the header)")
@@ -85,16 +118,19 @@ def main():
print("Frequency: %.2f [MHz]" % freq)
# Elliptical Gaussian beam (full width at half power; FWHP)
- if args.beam:
- beam = args.beam
- else:
+ if args.beam_size:
+ beam_size = args.beam_size
+ elif args.use_fitted_beam:
bmajor = header["BMAJ"] * 3600 # [arcsec]
bminor = header["BMIN"] * 3600 # [arcsec]
- beam = np.pi * bmajor*bminor / (4*np.log(2)) # [arcsec^2]
+ beam_size = np.pi * bmajor*bminor / (4*np.log(2)) # [arcsec^2]
print("Beam: (%.2f, %.2f) [arcsec]" % (bmajor, bminor))
- print("Beam size: %.2f [arcsec^2]" % beam)
+ else:
+ # Derive beam size using 'WSCNORMF' keyword
+ beam_size = calc_beam_size(header)
+ print("Beam size: %.2f [arcsec^2]" % beam_size)
- equiv = au.brightness_temperature(beam*au.arcsec**2, freq*au.MHz)
+ equiv = au.brightness_temperature(beam_size*au.arcsec**2, freq*au.MHz)
jybeam2k = au.Unit(unit).to(au.K, equivalencies=equiv)
print("Conversion factor [%s/beam] -> [K]: %g" % (unit, jybeam2k))