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August 29, 2015 14:11
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Test showing that non fixed scale results different photometric flux depending on the number of positions
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from astropy.io import fits | |
from astropy.wcs import WCS | |
import numpy as np | |
import astropy.units as u | |
from photutils import SkyCircularAperture, aperture_photometry | |
from photutils.extern.wcs_utils import pixel_to_skycoord | |
image_shape = (100, 200) | |
header = WCS({'CTYPE1': 'RA---TAN', | |
'CTYPE2': 'DEC--TAN', | |
'CRPIX1': int(image_shape[1] / 2), | |
'CRPIX2': int(image_shape[0] / 2)}, ).to_header() | |
hdu = fits.ImageHDU(np.ones(image_shape), header=header) | |
pos_p = u.Quantity(([150., 20., 150., 150.], | |
[65., 20., 6., 35.]), unit=u.pixel) | |
pos_p_s = u.Quantity(([150., ], [65., ]), unit=u.pixel) | |
pos = pixel_to_skycoord(pos_p[0], pos_p[1], WCS(hdu.header)) | |
pos_s = pixel_to_skycoord(pos_p_s[0], pos_p_s[1], WCS(hdu.header)) | |
photometry_skycoord_circ = aperture_photometry( | |
hdu, SkyCircularAperture(pos, 3 * u.deg)) | |
photometry_skycoord_circ_s = aperture_photometry( | |
hdu, SkyCircularAperture(pos_s, 3 * u.deg)) | |
print photometry_skycoord_circ | |
print photometry_skycoord_circ_s |
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