本文整理汇总了Python中astropy.io.fits.open方法的典型用法代码示例。如果您正苦于以下问题:Python fits.open方法的具体用法?Python fits.open怎么用?Python fits.open使用的例子?那么, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类astropy.io.fits
的用法示例。
在下文中一共展示了fits.open方法的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: __init__
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def __init__(self, base_fname):
"""
Args:
base_fname (str): The map should be stored in two FITS files, named
``base_fname + '_' + X + '.fits'``, where ``X`` is ``'ngp'`` and
``'sgp'``.
"""
self._data = {}
for pole in self.poles:
fname = '{}_{}.fits'.format(base_fname, pole)
try:
with fits.open(fname) as hdulist:
self._data[pole] = [hdulist[0].data, wcs.WCS(hdulist[0].header)]
except IOError as error:
print(dustexceptions.data_missing_message(self.map_name,
self.map_name_long))
raise error
示例2: parse_input_healpix_data
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def parse_input_healpix_data(input_data, field=0, hdu_in=None, nested=None):
"""
Parse input HEALPIX data to return a Numpy array and coordinate frame object.
"""
if isinstance(input_data, (TableHDU, BinTableHDU)):
data = input_data.data
header = input_data.header
coordinate_system_in = parse_coord_system(header['COORDSYS'])
array_in = data[data.columns[field].name].ravel()
if 'ORDERING' in header:
nested = header['ORDERING'].lower() == 'nested'
elif isinstance(input_data, str):
hdu = fits.open(input_data)[hdu_in or 1]
return parse_input_healpix_data(hdu, field=field)
elif isinstance(input_data, tuple) and isinstance(input_data[0], np.ndarray):
array_in = input_data[0]
coordinate_system_in = parse_coord_system(input_data[1])
else:
raise TypeError("input_data should either be an HDU object or a tuple of (array, frame)")
return array_in, coordinate_system_in, nested
示例3: main
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def main(infile, xypadsize):
"""Pad a fits image with zeros to padsize"""
pad_xsize, pad_ysize = [int(s) for s in xypadsize.split(' ')]
hdu = pyfits.open(infile)
imdata = hdu[0].data[0, 0]
(ysize, xsize) = imdata.shape
if xsize > pad_xsize or ysize > pad_ysize:
raise ValueError('pad_image: padded size is smaller than current size!')
if xsize == pad_xsize and ysize == pad_ysize:
return()
xoffset = (pad_xsize - xsize) / 2
yoffset = (pad_ysize - ysize) / 2
newdata=np.zeros((1, 1, pad_ysize, pad_xsize))
newdata[0, 0, yoffset:yoffset+ysize, xoffset:xoffset+xsize] = imdata
hdu[0].data = newdata
hdu[0].header['CRPIX1'] += xoffset
hdu[0].header['CRPIX2'] += yoffset
hdu.writeto(infile, clobber=True)
示例4: load_allstar_dr5
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def load_allstar_dr5():
"""
Open LAMOST DR5 allstar
:return: fits file opened by astropy
:rtype: astropy.io.fits.hdu.hdulist.HDUList
:History: 2018-Jun-17 - Written - Henry Leung (University of Toronto)
"""
import os
from astropy.io import fits
file_name = "LAMO5_2MS_AP9_SD14_UC4_PS1_AW_Carlin_M.fits"
_lamost_dr5_allsta_path = os.path.join(lamost_env(), "DR5", file_name)
if not os.path.isfile(_lamost_dr5_allsta_path):
raise FileNotFoundError(f'{file_name} file not found')
return fits.open(_lamost_dr5_allsta_path)
示例5: test_frame_type_invalid
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_frame_type_invalid(self) -> None:
with fits.open(self.fitsfile) as hdulist:
hdulist[10].header['ESO DET FRAM TYPE'] = 'Test'
hdulist.writeto(self.fitsfile, overwrite=True)
module = NearReadingModule(name_in='read5',
input_dir=self.test_dir+'near',
chopa_out_tag=self.positions[0],
chopb_out_tag=self.positions[1])
self.pipeline.add_module(module)
with pytest.raises(ValueError) as error:
self.pipeline.run_module('read5')
assert str(error.value) == 'Frame type (Test) not a valid value. Expecting HCYCLE1 or ' \
'HCYCLE2 as value for ESO DET FRAM TYPE.'
示例6: test_frame_type_missing
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_frame_type_missing(self) -> None:
with fits.open(self.fitsfile) as hdulist:
hdulist[10].header.remove('ESO DET FRAM TYPE')
hdulist.writeto(self.fitsfile, overwrite=True)
module = NearReadingModule(name_in='read6',
input_dir=self.test_dir+'near',
chopa_out_tag=self.positions[0],
chopb_out_tag=self.positions[1])
self.pipeline.add_module(module)
with pytest.raises(ValueError) as error:
self.pipeline.run_module('read6')
assert str(error.value) == 'Frame type not found in the FITS header. Image number: 9.'
示例7: test_odd_number_images
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_odd_number_images(self) -> None:
with fits.open(self.fitsfile) as hdulist:
del hdulist[11]
hdulist.writeto(self.fitsfile, overwrite=True)
module = NearReadingModule(name_in='read8',
input_dir=self.test_dir+'near',
chopa_out_tag=self.positions[0],
chopb_out_tag=self.positions[1])
self.pipeline.add_module(module)
with pytest.warns(UserWarning) as warning:
self.pipeline.run_module('read8')
assert len(warning) == 2
assert warning[0].message.args[0] == f'FITS file contains odd number of images: ' \
f'{self.fitsfile}'
assert warning[1].message.args[0] == 'The number of chop cycles (5) is not equal to ' \
'half the number of available HDU images (4).'
