本文整理汇总了Python中astropy.nddata.ccddata.CCDData类的典型用法代码示例。如果您正苦于以下问题:Python CCDData类的具体用法?Python CCDData怎么用?Python CCDData使用的例子?那么, 这里精选的类代码示例或许可以为您提供帮助。
在下文中一共展示了CCDData类的15个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: ccd_data
def ccd_data(request):
"""
Return a CCDData object with units of ADU.
The size of the data array is 100x100 but can be changed using the marker
@pytest.mark.data_size(N) on the test function, where N should be the
desired dimension.
Data values are initialized to random numbers drawn from a normal
distribution with mean of 0 and scale 1.
The scale can be changed with the marker @pytest.marker.scale(s) on the
test function, where s is the desired scale.
The mean can be changed with the marker @pytest.marker.scale(m) on the
test function, where m is the desired mean.
"""
size = value_from_markers('data_size', request)
scale = value_from_markers('data_scale', request)
mean = value_from_markers('data_mean', request)
with NumpyRNGContext(DEFAULTS['seed']):
data = np.random.normal(loc=mean, size=[size, size], scale=scale)
fake_meta = {'my_key': 42, 'your_key': 'not 42'}
ccd = CCDData(data, unit=u.adu)
ccd.header = fake_meta
return ccd
示例2: test_read_old_style_multiextensionfits
def test_read_old_style_multiextensionfits(tmpdir):
# Regression test for https://github.com/astropy/ccdproc/issues/664
#
# Prior to astropy 3.1 there was no uncertainty type saved
# in the multiextension fits files generated by CCDData
# because the uncertainty had to be StandardDevUncertainty.
#
# Current version should be able to read those in.
#
size = 4
# Value of the variables below are not important to the test.
data = np.zeros([size, size])
mask = data > 0.9
uncert = np.sqrt(data)
ccd = CCDData(data=data, mask=mask, uncertainty=uncert, unit='adu')
# We'll create the file manually to ensure we have the
# right extension names and no uncertainty type.
hdulist = ccd.to_hdu()
del hdulist[2].header['UTYPE']
file_name = tmpdir.join('old_ccddata_mef.fits').strpath
hdulist.writeto(file_name)
ccd = CCDData.read(file_name)
assert isinstance(ccd.uncertainty, StdDevUncertainty)
示例3: test_initialize_from_fits_with_invalid_unit_in_header
def test_initialize_from_fits_with_invalid_unit_in_header(tmpdir):
hdu = fits.PrimaryHDU(np.ones((2, 2)))
hdu.header['bunit'] = 'definetely-not-a-unit'
filename = tmpdir.join('afile.fits').strpath
hdu.writeto(filename)
with pytest.raises(ValueError):
CCDData.read(filename)
示例4: test_arithmetic_subtract_with_array
def test_arithmetic_subtract_with_array():
ccd = CCDData(np.ones((3, 3)), unit='')
res = ccd.subtract(np.arange(3))
np.testing.assert_array_equal(res.data, [[1, 0, -1]] * 3)
ccd = CCDData(np.ones((3, 3)), unit='adu')
with pytest.raises(ValueError):
ccd.subtract(np.arange(3))
示例5: test_wcs_attribute
def test_wcs_attribute(ccd_data, tmpdir):
"""
Check that WCS attribute gets added to header, and that if a CCDData
object is created from a FITS file with a header, and the WCS attribute
is modified, then the CCDData object is turned back into an hdu, the
WCS object overwrites the old WCS information in the header.
"""
tmpfile = tmpdir.join('temp.fits')
# This wcs example is taken from the astropy.wcs docs.
wcs = WCS(naxis=2)
wcs.wcs.crpix = np.array(ccd_data.shape) / 2
wcs.wcs.cdelt = np.array([-0.066667, 0.066667])
wcs.wcs.crval = [0, -90]
wcs.wcs.ctype = ["RA---AIR", "DEC--AIR"]
wcs.wcs.set_pv([(2, 1, 45.0)])
ccd_data.header = ccd_data.to_hdu()[0].header
ccd_data.header.extend(wcs.to_header(), useblanks=False)
ccd_data.write(tmpfile.strpath)
# Get the header length after it has been extended by the WCS keywords
original_header_length = len(ccd_data.header)
ccd_new = CCDData.read(tmpfile.strpath)
# WCS attribute should be set for ccd_new
assert ccd_new.wcs is not None
# WCS attribute should be equal to wcs above.
assert ccd_new.wcs.wcs == wcs.wcs
# Converting CCDData object with wcs to an hdu shouldn't
# create duplicate wcs-related entries in the header.
ccd_new_hdu = ccd_new.to_hdu()[0]
assert len(ccd_new_hdu.header) == original_header_length
# Making a CCDData with WCS (but not WCS in the header) should lead to
# WCS information in the header when it is converted to an HDU.
ccd_wcs_not_in_header = CCDData(ccd_data.data, wcs=wcs, unit="adu")
hdu = ccd_wcs_not_in_header.to_hdu()[0]
wcs_header = wcs.to_header()
for k in wcs_header.keys():
# Skip these keywords if they are in the WCS header because they are
# not WCS-specific.
if k in ['', 'COMMENT', 'HISTORY']:
continue
# No keyword from the WCS should be in the header.
assert k not in ccd_wcs_not_in_header.header
# Every keyword in the WCS should be in the header of the HDU
assert hdu.header[k] == wcs_header[k]
# Now check that if WCS of a CCDData is modified, then the CCDData is
# converted to an HDU, the WCS keywords in the header are overwritten
# with the appropriate keywords from the header.
#
# ccd_new has a WCS and WCS keywords in the header, so try modifying
# the WCS.
ccd_new.wcs.wcs.cdelt *= 2
ccd_new_hdu_mod_wcs = ccd_new.to_hdu()[0]
assert ccd_new_hdu_mod_wcs.header['CDELT1'] == ccd_new.wcs.wcs.cdelt[0]
assert ccd_new_hdu_mod_wcs.header['CDELT2'] == ccd_new.wcs.wcs.cdelt[1]
示例6: test_header2meta
def test_header2meta():
hdr = fits.header.Header()
hdr['observer'] = 'Edwin Hubble'
hdr['exptime'] = '3600'
d1 = CCDData(np.ones((5, 5)), unit=u.electron)
d1.header = hdr
assert d1.meta['OBSERVER'] == 'Edwin Hubble'
assert d1.header['OBSERVER'] == 'Edwin Hubble'
示例7: test_arithmetic_with_wcs_compare
def test_arithmetic_with_wcs_compare():
def return_diff_smaller_3(first, second):
return abs(first - second) <= 3
ccd1 = CCDData(np.ones((10, 10)), unit='', wcs=2)
ccd2 = CCDData(np.ones((10, 10)), unit='', wcs=5)
assert ccd1.add(ccd2, compare_wcs=return_diff_smaller_3).wcs == 2
assert ccd1.subtract(ccd2, compare_wcs=return_diff_smaller_3).wcs == 2
assert ccd1.multiply(ccd2, compare_wcs=return_diff_smaller_3).wcs == 2
assert ccd1.divide(ccd2, compare_wcs=return_diff_smaller_3).wcs == 2
示例8: test_initialize_from_FITS_bad_keyword_raises_error
def test_initialize_from_FITS_bad_keyword_raises_error(ccd_data, tmpdir):
# There are two fits.open keywords that are not permitted in ccdproc:
# do_not_scale_image_data and scale_back
filename = tmpdir.join('test.fits').strpath
ccd_data.write(filename)
with pytest.raises(TypeError):
CCDData.read(filename, unit=ccd_data.unit,
do_not_scale_image_data=True)
with pytest.raises(TypeError):
CCDData.read(filename, unit=ccd_data.unit, scale_back=True)
示例9: test_fromMEF
def test_fromMEF(ccd_data, tmpdir):
hdu = fits.PrimaryHDU(ccd_data)
hdu2 = fits.PrimaryHDU(2 * ccd_data.data)
hdulist = fits.HDUList(hdu)
hdulist.append(hdu2)
filename = tmpdir.join('afile.fits').strpath
hdulist.writeto(filename)
# by default, we reading from the first extension
cd = CCDData.read(filename, unit=u.electron)
np.testing.assert_array_equal(cd.data, ccd_data.data)
# but reading from the second should work too
cd = CCDData.read(filename, hdu=1, unit=u.electron)
np.testing.assert_array_equal(cd.data, 2 * ccd_data.data)
示例10: test_initialize_from_fits_with_unit_in_header
def test_initialize_from_fits_with_unit_in_header(tmpdir):
fake_img = np.random.random(size=(100, 100))
hdu = fits.PrimaryHDU(fake_img)
hdu.header['bunit'] = u.adu.to_string()
filename = tmpdir.join('afile.fits').strpath
hdu.writeto(filename)
ccd = CCDData.read(filename)
# ccd should pick up the unit adu from the fits header...did it?
assert ccd.unit is u.adu
# An explicit unit in the read overrides any unit in the FITS file
ccd2 = CCDData.read(filename, unit="photon")
assert ccd2.unit is u.photon
示例11: test_wcs_sip_handling
def test_wcs_sip_handling():
"""
Check whether the ctypes RA---TAN-SIP and DEC--TAN-SIP survive
a roundtrip unchanged.