示例8: test_header_attribute
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_header_attribute(self) -> None:
with fits.open(self.test_dir+'fits/images_0.fits') as hdu:
header = hdu[0].header
header['PARANG'] = 1.0
hdu.writeto(self.test_dir+'fits/images_0.fits', overwrite=True)
with fits.open(self.test_dir+'fits/images_1.fits') as hdu:
header = hdu[0].header
header['PARANG'] = 2.0
header['HIERARCH ESO DET DIT'] = 0.1
hdu.writeto(self.test_dir+'fits/images_1.fits', overwrite=True)
module = FitsReadingModule(name_in='read5',
input_dir=self.test_dir+'fits',
image_tag='input',
overwrite=True,
check=True)
self.pipeline.add_module(module)
self.pipeline.run_module('read5')
示例9: test_fits_read_textfile_exists
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_fits_read_textfile_exists(self) -> None:
with open(self.test_dir+'filenames.dat', 'w') as file_obj:
file_obj.write(self.test_dir+'fits/images_0.fits\n')
file_obj.write(self.test_dir+'fits/images_2.fits\n')
module = FitsReadingModule(name_in='read10',
input_dir=None,
image_tag='files',
overwrite=True,
check=True,
filenames=self.test_dir+'filenames.dat')
self.pipeline.add_module(module)
with pytest.raises(ValueError) as error:
self.pipeline.run_module('read10')
assert str(error.value) == f'The file {self.test_dir}fits/images_2.fits does not exist. ' \
f'Please check that the path is correct.'
示例10: load_spectrum
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def load_spectrum(filename, grid):
"""
Load a single spectrum
"""
file_in = pyfits.open(filename)
wl = np.array(file_in[0].data[2])
flux = np.array(file_in[0].data[0])
ivar = np.array((file_in[0].data[1]))
# correct for radial velocity of star
redshift = file_in[0].header['Z']
wl_shifted = wl - redshift * wl
# resample
flux_rs = (interpolate.interp1d(wl_shifted, flux))(grid)
ivar_rs = (interpolate.interp1d(wl_shifted, ivar))(grid)
ivar_rs[ivar_rs < 0] = 0. # in interpolating you can end up with neg
return flux_rs, ivar_rs
示例11: test_fine_channels
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_fine_channels(tmp_path):
"""
Break read_mwa_corr_fits by submitting files with different fine channels.
Test that error is raised if files with different numbers of fine channels
are submitted.
"""
mwa_uv = UVData()
bad_fine = str(tmp_path / "bad_gpubox06_01.fits")
with fits.open(filelist[2]) as mini6:
mini6[1].data = np.concatenate((mini6[1].data, mini6[1].data))
mini6.writeto(bad_fine)
with pytest.raises(ValueError) as cm:
mwa_uv.read([bad_fine, filelist[1]])
assert str(cm.value).startswith("files submitted have different fine")
del mwa_uv
示例12: test_diff_obs
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def test_diff_obs(tmp_path):
"""
Break read_mwa_corr_fits by submitting files from different observations.
Test that error is raised if files from different observations are
submitted in the same file list.
"""
mwa_uv = UVData()
bad_obs = str(tmp_path / "bad2_gpubox06_01.fits")
with fits.open(filelist[2]) as mini6:
mini6[0].header["OBSID"] = "1131733555"
mini6.writeto(bad_obs)
with pytest.raises(ValueError) as cm:
mwa_uv.read([bad_obs, filelist[0], filelist[1]])
assert str(cm.value).startswith("files from different observations")
del mwa_uv
示例13: find_fits_img_size
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def find_fits_img_size(filename):
"""
Returns the size of a FITS image, given a valid FITS image file
:param filename: The fully-qualified path of the FITS image file
:type filename: str
:returns: Tuple of horizontal/vertical dimensions
:rtype: tuple
"""
try:
return settings.THUMBNAIL_MAX_SIZE
except AttributeError:
hdul = fits.open(filename)
xsize = 0
ysize = 0
for hdu in hdul:
try:
xsize = max(xsize, hdu.header['NAXIS1'])
ysize = max(ysize, hdu.header['NAXIS2'])
except KeyError:
pass
return (xsize, ysize)
示例14: is_fits_image_file
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def is_fits_image_file(file):
"""
Checks if a file is a valid FITS image by checking if any header contains 'SCI' in the 'EXTNAME'.
:param file: The file to be checked.
:type file:
:returns: True if the file is a FITS image, False otherwise
:rtype: boolean
"""
with file.open() as f:
try:
hdul = fits.open(f)
except OSError: # OSError is raised if file is not FITS format
return False
for hdu in hdul:
if hdu.header.get('EXTNAME') == 'SCI':
return True
return False
示例15: add_all_spectra
# 需要导入模块: from astropy.io import fits [as 别名]
# 或者: from astropy.io.fits import open [as 别名]
def add_all_spectra():
from grizli.aws import db as grizli_db
roots = grizli_db.from_sql("select root,count(root) as n from redshift_fit group BY root order by n DESC", engine)
o = 1
for root in roots['root'][::o]:
existing = open('log').readlines()
if root+'\n' in existing:
print('Skip', root)
continue
fp = open('log', 'a')
fp.write(root+'\n')
fp.close()
try:
grizli_db.add_oned_spectra(root=root, engine=engine)
except:
pass