"""
data_file = get_pkg_data_filename('data/sip-wcs.fits')
def check_wcs_ctypes(header):
expected_wcs_ctypes = {
'CTYPE1': 'RA---TAN-SIP',
'CTYPE2': 'DEC--TAN-SIP'
}
return [header[k] == v for k, v in expected_wcs_ctypes.items()]
ccd_original = CCDData.read(data_file)
# After initialization the keywords should be in the WCS, not in the
# meta.
with fits.open(data_file) as raw:
good_ctype = check_wcs_ctypes(raw[0].header)
assert all(good_ctype)
ccd_new = ccd_original.to_hdu()
good_ctype = check_wcs_ctypes(ccd_new[0].header)
assert all(good_ctype)
# Try converting to header with wcs_relax=False and
# the header should contain the CTYPE keywords without
# the -SIP
ccd_no_relax = ccd_original.to_hdu(wcs_relax=False)
good_ctype = check_wcs_ctypes(ccd_no_relax[0].header)
assert not any(good_ctype)
assert ccd_no_relax[0].header['CTYPE1'] == 'RA---TAN'
assert ccd_no_relax[0].header['CTYPE2'] == 'DEC--TAN'
示例12: test_wcs_keywords_removed_from_header
def test_wcs_keywords_removed_from_header():
"""
Test, for the file included with the nddata tests, that WCS keywords are
properly removed from header.
"""
from astropy.nddata.ccddata import _KEEP_THESE_KEYWORDS_IN_HEADER
keepers = set(_KEEP_THESE_KEYWORDS_IN_HEADER)
data_file = get_pkg_data_filename('data/sip-wcs.fits')
ccd = CCDData.read(data_file)
wcs_header = ccd.wcs.to_header()
assert not (set(wcs_header) & set(ccd.meta) - keepers)
# Make sure that exceptions are not raised when trying to remove missing
# keywords. o4sp040b0_raw.fits of io.fits is missing keyword 'PC1_1'.
data_file1 = get_pkg_data_filename('../../io/fits/tests/data/o4sp040b0_raw.fits')
ccd = CCDData.read(data_file1, unit='count')
示例13: test_wcs_SIP_coefficient_keywords_removed
def test_wcs_SIP_coefficient_keywords_removed():
# If SIP polynomials are present, check that no more polynomial
# coefficients remain in the header. See #8598
# The SIP paper is ambiguous as to whether keywords like
# A_0_0 can appear in the header for a 2nd order or higher
# polynomial. The paper clearly says that the corrections
# are only for quadratic or higher order, so A_0_0 and the like
# should be zero if they are present, but they apparently can be
# there (or at least astrometry.net produces them).
# astropy WCS does not write those coefficients, so they were
# not being removed from the header even though they are WCS-related.
data_file = get_pkg_data_filename('data/sip-wcs.fits')
# Make sure the keywords added to this file for testing are there
hdu = fits.open(data_file)
test_keys = ['A_0_0', 'B_0_1']
for key in test_keys:
assert key in hdu[0].header
ccd = CCDData.read(data_file)
# Now the test...the two keywords above should have been removed.
for key in test_keys:
assert key not in ccd.header
示例14: test_infol_logged_if_unit_in_fits_header
def test_infol_logged_if_unit_in_fits_header(ccd_data, tmpdir):
tmpfile = tmpdir.join('temp.fits')
ccd_data.write(tmpfile.strpath)
log.setLevel('INFO')
explicit_unit_name = "photon"
with log.log_to_list() as log_list:
ccd_from_disk = CCDData.read(tmpfile.strpath, unit=explicit_unit_name)
assert explicit_unit_name in log_list[0].message
示例15: test_write_read_multiextensionfits_mask_default
def test_write_read_multiextensionfits_mask_default(ccd_data, tmpdir):
# Test that if a mask is present the mask is saved and loaded by default.
ccd_data.mask = ccd_data.data > 10
filename = tmpdir.join('afile.fits').strpath
ccd_data.write(filename)
ccd_after = CCDData.read(filename)
assert ccd_after.mask is not None
np.testing.assert_array_equal(ccd_data.mask, ccd_after.mask)